Unformatted text preview: Instructor Solutions Manual for Physics by Halliday, Resnick, and Krane
Paul Stanley Beloit College Volume 2
A Note To The Instructor...
The solutions here are somewhat brief, as they are designed for the instructor, not for the student. Check with the publishers before electronically posting any part of these solutions; website, ftp, or server access must be restricted to your students. I have been somewhat casual about subscripts whenever it is obvious that a problem is one dimensional, or that the choice of the coordinate system is irrelevant to the numerical solution. Although this does not change the validity of the answer, it will sometimes obfuscate the approach if viewed by a novice. There are some traditional formula, such as
2 2 vx = v0x + 2ax x,
which are not used in the text. The worked solutions use only material from the text, so there may be times when the solution here seems unnecessarily convoluted and drawn out. Yes, I know an easier approach existed. But if it was not in the text, I did not use it here. I also tried to avoid reinventing the wheel. There are some exercises and problems in the text which build upon previous exercises and problems. Instead of rederiving expressions, I simply refer you to the previous solution. I adopt a different approach for rounding of significant figures than previous authors; in particular, I usually round intermediate answers. As such, some of my answers will differ from those in the back of the book. Exercises and Problems which are enclosed in a box also appear in the Student's Solution Manual with considerably more detail and, when appropriate, include discussion on any physical implications of the answer. These student solutions carefully discuss the steps required for solving problems, point out the relevant equation numbers, or even specify where in the text additional information can be found. When two almost equivalent methods of solution exist, often both are presented. You are encouraged to refer students to the Student's Solution Manual for these exercises and problems. However, the material from the Student's Solution Manual must not be copied. Paul Stanley Beloit College stanley@clunet.edu
1
E251
The charge transferred is Q = (2.5 104 C/s)(20 106 s) = 5.0 101 C.
E252 Use Eq. 254: r= E253 Use Eq. 254: F = (8.99109 Nm2 /C2 )(3.12106 C)(1.48106 C) = 2.74 N. (0.123 m)2 (8.99109 Nm2 /C2 )(26.3106 C)(47.1106 C) = 1.40 m (5.66 N)
E254 (a) The forces are equal, so m1 a1 = m2 a2 , or m2 = (6.31107 kg)(7.22 m/s2 )/(9.16 m/s2 ) = 4.97107 kg. (b) Use Eq. 254: q= (6.31107 kg)(7.22 m/s2 )(3.20103 m)2 = 7.201011 C (8.99109 Nm2 /C2 )
E255
(a) Use Eq. 254, F = 1 q1 q2 1 (21.3 C)(21.3 C) = = 1.77 N 2 12 C2 /N m2 ) 4 0 r12 4(8.8510 (1.52 m)2
(b) In part (a) we found F12 ; to solve part (b) we need to first find F13 . Since q3 = q2 and r13 = r12 , we can immediately conclude that F13 = F12 . We must assess the direction of the force of q3 on q1 ; it will be directed along the line which connects the two charges, and will be directed away from q3 . The diagram below shows the directions.
F
23
F 12 F 23 F net
F 12
From this diagram we want to find the magnitude of the net force on q1 . The cosine law is appropriate here: F net 2
2 2 = F12 + F13  2F12 F13 cos , 2 = (1.77 N) + (1.77 N)2  2(1.77 N)(1.77 N) cos(120 ), = 9.40 N2 , = 3.07 N.
F net
2
E256 Originally F0 = CQ2 = 0.088 N, where C is a constant. When sphere 3 touches 1 the 0 charge on both becomes Q0 /2. When sphere 3 the touches sphere 2 the charge on each becomes (Q0 + Q0 /2)/2 = 3Q0 /4. The force between sphere 1 and 2 is then F = C(Q0 /2)(3Q0 /4) = (3/8)CQ2 = (3/8)F0 = 0.033 N. 0 E257 The forces on q3 are F31 and F32 . These forces are given by the vector form of Coulomb's Law, Eq. 255, F31 F32 = = 1 q3 q1 1 q3 q1 ^ ^ , r 2 r31 = 4 2 31 4 0 r31 0 (2d) 1 q3 q2 1 q3 q2 ^ ^ . r 2 r32 = 4 2 32 4 0 r32 0 (d)
These two forces are the only forces which act on q3 , so in order to have q3 in equilibrium the forces must be equal in magnitude, but opposite in direction. In short, F31 1 q3 q1 ^31 r 4 0 (2d)2 q1 ^31 r 4 = F32 , 1 q3 q2 ^32 , =  r 4 0 (d)2 q2 =  ^32 . r 1
Note that ^31 and ^32 both point in the same direction and are both of unit length. We then get r r q1 = 4q2 . E258 The horizontal and vertical contributions from the upper left charge and lower right charge are straightforward to find. The contributions from the upper left charge require slightly more work. The diagonal distance is 2a; the components will be weighted by cos 45 = 2/2. The diagonal charge will contribute 1 (q)(2q) 2^ 2 q2 ^ Fx = i= i, 4 0 ( 2a)2 2 8 0 a2 1 (q)(2q) 2 ^ 2 q2 ^ Fy = j= j. 4 0 ( 2a)2 2 8 0 a2 (a) The horizontal component of the net force is then 1 (2q)(2q)^ 2 q2 ^ Fx = i+ i, 4 0 a2 8 0 a2 4 + 2/2 q 2 ^ = i, 4 0 a2 = (4.707)(8.99109 N m2 /C2 )(1.13106 C)2 /(0.152 m)2^ = 2.34 N ^ i i.
(b) The vertical component of the net force is then 1 (q)(2q) ^ 2 q2 ^ j+ j, Fy =  2 4 0 a 8 0 a2 2 + 2/2 q 2 ^ = j, 8 0 a2 = (1.293)(8.99109 N m2 /C2 )(1.13106 C)2 /(0.152 m)2^ = 0.642 N ^ j j. 3
E259 The magnitude of the force on the negative charge from each positive charge is F = (8.99109 N m2 /C2 )(4.18106 C)(6.36106 C)/(0.13 m)2 = 14.1 N. The force from each positive charge is directed along the side of the triangle; but from symmetry only the component along the bisector is of interest. This means that we need to weight the above answer by a factor of 2 cos(30 ) = 1.73. The net force is then 24.5 N. E2510 Let the charge on one sphere be q, then the charge on the other sphere is Q = (52.6 106 C)  q. Then 1 qQ = F, 4 0 r2 (8.99109 Nm2 /C2 )q(52.6106 C  q) = (1.19 N)(1.94 m)2 . Solve this quadratic expression for q and get answers q1 = 4.02105 C and q2 = 1.24106 N. E2511 This problem is similar to Ex. 257. There are some additional issues, however. It is easy enough to write expressions for the forces on the third charge F31 F32 Then F31 1 q3 q1 ^ 2 r31 4 0 r31 q1 ^ 2 r31 r31 = F32 , 1 q3 q2 ^ =  2 r32 , 4 0 r32 q2 =  2 ^32 . r r32 = = 1 q3 q1 ^ 2 r31 , 4 0 r31 1 q3 q2 ^ 2 r32 . 4 0 r32
The only way to satisfy the vector nature of the above expression is to have ^31 = ^32 ; this means r r that q3 must be collinear with q1 and q2 . q3 could be between q1 and q2 , or it could be on either side. Let's resolve this issue now by putting the values for q1 and q2 into the expression: (1.07 C) ^31 r 2 r31
2 r32 ^31 r
= 
(3.28 C) ^32 , r 2 r32
2 = (3.07)r31 ^32 . r
Since squared quantities are positive, we can only get this to work if ^31 = ^32 , so q3 is not between r r q1 and q2 . We are then left with 2 2 r32 = (3.07)r31 , so that q3 is closer to q1 than it is to q2 . Then r32 = r31 + r12 = r31 + 0.618 m, and if we take the square root of both sides of the above expression, r31 + (0.618 m) = (3.07)r31 ,
(0.618 m) = (3.07)r31  r31 , (0.618 m) = 0.752r31 , 0.822 m = r31 4
E2512 The magnitude of the magnetic force between any two charges is kq 2 /a2 , where a = 0.153 m. The force between each charge is directed along the side of the triangle; but from symmetry only the component along the bisector is of interest. This means that we need to weight the above answer by a factor of 2 cos(30 ) = 1.73. The net force on any charge is then 1.73kq 2 /a2 . The length of the angle bisector, d, is given by d = a cos(30 ). The distance from any charge to the center of the equilateral triangle is x, given by x2 = (a/2)2 + (d  x)2 . Then x = a2 /8d + d/2 = 0.644a. The angle between the strings and the plane of the charges is , given by sin = x/(1.17 m) = (0.644)(0.153 m)/(1.17 m) = 0.0842, or = 4.83 . The force of gravity on each ball is directed vertically and the electric force is directed horizontally. The two must then be related by tan = F E /F G , so 1.73(8.99109 N m2 /C2 )q 2 /(0.153 m)2 = (0.0133 kg)(9.81 m/s2 ) tan(4.83 ), or q = 1.29107 C. E2513 On any corner charge there are seven forces; one from each of the other seven charges. The net force will be the sum. Since all eight charges are the same all of the forces will be repulsive. We need to sketch a diagram to show how the charges are labeled.
2 6 4
1
7
3
8
The magnitude of the force of charge 2 on charge 1 is F12 = 1 q2 2 , 4 0 r12
5
where r12 = a, the length of a side. Since both charges are the same we wrote q 2 . By symmetry we expect that the magnitudes of F12 , F13 , and F14 will all be the same and they will all be at right angles to each other directed along the edges of the cube. Written in terms of vectors the forces
5
would be F12 F13 F14 The force from charge 5 is 1 q2 2 , 4 0 r15 and is directed along the side diagonal away from charge 5. The distance r15 is also the side diagonal distance, and can be found from 2 r15 = a2 + a2 = 2a2 , F15 = then 1 q2 . 4 0 2a2 By symmetry we expect that the magnitudes of F15 , F16 , and F17 will all be the same and they will all be directed along the diagonals of the faces of the cube. In terms of components we would have F15 = F15 F16 F17 = = = 1 q2 4 0 2a2 1 q2 4 0 2a2 1 q2 4 0 2a2 ^ ^ 2 + k/ 2 , j/ ^ 2 + k/ 2 , ^ i/ ^ 2 +^ 2 . i/ j/ = = = 1 q2 ^ i, 4 0 a2 1 q2 ^ j, 4 0 a2 1 q2 ^ k. 4 0 a2
The last force is the force from charge 8 on charge 1, and is given by F18 = 1 q2 2 , 4 0 r18
and is directed along the cube diagonal away from charge 8. The distance r18 is also the cube diagonal distance, and can be found from
2 r18 = a2 + a2 + a2 = 3a2 ,
then in term of components F18 = 1 q2 ^ ^ i/ 3 + ^ 3 + k/ 3 . j/ 2 4 0 3a
We can add the components together. By symmetry we expect the same answer for each components, so we'll just do one. How about ^ This component has contributions from charge 2, 6, 7, i. and 8: 1 1 q2 1 2 , + + 2 4 0 a 1 2 2 3 3 or 1 q2 (1.90) 4 0 a2 The three components add according to Pythagoras to pick up a final factor of 3, so F net = (0.262) q2 . 2 0a
6
E2514 (a) Yes. Changing the sign of y will change the sign of Fy ; since this is equivalent to putting the charge q0 on the "other" side, we would expect the force to also push in the "other" direction. (b) The equation should look Eq. 2515, except all y's should be replaced by x's. Then Fx = 1 q0 q . 4 0 x x2 + L2 /4
(c) Setting the particle a distance d away should give a force with the same magnitude as F = 1 4 0 d q0 q d2 + L2 /4 .
This force is directed along the 45 line, so Fx = F cos 45 and Fy = F sin 45 . (d) Let the distance be d = x2 + y 2 , and then use the fact that Fx /F = cos = x/d. Then Fx = F and Fy = F 1 x q0 q x = . 2 + y 2 + L2 /4)3/2 d 4 0 (x 1 y q0 q y = . 2 + y 2 + L2 /4)3/2 d 4 0 (x
E2515 (a) The equation is valid for both positive and negative z, so in vector form it would read ^ F = Fz k = 1 q0 q z ^ k. 4 0 (z 2 + R2 )3/2
(b) The equation is not valid for both positive and negative Reversing the sign of z should z. reverse the sign of Fz , and one way to fix this is to write 1 = z/ z 2 . Then ^ F = Fz k = 1 2q0 qz 4 0 R2 1 1  2 z z2 ^ k.
E2516 Divide the rod into small differential lengths dr, each with charge dQ = (Q/L)dr. Each differential length contributes a differential force dF = Integrate: F = = 1 qQ dr, 4 0 r2 L x 1 qQ 1 1  4 0 L x x + L dF =
x+L
1 q dQ 1 qQ = dr. 2 4 0 r 4 0 r2 L
E2517 You must solve Ex. 16 before solving this problem! q0 refers to the charge that had been called q in that problem. In either case the distance from q0 will be the same regardless of the sign of q; if q = Q then q will be on the right, while if q = Q then q will be on the left. Setting the forces equal to each other one gets 1 qQ 4 0 L or r= x(x + L). 7 1 1  x x+L = 1 qQ , 4 0 r2
E2518 You must solve Ex. 16 and Ex. 17 before solving this problem. If all charges are positive then moving q0 off axis will result in a net force away from the axis. That's unstable. If q = Q then both q and Q are on the same side of q0 . Moving q0 closer to q will result in the attractive force growing faster than the repulsive force, so q0 will move away from equilibrium. E2519 We can start with the work that was done for us on Page 577, except since we are concerned with sin = z/r we would have dFx = dF sin = 1 q0 dz 4 0 (y 2 + z 2 ) z y2 + z2 .
We will need to take into consideration that changes sign for the two halves of the rod. Then Fx = = = q0 4 0 q0 2 0 q0 2 0 q0 2 0
0 L/2 L/2 0
(y 2
z dz + + z 2 )3/2
L/2 0
+z dz (y 2 + z 2 )3/2
,
z dz , (y 2 + z 2 )3/2
L/2
1 y2 + z2 1  y y2
,
0
=
1 + (L/2)2
.
E2520 Use Eq. 2515 to find the magnitude of the force from any one rod, but write it as F = 1 4 0 r qQ r2 + L2 /4 ,
where r2 = z 2 + L2 /4. The component of this along the z axis is Fz = F z/r. Since there are 4 rods, we have 1 qQz 1 qQz F = ,= , 2 2 + L2 /4 2 + L2 /4) z 2 + L2 /2 0r r 0 (z Equating the electric force with the force of gravity and solving for Q, Q= putting in the numbers, (8.851012 C2 /Nm2 )(3.46107 kg)(9.8m/s2 ) ((0.214m)2+(0.25m)2 /4) (0.214m)2 +(0.25m)2 /2 (2.451012 C)(0.214 m) so Q = 3.07106 C. E2521 In each case we conserve charge by making sure that the total number of protons is the same on both sides of the expression. We also need to conserve the number of neutrons. (a) Hydrogen has one proton, Beryllium has four, so X must have five protons. Then X must be Boron, B. (b) Carbon has six protons, Hydrogen has one, so X must have seven. Then X is Nitrogen, N. (c) Nitrogen has seven protons, Hydrogen has one, but Helium has two, so X has 7 + 1  2 = 6 protons. This means X is Carbon, C. 8 0 mg 2 (z + L2 /4) z 2 + L2 /2; qz
E2522 (a) Use Eq. 254: F = (8.99109 Nm2 /C2 )(2)(90)(1.601019 C)2 = 290 N. (121015 m)2
(b) a = (290 N)/(4)(1.661027 kg) = 4.41028 m/s2 . E2523 Use Eq. 254: F = (8.99109 Nm2 /C2 )(1.601019 C)2 = 2.89109 N. (2821012 m)2
E2524 (a) Use Eq. 254: q= (3.7109 N)(5.01010 m)2 = 3.201019 C. (8.99109 Nm2 /C2 )
(b) N = (3.201019 C)/(1.601019 C) = 2. E2525 Use Eq. 254, F = ( 1 1.6 1019 C)( 1 1.6 1019 C) 1 q1 q2 3 3 = = 3.8 N. 2 4 0 r12 4(8.85 1012 C2 /N m2 )(2.6 1015 m)2
E2526 (a) N = (1.15107 C)/(1.601019 C) = 7.191011 . (b) The penny has enough electrons to make a total charge of 1.37105 C. The fraction is then (1.15107 C)/(1.37105 C) = 8.401013 . E2527 Equate the magnitudes of the forces: 1 q2 = mg, 4 0 r2 so r= (8.99109 Nm2 /C2 )(1.601019 C)2 = 5.07 m (9.111031 kg)(9.81 m/s2 )
E2528 Q = (75.0 kg)(1.601019 C)/(9.111031 kg) = 1.31013 C. E2529 The mass of water is (250 cm3 )(1.00 g/cm ) = 250 g. The number of moles of water is (250 g)/(18.0 g/mol) = 13.9 mol. The number of water molecules is (13.9 mol)(6.021023 mol1 ) = 8.371024 . Each molecule has ten protons, so the total positive charge is Q = (8.371024 )(10)(1.601019 C) = 1.34107 C. E2530 The total positive charge in 0.250 kg of water is 1.34107 C. Mary's imbalance is then q1 = (52.0)(4)(1.34107 C)(0.0001) = 2.79105 C, while John's imbalance is q2 = (90.7)(4)(1.34107 C)(0.0001) = 4.86105 C, The electrostatic force of attraction is then 1 q1 q2 (2.79105 )(4.86105 ) F = = (8.99109 N m2 /C2 ) = 1.61018 N. 4 0 r2 (28.0 m)2 9
3
E2531
(a) The gravitational force of attraction between the Moon and the Earth is FG = GM E M M , R2
where R is the distance between them. If both the Earth and the moon are provided a charge q, then the electrostatic repulsion would be FE = 1 q2 . 4 0 R2
Setting these two expression equal to each other, q2 = GM E M M , 4 0 which has solution q = = = 4 0 GM E M M , 4(8.851012 C2/Nm2 )(6.671011 Nm2/kg2 )(5.981024 kg)(7.361022 kg), 5.71 1013 C. (5.71 1013 C)/(1.60 1019 C) = 3.57 1032 protons on each body. The mass of protons needed is then (3.57 1032 )(1.67 1027 kg) = 5.97 1065 kg. Ignoring the mass of the electron (why not?) we can assume that hydrogen is all protons, so we need that much hydrogen. P251 them is Assume that the spheres initially have charges q1 and q2 . The force of attraction between F1 = 1 q1 q2 = 0.108 N, 2 4 0 r12
(b) We need
where r12 = 0.500 m. The net charge is q1 + q2 , and after the conducting wire is connected each sphere will get half of the total. The spheres will have the same charge, and repel with a force of F2 = 1 1 (q1 + q2 ) 1 (q1 + q2 ) 2 2 = 0.0360 N. 2 4 0 r12
Since we know the separation of the spheres we can find q1 + q2 quickly,
2 q1 + q2 = 2 4 0 r12 (0.0360 N) = 2.00 C
We'll put this back into the first expression and solve for q2 . 0.108 N = 1 (2.00 C  q2 )q2 , 2 4 0 r12
3.00 1012 C2 = (2.00 C  q2 )q2 , 2 0 = q2 + (2.00 C)q2 + (1.73 C)2 . The solution is q2 = 3.0 C or q2 = 1.0 C. Then q1 = 1.0 C or q1 = 3.0 C. 10
P252 The electrostatic force on Q from each q has magnitude qQ/4 0 a2 , where a is the length of the side of the square. The magnitude of the vertical (horizontal) component of the force of Q on Q is 2Q2 /16 0 a2 . (a) In order to have a zero net force on Q the magnitudes of the two contributions must balance, so 2 2Q qQ = , 2 16 0 a 4 0 a2 or q = 2Q/4. The charges must actually have opposite charge. (b) No. P253 (a) The third charge, q3 , will be between the first two. The net force on the third charge will be zero if 1 q q3 1 4q q3 2 = 4 2 , 4 0 r31 0 r32 1 2 = r31 r32 The total distance is L, so r31 + r32 = L, or r31 = L/3 and r32 = 2L/3. Now that we have found the position of the third charge we need to find the magnitude. The second and third charges both exert a force on the first charge; we want this net force on the first charge to be zero, so 1 q q3 1 q 4q 2 = 4 2 , 4 0 r13 0 r12 or q3 4q = 2, (L/3)2 L which has solution q3 = 4q/9. The negative sign is because the force between the first and second charge must be in the opposite direction to the force between the first and third charge. (b) Consider what happens to the net force on the middle charge if is is displaced a small distance z. If the charge 3 is moved toward charge 1 then the force of attraction with charge 1 will increase. But moving charge 3 closer to charge 1 means moving charge 3 away from charge 2, so the force of attraction between charge 3 and charge 2 will decrease. So charge 3 experiences more attraction to ward the charge that it moves toward, and less attraction to the charge it moves away from. Sounds unstable to me. P254 (a) The electrostatic force on the charge on the right has magnitude F = q2 , 4 0 x2 which will occur if
The weight of the ball is W = mg, and the two forces are related by F/W = tan sin = x/2L. Combining, 2Lq 2 = 4 0 mgx3 , so x= (b) Rearrange and solve for q, q= 2(8.851012 C2 /N m2 )(0.0112 kg)(9.81 m/s2 )(4.70102 m)3 = 2.28108 C. (1.22 m) q2 L 2 0
1/3
.
11
P255 (a) Originally the balls would not repel, so they would move together and touch; after touching the balls would "split" the charge ending up with q/2 each. They would then repel again. (b) The new equilibrium separation is x = P256 (q/2)2 L 2 0 mg
1/3
=
1 4
1/3
x = 2.96 cm.
Take the time derivative of the expression in Problem 254. Then dx 2 x dq 2 (4.70102 m) = = (1.20109 C/s) = 1.65103 m/s. dt 3 q dt 3 (2.28108 C)
P257
The force between the two charges is F = 1 (Q  q)q . 2 4 0 r12
We want to maximize this force with respect to variation in q, this means finding dF/dq and setting it equal to 0. Then d 1 (Q  q)q 1 Q  2q dF = = . 2 2 dq dq 4 0 r12 4 0 r12 This will vanish if Q  2q = 0, or q = 1 Q. 2 P258 Displace the charge q a distance y. The net restoring force on q will be approximately F 2 qQ 1 y qQ 16 = y. 4 0 (d/2)2 (d/2) 4 0 d3
Since F/y is effectively a force constant, the period of oscillation is T = 2 m = k
0 m 3 3
d
1/2
qQ
.
P259 Displace the charge q a distance x toward one of the positive charges Q. The net restoring force on q will be F = qQ 1 1  2 4 0 (d/2  x) (d/2 + x)2 qQ 32 x. 4 0 d3 ,
Since F/x is effectively a force constant, the period of oscillation is T = 2 m = k
0 m 3 3
d
1/2
2qQ
.
12
P2510 (a) Zero, by symmetry. (b) Removing a positive Cesium ion is equivalent to adding a singly charged negative ion at that same location. The net force is then F = e2 /4 0 r2 , where r is the distance between the Chloride ion and the newly placed negative ion, or r= The force is then F = (1.61019 C)2 = 1.92109 N. 4(8.851012 C2 /N m2 )3(0.20109 m)2 3(0.20109 m)2
P2511 We can pretend that this problem is in a single plane containing all three charges. The magnitude of the force on the test charge q0 from the charge q on the left is Fl = q q0 1 . 4 0 (a2 + R2 )
A force of identical magnitude exists from the charge on the right. we need to add these two forces as vectors. Only the components along R will survive, and each force will contribute an amount F l sin = F l so the net force on the test particle will be q q0 R 2 . 4 0 (a2 + R2 ) R2 + a2 We want to find the maximum value as a function of R. This means take the derivative, and set it equal to zero. The derivative is 2q q0 4 0 which will vanish when a2 + R2 = 3R2 , a simple quadratic equation with solutions R = a/ 2. 1 3R2  2 2 )3/2 +R (a + R2 )5/2 , R2 R , + a2
(a2
13
E261 E = F/q = ma/q. Then E = (9.111031 kg)(1.84109 m/s2 )/(1.601019 C) = 1.05102 N/C. E262 The answers to (a) and (b) are the same! F = Eq = (3.0106 N/C)(1.601019 C) = 4.81013 N. E263 F = W , or Eq = mg, so E= mg (6.64 1027 kg)(9.81 m/s2 ) = = 2.03 107 N/C. q 2(1.60 1019 C)
The alpha particle has a positive charge, this means that it will experience an electric force which is in the same direction as the electric field. Since the gravitational force is down, the electric force, and consequently the electric field, must be directed up. E264 (a) E = F/q = (3.0106 N)/(2.0109 C) = 1.5103 N/C. (b) F = Eq = (1.5103 N/C)(1.601019 C) = 2.41016 N. (c) F = mg = (1.671027 kg)(9.81 m/s2 ) = 1.61026 N. (d) (2.41016 N)/(1.61026 N) = 1.51010 . E265 Rearrange E = q/4 0 r2 , q = 4(8.851012 C2 /N m2 )(0.750 m)2 (2.30 N/C) = 1.441010 C. E266 p = qd = (1.601019 C)(4.30109 ) = 6.881028 C m. E267 Use Eq. 2612 for points along the perpendicular bisector. Then E= 1 p (3.56 1029 C m) = (8.99 109 N m2 /C2 ) = 1.95 104 N/C. 4 0 x3 (25.4 109 m)3
E268 If the charges on the line x = a where +q and q instead of +2q and 2q then at the center of the square E = 0 by symmetry. This simplifies the problem into finding E for a charge +q at (a, 0) and q at (a, a). This is a dipole, and the field is given by Eq. 2611. For this exercise we have x = a/2 and d = a, so 1 qa E= , 4 0 [2(a/2)2 ]3/2 or, putting in the numbers, E = 1.11105 N/C. E269 The charges at 1 and 7 are opposite and can be effectively replaced with a single charge of 6q at 7. The same is true for 2 and 8, 3 and 9, on up to 6 and 12. By symmetry we expect the field to point along a line so that three charges are above and three below. That would mean 9:30. E2610 If both charges are positive then Eq. 2610 would read E = 2E+ sin , and Eq. 2611 would look like 1 q x , E = 2 2 + (d/2)2 2 + (d/2)2 4 0 x x 1 q x 2 4 0 x2 x2 when x d. This can be simplified to E = 2q/4 0 x2 . 14
E2611 Treat the two charges on the left as one dipole and treat the two charges on the right as a second dipole. Point P is on the perpendicular bisector of both dipoles, so we can use Eq. 2612 to find the two fields. For the dipole on the left p = 2aq and the electric field due to this dipole at P has magnitude El = 2aq 1 4 0 (x + a)3
and is directed up. For the dipole on the right p = 2aq and the electric field due to this dipole at P has magnitude Er = 1 2aq 4 0 (x  a)3
and is directed down. The net electric field at P is the sum of these two fields, but since the two component fields point in opposite directions we must actually subtract these values, E = Er  El, 2aq 1 1 =  , 3 4 0 (x  a) (x + a)3 aq 1 1 1 =  3 3 2 0 x (1  a/x) (1 + a/x)3 aq 1 ((1 + 3a/x)  (1  3a/x)) , 2 0 x3 aq 1 (6a/x) , 2 0 x3 3(2qa2 ) . 2 0 x4
.
We can use the binomial expansion on the terms containing 1 a/x, E = =
E2612 Do a series expansion on the part in the parentheses 1 Substitute this in, Ez R2 Q = . 2 2 0 2z 4 0 z 2 1 1 + R2 /z 2 1 1 1 R2 2 z2 = R2 . 2z 2
E2613 At the surface z = 0 and Ez = /2 0 . Half of this value occurs when z is given by 1 z , =1 2 z 2 + R2 which can be written as z 2 + R2 = (2z)2 . Solve this, and z = R/ 3. E2614 Look at Eq. 2618. The electric field will be a maximum when z/(z 2 + R2 )3/2 is a maximum. Take the derivative of this with respect to z, and get 1 3 2z 2 z 2 + R2  3z 2  = . 2 (z 2 + R2 )5/2 (z 2 + R2 )3/2 (z 2 + R2 )5/2 This will vanish when the numerator vanishes, or when z = R/ 2. 15
E2615 (a) The electric field strength just above the center surface of a charged disk is given by Eq. 2619, but with z = 0, E= 2 0 The surface charge density is = q/A = q/(R2 ). Combining, q = 2 0 R2 E = 2(8.85 1012 C2 /N m2 )(2.5 102 m)2 (3 106 N/C) = 1.04 107 C. Notice we used an electric field strength of E = 3 106 N/C, which is the field at air breaks down and sparks happen. (b) We want to find out how many atoms are on the surface; if a is the cross sectional area of one atom, and N the number of atoms, then A = N a is the surface area of the disk. The number of atoms is (0.0250 m)2 A = = 1.31 1017 N= a (0.015 1018 m2 ) (c) The total charge on the disk is 1.04 107 C, this corresponds to (1.04 107 C)/(1.6 1019 C) = 6.5 1011 electrons. (We are ignoring the sign of the charge here.) If each surface atom can have at most one excess electron, then the fraction of atoms which are charged is (6.5 1011 )/(1.31 1017 ) = 4.96 106 , which isn't very many. E2616 Imagine switching the positive and negative charges. The electric field would also need to switch directions. By symmetry, then, the electric field can only point vertically down. Keeping only that component,
/2
E
= =
2
0
1 d sin , 4 0 r2
2 . 4 0 r2
But = q/(/2), so E = q/ 2 0 r2 . E2617 We want to fit the data to Eq. 2619, Ez = 2 0 1 z + R2 .
z2
There are only two variables, R and q, with q = R2 . We can find very easily if we assume that the measurements have no error because then at the surface (where z = 0), the expression for the electric field simplifies to E= . 2 0
Then = 2 0 E = 2(8.854 1012 C2 /N m2 )(2.043 107 N/C) = 3.618 104 C/m2 . Finding the radius will take a little more work. We can choose one point, and make that the reference point, and then solve for R. Starting with Ez = 2 0 1 16 z2 z + R2 ,
and then rearranging, 2 0 Ez 2 0 Ez 1 1 + (R/z)2 1 + (R/z)2 R z = 1 z , z 2 + R2 1
= 1 = = =
1 + (R/z)2 2 0 Ez 1 , 1 2, (1  2 0 Ez /) 1 (1  2 0 Ez /)
2
,
 1.
Using z = 0.03 m and Ez = 1.187 107 N/C, along with our value of = 3.618 104 C/m2 , we find R z R = = 1 (1 
2 2(8.8541012 C2/Nm2 )(1.187107 N/C)/(3.618104 C/m2 ))
 1,
2.167(0.03 m) = 0.065 m.
(b) And now find the charge from the charge density and the radius, q = R2 = (0.065 m)2 (3.618 104 C/m2 ) = 4.80 C. E2618 (a) = q/L. (b) Integrate: E = = = 1 dxx2 , 4 0 a 1 1  , 4 0 a L + a q 1 , 4 0 a(L + a)
L+a
since = q/L. (c) If a L then L can be replaced with 0 in the above expression. E2619 A sketch of the field looks like this.
17
E2620 (a) F = Eq = (40 N/C)(1.601019 C) = 6.41018 N (b) Lines are twice as far apart, so the field is half as large, or E = 20N/C. E2621 Consider a view of the disk on edge.
E2622 A sketch of the field looks like this.
18
E2623 To the right. E2624 (a) The electric field is zero nearer to the smaller charge; since the charges have opposite signs it must be to the right of the +2q charge. Equating the magnitudes of the two fields, 2q 5q = , 4 0 x2 4 0 (x + a)2 or which has solution x= 5x = 2(x + a),
2a = 2.72a. 5 2
E2625 This can be done quickly with a spreadsheet.
E
x d
E2626 (a) At point A, E= 1 4 0  q 2q  d2 (2d)2 = 1 q , 4 0 2d2
19
where the negative sign indicates that E is directed to the left. At point B, 1 q 2q 1 6q E=  = , 2 2 4 0 (d/2) (d/2) 4 0 d2 where the positive sign indicates that E is directed to the right. At point C, q 2q 1 7q 1 + 2 = , E= 2 4 0 (2d) d 4 0 4d2 where the negative sign indicates that E is directed to the left. E2627 (a) The electric field does (negative) work on the electron. The magnitude of this work is W = F d, where F = Eq is the magnitude of the electric force on the electron and d is the distance through which the electron moves. Combining, W = F d = q E d, which gives the work done by the electric field on the electron. The electron originally possessed a 1 kinetic energy of K = 2 mv 2 , since we want to bring the electron to a rest, the work done must be negative. The charge q of the electron is negative, so E and d are pointing in the same direction, and E d = Ed. By the work energy theorem, 1 W = K = 0  mv 2 . 2 We put all of this together and find d, d= mv 2 (9.111031 kg)(4.86 106 m/s)2 W = = = 0.0653 m. qE 2qE 2(1.601019 C)(1030 N/C)
(b) Eq = ma gives the magnitude of the acceleration, and v f = v i + at gives the time. But v f = 0. Combining these expressions, t= mv i (9.111031 kg)(4.86 106 m/s) = = 2.69108 s. Eq (1030 N/C)(1.601019 C)
(c) We will apply the work energy theorem again, except now we don't assume the final kinetic energy is zero. Instead, W = K = K f  K i , and dividing through by the initial kinetic energy to get the fraction lost, W Kf  Ki = = fractional change of kinetic energy. Ki Ki But K i = 1 mv 2 , and W = qEd, so the fractional change is 2 W (1.601019 C)(1030 N/C)(7.88103 m) qEd = = 12.1%. = 1 1 2 31 kg)(4.86 106 m/s)2 Ki 2 mv 2 (9.1110 E2628 (a) a = Eq/m = (2.16104 N/C)(1.601019 C)/(1.671027 kg) = 2.071012 m/s2 . (b) v = 2ax = 2(2.071012 m/s2 )(1.22102 m) = 2.25105 m/s.
20
E2629 (a) E = 2q/4 0 r2 , or E= (1.88107 C) = 5.85105 N/C. 2(8.851012 C2 /N m2 )(0.152 m/2)2
(b) F = Eq = (5.85105 N/C)(1.601019 C) = 9.361014 N. E2630 (a) The average speed between the plates is (1.95102 m)/(14.7109 s) = 1.33106 m/s. The speed with which the electron hits the plate is twice this, or 2.65106 m/s. (b) The acceleration is a = (2.65106 m/s)/(14.7109 s) = 1.801014 m/s2 . The electric field then has magnitude E = ma/q, or E = (9.111031 kg)(1.801014 m/s2 )/(1.601019 C) = 1.03103 N/C. E2631 The drop is balanced if the electric force is equal to the force of gravity, or Eq = mg. The mass of the drop is given in terms of the density by 4 m = V = r3 . 3 Combining, q= mg 4r3 g 4(851 kg/m3 )(1.64106 m)3 (9.81 m/s2 ) = = = 8.111019 C. E 3E 3(1.92105 N/C)
We want the charge in terms of e, so we divide, and get q (8.111019 C) = = 5.07 5. e (1.601019 C) E2632 (b) F = (8.99109 N m2 /C2 )(2.16106 C)(85.3109 C)/(0.117m)2 = 0.121 N. (a) E2 = F/q1 = (0.121 N)/(2.16106 C) = 5.60104 N/C. E1 = F/q2 = (0.121 N)/(85.3109 C) = 1.42106 N/C. E2633 If each value of q measured by Millikan was a multiple of e, then the difference between any two values of q must also be a multiple of q. The smallest difference would be the smallest multiple, and this multiple might be unity. The differences are 1.641, 1.63, 1.60, 1.63, 3.30, 3.35, 3.18, 3.24, all times 1019 C. This is a pretty clear indication that the fundamental charge is on the order of 1.6 1019 C. If so, the likely number of fundamental charges on each of the drops is shown below in a table arranged like the one in the book: 4 5 7 8 10 11 12 14 16
The total number of charges is 87, while the total charge is 142.69 1019 C, so the average charge per quanta is 1.64 1019 C.
21
E2634 Because of the electric field the acceleration toward the ground of a charged particle is not g, but g Eq/m, where the sign depends on the direction of the electric field. (a) If the lower plate is positively charged then a = g  Eq/m. Replace g in the pendulum period expression by this, and then L T = 2 . g  Eq/m (b) If the lower plate is negatively charged then a = g + Eq/m. Replace g in the pendulum period expression by this, and then T = 2 L . g + Eq/m
E2635 The ink drop travels an additional time t = d/vx , where d is the additional horizontal distance between the plates and the paper. During this time it travels an additional vertical distance y = vy t , where vy = at = 2y/t = 2yvx /L. Combining, y = 2yvx t 2yd 2(6.4104 m)(6.8103 m) = = = 5.44104 m, L L (1.6102 m)
so the total deflection is y + y = 1.18103 m. E2636 (a) p = (1.48109 C)(6.23106 m) = 9.221015 C m. (b) U = 2pE = 2(9.221015 C m)(1100 N/C) = 2.031011 J. E2637 Use = pE sin , where is the angle between p and E. For this dipole p = qd = 2ed or p = 2(1.6 1019 C)(0.78 109 m) = 2.5 1028 C m. For all three cases pE = (2.5 1028 C m)(3.4 106 N/C) = 8.5 1022 N m. The only thing we care about is the angle. (a) For the parallel case = 0, so sin = 0, and = 0. (b) For the perpendicular case = 90 , so sin = 1, and = 8.5 1022 N m.. (c) For the antiparallel case = 180 , so sin = 0, and = 0. E2638 (c) Equal and opposite, or 5.221016 N. (d) Use Eq. 2612 and F = Eq. Then p = = = E2639 4 0 x3 F , q 4(8.851012 C2 /N m2 )(0.285m)3 (5.221016 N) , (3.16106 C) 4.251022 C m.
The pointlike nucleus contributes an electric field E+ = 1 Ze , 4 0 r2
while the uniform sphere of negatively charged electron cloud of radius R contributes an electric field given by Eq. 2624, 1 Zer E = . 4 0 R3 22
The net electric field is just the sum, E= Ze 4 0 1 r  3 r2 R
E2640 The shell theorem first described for gravitation in chapter 14 is applicable here since both electric forces and gravitational forces fall off as 1/r2 . The net positive charge inside the sphere of radius d/2 is given by Q = 2e(d/2)3 /R3 = ed3 /4R3 . The net force on either electron will be zero when eQ 4e2 d3 e2 d e2 = = 2 = 3, d2 (d/2)2 d 4R3 R which has solution d = R. P261 (a) Let the positive charge be located closer to the point in question, then the electric field from the positive charge is q 1 E+ = 4 0 (x  d/2)2 and is directed away from the dipole. The negative charge is located farther from the point in question, so E = 1 q 4 0 (x + d/2)2
and is directed toward the dipole. The net electric field is the sum of these two fields, but since the two component fields point in opposite direction we must actually subtract these values, E = E +  E , 1 q 1 q  , = 4 0 (z  d/2)2 4 0 (z + d/2)2 1 1 1 q  = 4 0 z 2 (1  d/2z)2 (1 + d/2z)2
We can use the binomial expansion on the terms containing 1 d/2z, E = 1 q ((1 + d/z)  (1  d/z)) , 4 0 z 2 1 qd 2 0 z 3
(b) The electric field is directed away from the positive charge when you are closer to the positive charge; the electric field is directed toward the negative charge when you are closer to the negative charge. In short, along the axis the electric field is directed in the same direction as the dipole moment. P262 The key to this problem will be the expansion of 1 1 2 (x2 + (z d/2)2 )3/2 (x + z 2 )3/2 1 3 zd 2 x2 + z 2 .
23
for d
x2 + z 2 . Far from the charges the electric field of the positive charge has magnitude E+ = 1 q , 4 0 x2 + (z  d/2)2 x x2 + (z  d/2)2 (z  d/2)
the components of this are Ex,+ Ez,+ = = q 1 2 + z2 4 0 x q 1 4 0 x2 + z 2 , .
x2 + (z  d/2)2 3 zd 2 x2 + z 2 3 zd 1+ 2 x2 + z 2 1+
Expand both according to the first sentence, then Ex,+ Ez,+ = 1 xq 4 0 (x2 + z 2 )3/2 1 (z  d/2)q 4 0 (x2 + z 2 )3/2 , .
Similar expression exist for the negative charge, except we must replace q with q and the + in the parentheses with a , and z  d/2 with z + d/2 in the Ez expression. All that is left is to add the expressions. Then Ex = = Ez = = = 1 xq 3 zd 1 xq 1+ + 4 0 (x2 + z 2 )3/2 2 x2 + z 2 4 0 (x2 + z 2 )3/2 3xqzd 1 , 4 0 (x2 + z 2 )5/2 3 zd 1 (z  d/2)q 1 (z + d/2)q 1+ + 2 + z2 2 + z 2 )3/2 4 0 (x 2x 4 0 (x2 + z 2 )3/2 1 3z 2 dq 1 dq  , 2 + z 2 )5/2 4 0 (x 4 0 (x2 + z 2 )3/2 1 (2z 2  x2 )dq . 4 0 (x2 + z 2 )5/2 1 3 zd 2 x2 + z 2 ,
1
3 zd 2 x2 + z 2
,
P263 (a) Each point on the ring is a distance z 2 + R2 from the point on the axis in question. Since all points are equal distant and subtend the same angle from the axis then the top half of the ring contributes q1 z E1z = , 2 + R2 ) 2 + R2 4 0 (x z while the bottom half contributes a similar expression. Add, and Ez = q1 + q2 z q = 4 0 (z 2 + R2 )3/2 4
0
(z 2
z , + R2 )3/2
which is identical to Eq. 2618. (b) The perpendicular component would be zero if q1 = q2 . It isn't, so it must be the difference q1  q2 which is of interest. Assume this charge difference is evenly distributed on the top half of the ring. If it is a positive difference, then E must point down. We are only interested then in the vertical component as we integrate around the top half of the ring. Then E = = 1 (q1  q2 )/ cos d, 4 0 z 2 + R2 0 q1  q2 1 . 2 2 + R2 2 0 z 24
P264 Use the approximation 1/(z d)2 (1/z 2 )(1 Add the contributions: E = = where Q = 2qd2 .
2d/z + 3d2 /z 2 ).
q 2q q 1  2 + , 2 4 0 (z + d) z (z  d)2 q 2d 3d2 2d 3d2 1 + 2 2+1+ + 2 2 4 0 z z z z z 2 q 6d 3Q = , 4 0 z 2 z 2 4 0 z 4
,
P265 A monopole field falls off as 1/r2 . A dipole field falls off as 1/r3 , and consists of two oppositely charge monopoles close together. A quadrupole field (see Exercise 11 above or read Problem 4) falls off as 1/r4 and (can) consist of two otherwise identical dipoles arranged with antiparallel dipole moments. Just taking a leap of faith it seems as if we can construct a 1/r6 field behavior by extending the reasoning. First we need an octopole which is constructed from a quadrupole. We want to keep things as simple as possible, so the construction steps are 1. The monopole is a charge +q at x = 0. 2. The dipole is a charge +q at x = 0 and a charge q at x = a. We'll call this a dipole at x = a/2 3. The quadrupole is the dipole at x = a/2, and a second dipole pointing the other way at x = a/2. The charges are then q at x = a, +2q at x = 0, and q at x = a. 4. The octopole will be two stacked, offset quadrupoles. There will be q at x = a, +3q at x = 0, 3q at x = a, and +q at x = 2a. 5. Finally, our distribution with a far field behavior of 1/r6 . There will be +q at x = 2a, 4q at x = a, +6q at x = 0, 4q at x = a, and +q at x = 2a. P266 The vertical component of E is simply half of Eq. 2617. The horizontal component is given by a variation of the work required to derive Eq. 2616, dEz = dE sin = 1 dz 4 0 y 2 + z 2 z y2 + z2 ,
which integrates to zero if the limits are  to +, but in this case,
Ez =
0
dEz =
1 . 4 0 z
Since the vertical and horizontal components are equal then E makes an angle of 45 . P267 (a) Swap all positive and negative charges in the problem and the electric field must reverse direction. But this is the same as flipping the problem over; consequently, the electric field must point parallel to the rod. This only holds true at point P , because point P doesn't move when you flip the rod.
25
(b) We are only interested in the vertical component of the field as contributed from each point on the rod. We can integrate only half of the rod and double the answer, so we want to evaluate
L/2
Ez
= 2
0
1 dz 4 0 y 2 + z 2
z y2 + z2
,
=
(L/2)2 + y 2  y 2 . 4 0 y (L/2)2 + y 2 L, then the expression simplifies with a Taylor L2 , 4 0 y 3
(c) The previous expression is exact. If y expansion to Ez = which looks similar to a dipole. P268 Evaluate E=
0 R
1 z dq , 4 0 (z 2 + r2 )3/2
where r is the radius of the ring, z the distance to the plane of the ring, and dq the differential charge on the ring. But r2 + z 2 = R2 , and dq = (2r dr), where = q/2R2 . Then R q R2  r2 r dr E = , R5 0 4 0 q 1 = . 4 0 3R2 P269 The key statement is the second italicized paragraph on page 595; the number of field lines through a unit crosssectional area is proportional to the electric field strength. If the exponent is n, then the electric field strength a distance r from a point charge is E= kq , rn
and the total cross sectional area at a distance r is the area of a spherical shell, 4r2 . Then the number of field lines through the shell is proportional to EA = kq 4r2 = 4kqr2n . rn
Note that the number of field lines varies with r if n = 2. This means that as we go farther from the point charge we need more and more field lines (or fewer and fewer). But the field lines can only start on charges, and we don't have any except for the point charge. We have a problem; we really do need n = 2 if we want workable field lines. P2610 The distance traveled by the electron will be d1 = a1 t2 /2; the distance traveled by the proton will be d2 = a2 t2 /2. a1 and a2 are related by m1 a1 = m2 a2 , since the electric force is the same (same charge magnitude). Then d1 + d2 = (a1 + a2 )t2 /2 is the 5.00 cm distance. Divide by the proton distance, and then d1 + d2 a1 + a2 m2 = = + 1. d2 a2 m1 Then d2 = (5.00102 m)/(1.671027 /9.111031 + 1) = 2.73105 m. 26
P2611 This is merely a fancy projectile motion problem. vx = v0 cos while vy,0 = v0 sin . The x and y positions are x = vx t and y= 1 2 ax2 at + vy,0 t = 2 + x tan . 2 2v0 cos2
The acceleration of the electron is vertically down and has a magnitude of a= F Eq (1870 N/C)(1.61019 C) = = = 3.2841014 m/s2 . m m (9.111031 kg)
We want to find out how the vertical velocity of the electron at the location of the top plate. If we get an imaginary answer, then the electron doesn't get as high as the top plate. vy = vy,0 2 + 2ay,
= (5.83106 m/s)2 sin(39 )2 + 2(3.2841014 m/s2 )(1.97102 m), = 7.226105 m/s. This is a real answer, so this means the electron either hits the top plate, or it misses both plates. The time taken to reach the height of the top plate is t= vy (7.226105 m/s)  (5.83106 m/s) sin(39 ) = = 8.972109 s. a (3.2841014 m/s2 )
In this time the electron has moved a horizontal distance of x = (5.83106 m/s) cos(39 )(8.972109 s) = 4.065102 m. This is clearly on the upper plate. P2612 Near the center of the ring z R, so a Taylor expansion yields E= z . 2 0 R2
The force on the electron is F = Ee, so the effective "spring" constant is k = e/2 0 R2 . This means = P2613 k = m e = 2 0 mR2 eq . 4 0 mR3
U = pE cos , so the work required to flip the dipole is W = pE [cos(0 + )  cos 0 ] = 2pE cos 0 .
P2614 If the torque on a system is given by   = , where is a constant, then the frequency of oscillation of the system is f = /I/2. In this case = pE sin pE, so f= pE/I/2.
27
P2615 Use the a variation of the exact result from Problem 261. The two charge are positive, but since we will eventually focus on the area between the charges we must subtract the two field contributions, since they point in opposite directions. Then Ez = and then take the derivative, dEz q = dz 2 1 1  (z  a/2)3 (z + a/2)3 a, , . q 4 1 1  (z  a/2)2 (z + a/2)2
0
0
Applying the binomial expansion for points z dEz dz = 
8q 1 1 1  3 3 2 0 a (2z/a  1) (2z/a + 1)3 8q 1  ((1 + 6z/a)  (1  6z/a)) , 2 0 a3 8q 1 = . 0 a3
There were some fancy sign flips in the second line, so review those steps carefully! (b) The electrostatic force on a dipole is the difference in the magnitudes of the electrostatic forces on the two charges that make up the dipole. Near the center of the above charge arrangement the electric field behaves as Ez Ez (0) + The net force on a dipole is F+  F = q(E+  E ) = q Ez (0) + dEz dz z+  Ez (0) 
z=0
dEz dz
z + higher ordered terms.
z=0
dEz dz
z
z=0
where the "+" and "" subscripts refer to the locations of the positive and negative charges. This last line can be simplified to yield q dEz dz (z+  z ) = qd
z=0
dEz dz
.
z=0
28
E271 E = (1800 N/C)(3.2103 m)2 cos(145 ) = 7.8103 N m2 /C. E272 The right face has an area element given by A = (1.4 m)2^ j. 2 ^ ^ = 0. (a) E = A E = (2.0 m )j (6 N/C)i (b) E = (2.0 m2 )^ (2 N/C)^ = 4N m2 /C. j j ^ (c) E = (2.0 m2 )^ [(3 N/C)^ + (4 N/C)k] = 0. j i (d) In each case the field is uniform so we can simply evaluate E = E A, where A has six parts, one for every face. The faces, however, have the same size but are organized in pairs with opposite directions. These will cancel, so the total flux is zero in all three cases. E273 (a) The flat base is easy enough, since according to Eq. 277, E = E dA.
There are two important facts to consider in order to integrate this expression. E is parallel to the axis of the hemisphere, E points inward while dA points outward on the flat base. E is uniform, so it is everywhere the same on the flat base. Since E is antiparallel to dA, E dA = E dA, then E = Since E is uniform we can simplify this as E =  E dA = E dA = EA = R2 E. E dA =  E dA.
The last steps are just substituting the area of a circle for the flat side of the hemisphere. (b) We must first sort out the dot product
E dA R
We can simplify the vector part of the problem with E dA = cos E dA, so E = E dA = cos E dA
Once again, E is uniform, so we can take it out of the integral, E = cos E dA = E cos dA
Finally, dA = (R d)(R sin d) on the surface of a sphere centered on R = 0. 29
We'll integrate around the axis, from 0 to 2. We'll integrate from the axis to the equator, from 0 to /2. Then
2 /2
E = E
cos dA = E
0 0
R2 cos sin d d.
Pulling out the constants, doing the integration, and then writing 2 cos sin as sin(2),
/2 /2
E = 2R2 E
0
cos sin d = R2 E
0
sin(2) d,
Change variables and let = 2, then we have
E = R2 E
0
1 sin d = R2 E. 2
E274 Through S1 , E = q/ 0 . Through S2 , E = q/ 0 . Through S3 , E = q/ 0 . Through S4 , E = 0. Through S5 , E = q/ 0 . E275 By Eq. 278, E = q
0
=
(1.84 C) = 2.08105 N m2 /C. (8.851012 C2 /N m2 )
E276 The total flux through the sphere is E = (1 + 2  3 + 4  5 + 6)(103 N m2 /C) = 3103 N m2 /C. The charge inside the die is (8.851012 C2 /N m2 )(3103 N m2 /C) = 2.66108 C. E277 The total flux through a cube would be q/ 0 . Since the charge is in the center of the cube we expect that the flux through any side would be the same, or 1/6 of the total flux. Hence the flux through the square surface is q/6 0 . E278 If the electric field is uniform then there are no free charges near (or inside) the net. The flux through the netting must be equal to, but opposite in sign, from the flux through the opening. The flux through the opening is Ea2 , so the flux through the netting is Ea2 . E279 There is no flux through the sides of the cube. The flux through the top of the cube is (58 N/C)(100 m)2 = 5.8105 N m2 /C. The flux through the bottom of the cube is (110 N/C)(100 m)2 = 1.1106 N m2 /C. The total flux is the sum, so the charge contained in the cube is q = (8.851012 C2 /N m2 )(5.2105 N m2 /C) = 4.60106 C. E2710 (a) There is only a flux through the right and left faces. Through the right face R = (2.0 m2 )^ (3 N/C m)(1.4 m)^ = 8.4 N m2 /C. j j The flux through the left face is zero because y = 0. 30
E2711 There are eight cubes which can be "wrapped" around the charge. Each cube has three external faces that are indistinguishable for a total of twentyfour faces, each with the same flux E . The total flux is q/ 0 , so the flux through one face is E = q/24 0 . Note that this is the flux through faces opposite the charge; for faces which touch the charge the electric field is parallel to the surface, so the flux would be zero. E2712 Use Eq. 2711, = 2 0 rE = 2(8.851012 C2 /N m2 )(1.96 m)(4.52104 N/C) = 4.93106 C/m. E2713 (a) q = A = (2.0106 C/m2 )(0.12 m)(0.42 m) = 3.17107 C. (b) The charge density will be the same! q = A = (2.0 106 C/m2 )(0.08 m)(0.28 m) = 1.41107 C. E2714 The electric field from the sheet on the left is of magnitude E l = /2 0 , and points directly away from the sheet. The magnitude of the electric field from the sheet on the right is the same, but it points directly away from the sheet on the right. (a) To the left of the sheets the two fields add since they point in the same direction. This means that the electric field is E = (/ 0 )^ i. (b) Between the sheets the two electric fields cancel, so E = 0. (c) To the right of the sheets the two fields add since they point in the same direction. This means that the electric field is E = (/ 0 )^ i. E2715 The electric field from the plate on the left is of magnitude E l = /2 0 , and points directly toward the plate. The magnitude of the electric field from the plate on the right is the same, but it points directly away from the plate on the right. (a) To the left of the plates the two fields cancel since they point in the opposite directions. This means that the electric field is E = 0. (b) Between the plates the two electric fields add since they point in the same direction. This means that the electric field is E = (/ 0 )^ i. (c) To the right of the plates the two fields cancel since they point in the opposite directions. This means that the electric field is E = 0. E2716 The magnitude of the electric field is E = mg/q. The surface charge density on the plates is = 0 E = 0 mg/q, or = (8.851012 C2 /N m2 )(9.111031 kg)(9.81 m/s2 ) = 4.941022 C/m2 . (1.601019 C)
E2717 We don't really need to write an integral, we just need the charge per unit length in the cylinder to be equal to zero. This means that the positive charge in cylinder must be +3.60nC/m. This positive charge is uniformly distributed in a circle of radius R = 1.50 cm, so = 3.60nC/m 3.60nC/m = = 5.09C/m3 . R2 (0.0150 m)2
31
E2718 The problem has spherical symmetry, so use a Gaussian surface which is a spherical shell. The E field will be perpendicular to the surface, so Gauss' law will simplify to q enc /
0
=
E dA =
E dA = E
dA = 4r2 E.
(a) For point P1 the charge enclosed is q enc = 1.26107 C, so E= 4(8.851012 C2 /N (1.26107 C) = 3.38106 N/C. m2 )(1.83102 m)2
(b) Inside a conductor E = 0. E2719 The proton orbits with a speed v, so the centripetal force on the proton is FC = mv 2 /r. This centripetal force is from the electrostatic attraction with the sphere; so long as the proton is outside the sphere the electric field is equivalent to that of a point charge Q (Eq. 2715), E= 1 Q . 4 0 r2
If q is the charge on the proton we can write F = Eq, or 1 Q mv 2 =q r 4 0 r2 Solving for Q, Q = = 4 0 mv 2 r , q 4(8.851012 C2 /N m2 )(1.671027 kg)(294103 m/s)2 (0.0113 m) , (1.601019 C)
= 1.13109 C. E2720 The problem has spherical symmetry, so use a Gaussian surface which is a spherical shell. The E field will be perpendicular to the surface, so Gauss' law will simplify to q enc /
0
=
E dA =
E dA = E
dA = 4r2 E.
(a) At r = 0.120 m q enc = 4.06108 C. Then E= 4(8.851012 C2 /N (4.06108 C) = 2.54104 N/C. m2 )(1.20101 m)2
(b) At r = 0.220 m q enc = 5.99108 C. Then E= 4(8.851012 C2 /N (5.99108 C) = 1.11104 N/C. m2 )(2.20101 m)2
(c) At r = 0.0818 m q enc = 0 C. Then E = 0.
32
E2721 The problem has cylindrical symmetry, so use a Gaussian surface which is a cylindrical shell. The E field will be perpendicular to the curved surface and parallel to the end surfaces, so Gauss' law will simplify to q enc /
0
=
E dA =
E dA = E
dA = 2rLE,
where L is the length of the cylinder. Note that = q/2rL represents a surface charge density. (a) r = 0.0410 m is between the two cylinders. Then E= (24.1106 C/m2 )(0.0322 m) = 2.14106 N/C. (8.851012 C2 /N m2 )(0.0410 m)
It points outward. (b) r = 0.0820 m is outside the two cylinders. Then E= (24.1106 C/m2 )(0.0322 m) + (18.0106 C/m2 )(0.0618 m) = 4.64105 N/C. (8.851012 C2 /N m2 )(0.0820 m)
The negative sign is because it is pointing inward. E2722 The problem has cylindrical symmetry, so use a Gaussian surface which is a cylindrical shell. The E field will be perpendicular to the curved surface and parallel to the end surfaces, so Gauss' law will simplify to q enc /
0
=
E dA =
E dA = E
dA = 2rLE,
where L is the length of the cylinder. The charge enclosed is q enc = The electric field is given by E= At the surface, Es = Solve for r when E is half of this: 3R r 2  R2 = , 8 2r 3rR = 4r2  4R2 , 0 = 4r2  3rR  4R2 . The solution is r = 1.443R. That's (2R  1.443R) = 0.557R beneath the surface. E2723 The electric field must do work on the electron to stop it. The electric field is given by E = /2 0 . The work done is W = F d = Eqd. d is the distance in question, so d= 2 0K 2(8.851012 C2 /N m2 )(1.15105 eV) = = 0.979 m q (2.08106 C/m2 )e 33 (2R)2  R2 3R = . 2 0 2R 4 0 r 2  R2 L r2  R2 = . 2 0 rL 2 0r dV = L r2  R2
E2724 Let the spherical Gaussian surface have a radius of R and be centered on the origin. Choose the orientation of the axis so that the infinite line of charge is along the z axis. The electric field is then directed radially outward from the z axis with magnitude E = /2 0 , where is the perpendicular distance from the z axis. Now we want to evaluate E = E dA,
over the surface of the sphere. In spherical coordinates, dA = R2 sin d d, = R sin , and E dA = EA sin . Then 2R sin R d d = . E = 2 0 0 E2725 (a) The problem has cylindrical symmetry, so use a Gaussian surface which is a cylindrical shell. The E field will be perpendicular to the curved surface and parallel to the end surfaces, so Gauss' law will simplify to q enc /
0
=
E dA =
E dA = E
dA = 2rLE,
where L is the length of the cylinder. Now for the q enc part. If the (uniform) volume charge density is , then the charge enclosed in the Gaussian cylinder is q enc = dV = dV = V = r2 L.
Combining, r2 L/ 0 = E2rL or E = r/2 0 . (b) Outside the charged cylinder the charge enclosed in the Gaussian surface is just the charge in the cylinder. Then q enc = and R2 L/ and then finally E= R2 . 2 0r
0
dV =
dV = V = R2 L. = E2rL,
E2726 (a) q = 4(1.22 m)2 (8.13106 C/m2 ) = 1.52104 C. (b) E = q/ 0 = (1.52104 C)/(8.851012 C2 /N m2 ) = 1.72107 N m2 /C. (c) E = / 0 = (8.13106 C/m2 )/(8.851012 C2 /N m2 ) = 9.19105 N/C E2727 (a) = (2.4106 C)/4(0.65 m)2 = 4.52107 C/m2 . (b) E = / 0 = (4.52107 C/m2 )/(8.851012 C2 /N m2 ) = 5.11104 N/C. E2728 E = / E2729
0
= q/4r2 0 .
(a) The near field is given by Eq. 2712, E = /2 0 , so E (6.0106 C)/(8.0102 m)2 = 5.3107 N/C. 2(8.851012 C2 /N m2 )
(b) Very far from any object a point charge approximation is valid. Then E= 1 q 1 (6.0106 C) = = 60N/C. 4 0 r2 4(8.851012 C2 /N m2 ) (30 m)2 34
P271
For a spherically symmetric mass distribution choose a spherical Gaussian shell. Then g dA = g dA = g dA = 4r2 g.
Then
g gr2 = = m, 4G G g=
or
Gm . r2 The negative sign indicates the direction; g point toward the mass center. P272 (a) The flux through all surfaces except the right and left faces will be zero. Through the left face, l = Ey A = b aa2 . Through the right face, The net flux is then = ba5/2 ( 2  1) = (8830 N/C m1/2 )(0.130 m)5/2 ( 2  1) = 22.3 N m2 /C. (b) The charge enclosed is q = (8.851012 C2 /N m2 )(22.3 N m2 /C) = 1.971010 C. P273 The net force on the small sphere is zero; this force is the vector sum of the force of gravity W , the electric force FE , and the tension T . r = Ey A = b 2aa2 .
T
FE
W
These forces are related by Eq = mg tan . We also have E = /2 0 , so = = = 2 0 mg tan , q 2(8.851012 C2 /N m2 )(1.12106 kg)(9.81 m/s2 ) tan(27.4 ) , (19.7109 C) 5.11109 C/m2 .
35
P274 The materials are conducting, so all charge will reside on the surfaces. The electric field inside any conductor is zero. The problem has spherical symmetry, so use a Gaussian surface which is a spherical shell. The E field will be perpendicular to the surface, so Gauss' law will simplify to q enc /
0
=
E dA =
E dA = E
dA = 4r2 E.
Consequently, E = q enc /4 0 r2 . (a) Within the sphere E = 0. (b) Between the sphere and the shell q enc = q. Then E = q/4 0 r2 . (c) Within the shell E = 0. (d) Outside the shell q enc = +q  q = 0. Then E = 0. (e) Since E = 0 inside the shell, q enc = 0, this requires that q reside on the inside surface. This is no charge on the outside surface. P275 The problem has cylindrical symmetry, so use a Gaussian surface which is a cylindrical shell. The E field will be perpendicular to the curved surface and parallel to the end surfaces, so Gauss' law will simplify to q enc /
0
=
E dA =
E dA = E
dA = 2rLE,
where L is the length of the cylinder. Consequently, E = q enc /2 0 rL. (a) Outside the conducting shell q enc = +q  2q = q. Then E = q/2 0 rL. The negative sign indicates that the field is pointing inward toward the axis of the cylinder. (b) Since E = 0 inside the conducting shell, q enc = 0, which means a charge of q is on the inside surface of the shell. The remaining q must reside on the outside surface of the shell. (c) In the region between the cylinders q enc = +q. Then E = +q/2 0 rL. The positive sign indicates that the field is pointing outward from the axis of the cylinder. P276 Subtract Eq. 2619 from Eq. 2620. Then z E= . 2 0 z 2 + R2
P277 This problem is closely related to Ex. 2725, except for the part concerning q enc . We'll set up the problem the same way: the Gaussian surface will be a (imaginary) cylinder centered on the axis of the physical cylinder. For Gaussian surfaces of radius r < R, there is no charge enclosed while for Gaussian surfaces of radius r > R, q enc = l. We've already worked out the integral E dA = 2rlE,
tube
for the cylinder, and then from Gauss' law, q enc =
0
tube
E dA = 2 0 rlE.
(a) When r < R there is no enclosed charge, so the left hand vanishes and consequently E = 0 inside the physical cylinder. (b) When r > R there is a charge l enclosed, so E= . 2 0 r 36
P278 This problem is closely related to Ex. 2725, except for the part concerning q enc . We'll set up the problem the same way: the Gaussian surface will be a (imaginary) cylinder centered on the axis of the physical cylinders. For Gaussian surfaces of radius r < a, there is no charge enclosed while for Gaussian surfaces of radius b > r > a, q enc = l. We've already worked out the integral E dA = 2rlE,
tube
for the cylinder, and then from Gauss' law, q enc =
0
tube
E dA = 2 0 rlE.
(a) When r < a there is no enclosed charge, so the left hand vanishes and consequently E = 0 inside the inner cylinder. (b) When b > r > a there is a charge l enclosed, so E= . 2 0 r
P279 Uniform circular orbits require a constant net force towards the center, so F = Eq = q/2 0 r. The speed of the positron is given by F = mv 2 /r; the kinetic energy is K = mv 2 /2 = F r/2. Combining, K = = = P2710 = 2 0 rE, so q = 2(8.851012 C2 /N m2 )(0.014 m)(0.16 m)(2.9104 N/C) = 3.6109 C. P2711 (a) Put a spherical Gaussian surface inside the shell centered on the point charge. Gauss' law states q enc E dA = .
0
q , 4 0 (30109 C/m)(1.61019 C) , 4((8.85 1012 C2 /N m2 ) 4.311017 J = 270 eV.
Since there is spherical symmetry the electric field is normal to the spherical Gaussian surface, and it is everywhere the same on this surface. The dot product simplifies to E dA = E dA, while since E is a constant on the surface we can pull it out of the integral, and we end up with E dA = q
0
,
where q is the point charge in the center. Now dA = 4r2 , where r is the radius of the Gaussian surface, so q E= . 4 0 r2 (b) Repeat the above steps, except put the Gaussian surface outside the conducting shell. Keep it centered on the charge. Two things are different from the above derivation: (1) r is bigger, and 37
(2) there is an uncharged spherical conducting shell inside the Gaussian surface. Neither change will affect the surface integral or q enc , so the electric field outside the shell is still E= q , 4 0 r2
(c) This is a subtle question. With all the symmetry here it appears as if the shell has no effect; the field just looks like a point charge field. If, however, the charge were moved off center the field inside the shell would become distorted, and we wouldn't be able to use Gauss' law to find it. So the shell does make a difference. Outside the shell, however, we can't tell what is going on inside the shell. So the electric field outside the shell looks like a point charge field originating from the center of the shell regardless of where inside the shell the point charge is placed! (d) Yes, q induces surface charges on the shell. There will be a charge q on the inside surface and a charge q on the outside surface. (e) Yes, as there is an electric field from the shell, isn't there? (f) No, as the electric field from the outside charge won't make it through a conducting shell. The conductor acts as a shield. (g) No, this is not a contradiction, because the outside charge never experienced any electrostatic attraction or repulsion from the inside charge. The force is between the shell and the outside charge. P2712 Then The repulsive electrostatic forces must exactly balance the attractive gravitational forces. 1 q2 m2 =G 2 , 4 0 r2 r (1.601019 C) 4(8.851012 C2 /N m2 )(6.671011 N m2 /kg ) P2713 The problem has spherical symmetry, so use a Gaussian surface which is a spherical shell. The E field will be perpendicular to the surface, so Gauss' law will simplify to q enc /
0 2
or m = q/ 4 0 G. Numerically, m=
= 1.86109 kg.
=
E dA =
E dA = E
dA = 4r2 E.
Consequently, E = q enc /4 0 r2 . q enc = q + 4 r2 dr, or
r
q enc = q + 4
a
Ar dr = q + 2A(r2  a2 ).
The electric field will be constant if q enc behaves as r2 , which requires q = 2Aa2 , or A = q/2a2 . P2714 (a) The problem has spherical symmetry, so use a Gaussian surface which is a spherical shell. The E field will be perpendicular to the surface, so Gauss' law will simplify to q enc /
0
=
E dA =
E dA = E
dA = 4r2 E.
Consequently, E = q enc /4 0 r2 . q enc = 4 r2 dr = 4r3 /3, so E = r/3 38
0
and is directed radially out from the center. Then E = r/3 0 . (b) The electric field in the hole is given by Eh = E  Eb , where E is the field from part (a) and Eb is the field that would be produced by the matter that would have been in the hole had the hole not been there. Then Eb = b/3 0 , where b is a vector pointing from the center of the hole. Then Eh = But r  b = a, so Eh = a/3 0 . P2715 If a point is an equilibrium point then the electric field at that point should be zero. If it is a stable point then moving the test charge (assumed positive) a small distance from the equilibrium point should result in a restoring force directed back toward the equilibrium point. In other words, there will be a point where the electric field is zero, and around this point there will be an electric field pointing inward. Applying Gauss' law to a small surface surrounding our point P , we have a net inward flux, so there must be a negative charge inside the surface. But there should be nothing inside the surface except an empty point P , so we have a contradiction. P2716 (a) Follow the example on Page 618. By symmetry E = 0 along the median plane. The charge enclosed between the median plane and a surface a distance x from the plane is q = Ax. Then E = Ax/ 0 A = A/ 0 . (b) Outside the slab the charge enclosed between the median plane and a surface a distance x from the plane is is q = Ad/2, regardless of x. The E = Ad/2/ 0 A = d/2 0 . P2717 (a) The total charge is the volume integral over the whole sphere, Q= dV. b r  = (r  b). 3 0 3 0 3 0
This is actually a three dimensional integral, and dV = A dr, where A = 4r2 . Then Q = = dV,
R
S r 4r2 dr, R 0 4S 1 4 = R , R 4 = S R3 .
(b) Put a spherical Gaussian surface inside the sphere centered on the center. We can use Gauss' law here because there is spherical symmetry in the entire problem, both inside and outside the Gaussian surface. Gauss' law states q enc E dA = .
0
39
Since there is spherical symmetry the electric field is normal to the spherical Gaussian surface, and it is everywhere the same on this surface. The dot product simplifies to E dA = E dA, while since E is a constant on the surface we can pull it out of the integral, and we end up with E Now dA = q enc
0
,
dA = 4r2 , where r is the radius of the Gaussian surface, so E= q enc . 4 0 r2
We aren't done yet, because the charge enclosed depends on the radius of the Gaussian surface. We need to do part (a) again, except this time we don't want to do the whole volume of the sphere, we only want to go out as far as the Gaussian surface. Then q enc = = dV,
r
S r 4r2 dr, R 0 4S 1 4 = r , R 4 r4 = S . R Combine these last two results and E = = = S r4 , 4 0 r2 R S r2 , 4 0 R Q r2 . 4 0 R4
In the last line we used the results of part (a) to eliminate S from the expression. P2718 (a) Inside the conductor E = 0, so a Gaussian surface which is embedded in the conductor but containing the hole must have a net enclosed charge of zero. The cavity wall must then have a charge of 3.0 C. (b) The net charge on the conductor is +10.0 C; the charge on the outer surface must then be +13.0 C. P2719 (a) Inside the shell E = 0, so the net charge inside a Gaussian surface embedded in the shell must be zero, so the inside surface has a charge Q. (b) Still Q; the outside has nothing to do with the inside. (c) (Q + q); see reason (a). (d) Yes.
40
Throughout this chapter we will use the convention that V () = 0 unless explicitly stated otherwise. Then the potential in the vicinity of a point charge will be given by Eq. 2818, V = q/4 0 r. E281 (a) Let U12 be the potential energy of the interaction between the two "up" quarks. Then U12 = (8.99109 N m2 /C2 ) (2/3)2 e(1.601019 C) = 4.84105 eV. (1.321015 m)
(b) Let U13 be the potential energy of the interaction between an "up" quark and a "down" quark. Then U13 = (8.99109 N m2 /C2 ) (1/3)(2/3)e(1.601019 C) = 2.42105 eV (1.321015 m)
Note that U13 = U23 . The total electric potential energy is the sum of these three terms, or zero. E282 There are six interaction terms, one for every charge pair. Number the charges clockwise from the upper left hand corner. Then U12 U23 U34 U41 U13 U24 Add these terms and get 2 4 2 The amount of work required is W = U . U= q2 q2 = 0.206 4 0 a 0a = = = = q 2 /4 q 2 /4 q 2 /4 q 2 /4
2 0 a, 0 a, 0 a, 0 a,
= (q) /4 0 ( 2a), = q 2 /4 0 ( 2a).
E283 (a) We build the electron one part at a time; each part has a charge q = e/3. Moving the first part from infinity to the location where we want to construct the electron is easy and takes no work at all. Moving the second part in requires work to change the potential energy to U12 = 1 q1 q2 , 4 0 r
which is basically Eq. 287. The separation r = 2.82 1015 m. Bringing in the third part requires work against the force of repulsion between the third charge and both of the other two charges. Potential energy then exists in the form U13 and U23 , where all three charges are the same, and all three separations are the same. Then U12 = U13 = U12 , so the total potential energy of the system is U =3 1 (e/3)2 3 (1.601019 C/3)2 = = 2.721014 J 4 0 r 4(8.851012 C2 /N m2 ) (2.821015 m)
(b) Dividing our answer by the speed of light squared to find the mass, m= 2.72 1014 J = 3.02 1031 kg. (3.00 108 m/s)2 41
E284 There are three interaction terms, one for every charge pair. Number the charges from the left; let a = 0.146 m. Then U12 U13 U23 = = = (25.5109 C)(17.2109 C) , 4 0 a (25.5109 C)(19.2109 C) , 4 0 (a + x) (17.2109 C)(19.2109 C) . 4 0 x
Add these and set it equal to zero. Then (25.5)(17.2) (25.5)(19.2) (17.2)(19.2) = + , a a+x x which has solution x = 1.405a = 0.205 m. E285 The volume of the nuclear material is 4a3 /3, where a = 8.01015 m. Upon dividing in half each part will have a radius r where 4r3 /3 = 4a3 /6. Consequently, r = a/ 3 2 = 6.351015 m. Each fragment will have a charge of +46e. (a) The force of repulsion is F = (46)2 (1.601019 C)2 = 3000 N 4(8.851012 C2 /N m2 )[2(6.351015 m)]2
(b) The potential energy is U= (46)2 e(1.601019 C) = 2.4108 eV 4(8.851012 C2 /N m2 )2(6.351015 m)
1 2 2 mv0
E286 This is a work/kinetic energy problem: v0 =
= qV . Then
2(1.601019 C)(10.3103 V) = 6.0107 m/s. (9.111031 kg)
E287 (a) The energy released is equal to the charges times the potential through which the charge was moved. Then U = qV = (30 C)(1.0 109 V) = 3.0 1010 J. (b) Although the problem mentions acceleration, we want to focus on energy. The energy will change the kinetic energy of the car from 0 to K f = 3.0 1010 J. The speed of the car is then v= 2K = m 2(3.0 1010 J) = 7100 m/s. (1200 kg)
(c) The energy required to melt ice is given by Q = mL, where L is the latent heat of fusion. Then Q (3.0 1010 J) m= = = 90, 100kg. L (3.33105 J/kg)
42
E288 (a) U = (1.601019 C)(1.23109 V) = 1.971010 J. (b) U = e(1.23109 V) = 1.23109 eV. E289 This is an energy conservation problem: bining, v = q2 2 0 m 1 1  , r1 r2 1 1  , (0.90103 m) (2.5103 m)
1 2 2 mv
= qV ; V = q/4 0 (1/r1  1/r2 ). Com
= =
(3.1106 C)2 2(8.851012 C2 /N m2 )(18106 kg) 2600 m/s.
E2810 This is an energy conservation problem: 1 q2 1 m(2v)2  = mv 2 . 2 4 0 r 2 Rearrange, r = = q2 , 6 0 mv 2 (1.601019 C)2 = 1.42109 m. 6(8.851012 C2 /N m2 )(9.111031 kg)(3.44105 m/s)2 )
E2811 (a) V = (1.601019 C)/4(8.851012 C2 /N m2 )(5.291011 m) = 27.2 V. (b) U = qV = (e)(27.2 V) = 27.2 eV. (c) For uniform circular orbits F = mv 2 /r; the force is electrical, or F = e2 /4 0 r2 . Kinetic energy is K = mv 2 /2 = F r/2, so K= e2 (1.601019 C) = = 13.6 eV. 12 C2 /N m2 )(5.291011 m) 8 0 r 8(8.8510
(d) The ionization energy is (K + U ), or E ion = [(13.6 eV) + (27.2 eV)] = 13.6 eV. E2812 (a) The electric potential at A is VA = 1 4 0 q1 q2 + r1 r2 = (8.99109 N m2 /C) (5.0106 C) (2.0106 C) + (0.15 m) (0.05 m) = 6.0104 V.
The electric potential at B is VB = 1 4 0 q1 q2 + r2 r1 = (8.99109 N m2 /C) (5.0106 C) (2.0106 C) + (0.05 m) (0.15 m) = 7.8105 V.
(b) W = qV = (3.0106 C)(6.0104 V  7.8105 V) = 2.5 J. (c) Since work is positive then external work is converted to electrostatic potential energy.
43
E2813
(a) The magnitude of the electric field would be found from E= F (3.90 1015 N) = = 2.44 104 N/C. q (1.60 1019 C)
(b) The potential difference between the plates is found by evaluating Eq. 2815,
b
V = 
a
E ds.
The electric field between two parallel plates is uniform and perpendicular to the plates. Then E ds = E ds along this path, and since E is uniform,
b b b
V = 
a
E ds = 
a
E ds = E
a
ds = Ex,
where x is the separation between the plates. Finally, V = (2.44 104 N/C)(0.120 m) = 2930 V. E2814 V = Ex, so x = 2 0 2(8.851012 C2 /N m2 ) V = (48 V) = 7.1103 m (0.12106 C/m2 )
E2815 The electric field around an infinitely long straight wire is given by E = /2 0 r. The potential difference between the inner wire and the outer cylinder is given by
b
V = 
a
(/2 0 r) dr = (/2 0 ) ln(a/b).
The electric field near the surface of the wire is then given by E= V (855 V) = 1.32108 V/m. = = 2 0 a a ln(a/b) (6.70107 m) ln(6.70107 m/1.05102 m)
The electric field near the surface of the cylinder is then given by E= V (855 V) = = = 8.43103 V/m. 2 m) ln(6.70107 m/1.05102 m) 2 0 a a ln(a/b) (1.0510
E2816 V = Ex = (1.92105 N/C)(1.50102 m) = 2.88103 V. E2817 (a) This is an energy conservation problem: K= 1 (2)(79)e2 (2)(79)e(1.601019 C) = (8.99109 N m2 /C) = 3.2107 eV 4 0 r (7.01015 m)
(b) The alpha particles used by Rutherford never came close to hitting the gold nuclei. E2818 This is an energy conservation problem: mv 2 /2 = eq/4 0 r, or v= (1.601019 C)(1.761015 C) = 2.13104 m/s m2 )(1.22102 m)(9.111031 kg)
2(8.851012 C2 /N
44
E2819
(a) We evaluate VA and VB individually, and then find the difference. VA = 1 q 1 (1.16C) = = 5060 V, 12 C2 /N m2 ) (2.06 m) 4 0 r 4(8.85 10 1 q 1 (1.16C) = = 8910 V, 4 0 r 4(8.85 1012 C2 /N m2 ) (1.17 m)
and VB =
The difference is then VA  VB = 3850 V. (b) The answer is the same, since when concerning ourselves with electric potential we only care about distances, and not directions. E2820 The number of "excess" electrons on each grain is n= 4 0 rV 4(8.851012 C2 /N m)(1.0106 m)(400 V) = = 2.8105 e (1.601019 C)
E2821 The excess charge on the shuttle is q = 4 0 rV = 4(8.851012 C2 /N m)(10 m)(1.0 V) = 1.1109 C E2822 q = 1.37105 C, so V = (8.99109 N m2 /C2 ) E2823 (1.37105 C) = 1.93108 V. (6.37106 m)
The ratio of the electric potential to the electric field strength is V = E 1 q 4 0 r / 1 q 4 0 r2 = r.
In this problem r is the radius of the Earth, so at the surface of the Earth the potential is V = Er = (100 V/m)(6.38106 m) = 6.38108 V. E2824 Use Eq. 2822: V = (8.99109 N m2 /C2 ) (1.47)(3.341030 C m) = 1.63105 V. (52.0109 m)2
E2825 (a) When finding VA we need to consider the contribution from both the positive and the negative charge, so 1 q VA = qa + 4 0 a+d There will be a similar expression for VB , VB = 1 4 0 qa + q a+d .
45
Now to evaluate the difference. V A  VB = = = = q 1 1 qa +  4 0 a+d 4 0 q 1 1  , 2 0 a a + d q a+d a  2 0 a(a + d) a(a + d) q d . 2 0 a(a + d) qa + q a+d ,
,
(b) Does it do what we expect when d = 0? I expect it the difference to go to zero as the two points A and B get closer together. The numerator will go to zero as d gets smaller. The denominator, however, stays finite, which is a good thing. So yes, Va  VB 0 as d 0. E2826 (a) Since both charges are positive the electric potential from both charges will be positive. There will be no finite points where V = 0, since two positives can't add to zero. (b) Between the charges the electric field from each charge points toward the other, so E will vanish when q/x2 = 2q/(d  x)2 . This happens when d  x = 2x, or x = d/(1 + 2). E2827 The distance from C to either charge is 2d/2 = 1.39102 m. (a) V at C is 2(2.13106 C) V = (8.99109 N m2 /C2 ) = 2.76106 V (1.39102 m) (b) W = qV = (1.91106 C)(2.76106 V) = 5.27 J. (c) Don't forget about the potential energy of the original two charges! U0 = (8.99109 N m2 /C2 ) Add this to the answer from part (b) to get 7.35 J. E2828 The potential is given by Eq. 2832; at the surface V s = R/2 0 , half of this occurs when R2 + z 2  z = R/2, R2 + z 2 = R2 /4 + Rz + z 2 , 3R/4 = z. E2829 We can find the linear charge density by dividing the charge by the circumference, = (2.13106 C)2 = 2.08 J (1.96102 m)
Q , 2R where Q refers to the charge on the ring. The work done to move a charge q from a point x to the origin will be given by W W = qV, = q (V (0)  V (x)) , 1 Q 1 Q  = q 2 + x2 4 0 R 4 0 R2 qQ 1 1 . =  2 + x2 4 0 R R 46
,
Putting in the numbers, (5.931012 C)(9.12109 C) 4(8.851012 C2 /N m2 ) 1  1.48m 1 (1.48m)2 + (3.07m)2 = 1.861010 J.
E2830 (a) The electric field strength is greatest where the gradient of V is greatest. That is between d and e. (b) The least absolute value occurs where the gradient is zero, which is between b and c and again between e and f . E2831 The potential on the positive plate is 2(5.52 V) = 11.0 V; the electric field between the plates is E = (11.0 V)/(1.48102 m) = 743 V/m. E2832 Take the derivative: E = V /z. E2833 field, The radial potential gradient is just the magnitude of the radial component of the electric Er =  Then V r =  = 1 q , 4 0 r2 1 V r
79(1.60 1019 C) , 4(8.85 1012 C2 /N m2 ) (7.0 1015 m)2
= 2.321021 V/m. E2834 Evaluate V /r, and E= Ze 4 0 1 r +2 3 2 r 2R .
E2835 Ex = V /x = 2(1530 V/m2 )x. At the point in question, E = 2(1530 V/m2 )(1.28 102 m) = 39.2 V/m. E2836 Draw the wires so that they are perpendicular to the plane of the page; they will then "come out of" the page. The equipotential surfaces are then lines where they intersect the page, and they look like
47
E2837 (a) VB  VA  = W/q = (3.94 1019 J)/(1.60 1019 C) = 2.46 V. The electric field did work on the electron, so the electron was moving from a region of low potential to a region of high potential; or VB > VA . Consequently, VB  VA = 2.46 V. (b) VC is at the same potential as VB (both points are on the same equipotential line), so VC  VA = VB  VA = 2.46 V. (c) VC is at the same potential as VB (both points are on the same equipotential line), so VC  VB = 0 V. E2838 (a) For point charges r = q/4 0 V , so r = (8.99109 N m2 /C2 )(1.5108 C)/(30 V) = 4.5 m (b) No, since V 1/r. E2839 The dotted lines are equipotential lines, the solid arrows are electric field lines. Note that there are twice as many electric field lines from the larger charge!
48
E2840 The dotted lines are equipotential lines, the solid arrows are electric field lines.
E2841 This can easily be done with a spreadsheet. The following is a sketch; the electric field is the bold curve, the potential is the thin curve.
49
sphere radius
r
E2842 Originally V = q/4 0 r, where r is the radius of the smaller sphere. (a) Connecting the spheres will bring them to the same potential, or V1 = V2 . (b) q1 + q2 = q; V1 = q1 /4 0 r and V2 = q2 /4 0 2r; combining all of the above q2 = 2q1 and q1 = q/3 and q2 = 2q/3. E2843 (a) q = 4R2 , so V = q/4 0 R = R/ 0 , or V = (1.601019 C/m2 )(6.37106 m)/(8.851012 C2 /N m2 ) = 0.115 V (b) Pretend the Earth is a conductor, then E = /epsilon0 , so E = (1.601019 C/m2 )/(8.851012 C2 /N m2 ) = 1.81108 V/m. E2844 V = q/4 0 R, so V = (8.99109 N m2 /C2 )(15109 C)/(0.16 m) = 850 V. E2845 (a) q = 4 0 RV = 4(8.851012 C2 /N m2 )(0.152 m)(215 V) = 3.63109 C (b) = q/4R2 = (3.63109 C)/4(0.152 m)2 = 1.25108 C/m2 . E2846 The dotted lines are equipotential lines, the solid arrows are electric field lines.
50
E2847 (a) The total charge (Q = 57.2nC) will be divided up between the two spheres so that they are at the same potential. If q1 is the charge on one sphere, then q2 = Q  q1 is the charge on the other. Consequently V1 1 q1 4 0 r1 q 1 r2 q1 Putting in the numbers, we find q1 = Qr1 (57.2 nC)(12.2 cm) = = 38.6 nC, r2 + r1 (5.88 cm) + (12.2 cm) = V2 , 1 Q  q1 = , 4 0 r2 = (Q  q1 )r1 , Qr2 = . r2 + r1
and q2 = Q  q1 = (57.2 nC)  (38.6 nC) = 18.6 nC. (b) The potential on each sphere should be the same, so we only need to solve one. Then 1 q1 1 (38.6 nC) = = 2850 V. 12 C2 /N m2 ) (12.2 cm) 4 0 r1 4(8.85 10 E2848 (a) V = (8.99109 N m2 /C2 )(31.5109 C)/(0.162 m) = 1.75103 V. (b) V = q/4 0 r, so r = q/4 0 V , and then r = (8.99109 N m2 /C2 )(31.5109 C)/(1.20103 V) = 0.236 m. That is (0.236 m)  (0.162 m) = 0.074 m above the surface. 51
E2849
(a) Apply the point charge formula, but solve for the charge. Then 1 q 4 0 r q q = V, = = 4 0 rV, 4(8.85 1012 C2 /N m2 )(1 m)(106 V) = 0.11 mC.
Now that's a fairly small charge. But if the radius were decreased by a factor of 100, so would the charge (1.10 C). Consequently, smaller metal balls can be raised to higher potentials with less charge. (b) The electric field near the surface of the ball is a function of the surface charge density, E = / 0 . But surface charge density depends on the area, and varies as r2 . For a given potential, the electric field near the surface would then be given by E=
0
=
q 4
0
r2
=
V . r
Note that the electric field grows as the ball gets smaller. This means that the break down field is more likely to be exceeded with a low voltage small ball; you'll get sparking. E2850 A "Volt" is a Joule per Coulomb. The power required by the drive belt is the product (3.41106 V)(2.83103 C/s) = 9650 W. P281 (a) According to Newtonian mechanics we want K = 1 mv 2 to be equal to W = qV 2 which means mv 2 (0.511 MeV) V = = = 256 kV. 2q 2e mc2 is the rest mass energy of an electron. (b) Let's do some rearranging first. K K mc2 = mc2 = 1 1  2 1 1 1  2  1, 1 ,
K , +1 = mc2 1  2 1 = 1  2, K mc2 + 1 1 = 1  2, 2 K mc2 + 1 and finally, = Putting in the numbers, 1 so v = 0.746c. 52
(256 (511
1
1
K mc2
+1
2
1 keV) + 1 keV)
2
= 0.746,
P282 (a) The potential of the hollow sphere is V = q/4 0 r. The work required to increase the charge by an amount dq is dW = V /, dq. Integrating,
e
W =
0
e2 q dq = . 4 0 r 8 0 r
This corresponds to an electric potential energy of W = 8(8.851012 C2 /N e(1.601019 C) = 2.55105 eV = 4.081014 J. m2 )(2.821015 m)
(b) This would be a mass of m = (4.081014 J)/(3.00108 m/s)2 = 4.531031 kg. P283 The negative charge is held in orbit by electrostatic attraction, or mv 2 qQ = . r 4 0 r2 The kinetic energy of the charge is K= The electrostatic potential energy is U = so the total energy is E= The work required to change orbit is then W = P284 (a) V =  E dr, so
r
1 qQ mv 2 = . 2 8 0 r qQ , 4 0 r qQ . 8 0 r
qQ 8 0
1 1  r1 r2
.
V =
0
qr qr2 dr =  . 3 4 0 R 8 0 R3
(b) V = q/8 0 R. (c) If instead of V = 0 at r = 0 as was done in part (a) we take V = 0 at r = , then V = q/4 0 R on the surface of the sphere. The new expression for the potential inside the sphere will look like V = V + Vs , where V is the answer from part (a) and Vs is a constant so that the surface potential is correct. Then Vs = and then V = q 4 0 R + qR2 3qR2 = , 8 0 R3 8 0 R3
qr2 3qR2 q(3R2  r2 ) + = . 3 3 8 0 R 8 0 R 8 0 R3
53
P285 The total electric potential energy of the system is the sum of the three interaction pairs. One of these pairs does not change during the process, so it can be ignored when finding the change in potential energy. The change in electrical potential energy is then U = 2 q2 q2 q2 2 = 4 0 rf 4 0 ri 2 0 1 1  rf ri .
In this case ri = 1.72 m, while rf = 0.86 m. The change in potential energy is then U = 2(8.99109 N m2 /C2 )(0.122 C)2 The time required is t = (1.56108 )/(831 W) = 1.87105 s = 2.17 days. P286 (a) Apply conservation of energy: K= qQ qQ , or d = , 4 0 d 4 0 K 1 1  (0.86 m) (1.72 m) = 1.56108 J
where d is the distance of closest approach. (b) Apply conservation of energy: K= 1 qQ + mv 2 , 4 0 (2d) 2 K/m.
so, combining with the results in part (a), v = P287
(a) First apply Eq. 2818, but solve for r. Then r= q 4 0 V = (32.0 1012 C) = 562 m. 4(8.85 1012 C2 /N m2 )(512 V)
(b) If two such drops join together the charge doubles, and the volume of water doubles, but the radius of the new drop only increases by a factor of 3 2 = 1.26 because volume is proportional to the radius cubed. The potential on the surface of the new drop will be V new = = = The new potential is 813 V. P288 (a) The work done is W = F z = Eqz = qz/2 0 . (b) Since W = qV , V = z/2 0 , so V = V0  (/2 0 )z. 1 q new , 4 0 rnew 1 2q old , 4 0 3 2 rold 1 q old (2)2/3 = (2)2/3 V old . 4 0 rold
54
P289
(a) The potential at any point will be the sum of the contribution from each charge, V = 1 q1 1 q2 + , 4 0 r1 4 0 r2
where r1 is the distance the point in question from q1 and r2 is the distance the point in question from q2 . Pick a point, call it (x, y). Since q1 is at the origin, r1 = Since q2 is at (d, 0), where d = 9.60 nm, r2 = (x  d)2 + y 2 . x2 + y 2 .
Define the "Stanley Number" as S = 4 0 V . Equipotential surfaces are also equiStanley surfaces. In particular, when V = 0, so does S. We can then write the potential expression in a sightly simplified form q1 q2 S= + . r1 r2 If S = 0 we can rearrange and square this expression. q1 r1 2 r1 2 q1 x2 + y 2 2 q1 Let = q2 /q1 , then we can write 2 x2 + y 2 2 x2 + 2 y 2 (  1)x + 2xd + (2  1)y 2
2 2
=  = =
q2 , r2
2 r2 2, q2 (x  d)2 + y 2 , 2 q2
=
(x  d)2 + y 2 ,
= x2  2xd + d2 + y 2 , = d2 .
We complete the square for the (2  1)x2 + 2xd term by adding d2 /(2  1) to both sides of the equation. Then 2 d 1 (2  1) x + 2 + y 2 = d2 1 + 2 . 1 1 The center of the circle is at  2 d (9.60 nm) = = 5.4 nm. 1 (10/6)2  1
(b) The radius of the circle is 1+ d2 which can be simplified to d (c) No. 55 (10/6) = (9.6 nm) = 9.00 nm. 2  1 (10/6)2  1
1 2 1
2  1
,
P2810 An annulus is composed of differential rings of varying radii r and width dr; the charge on any ring is the product of the area of the ring, dA = 2r dr, and the surface charge density, or dq = dA = k 2k 2r dr = 2 dr. 3 r r
The potential at the center can be found by adding up the contributions from each ring. Since we are at the center, the contributions will each be dV = dq/4 0 r. Then
b
V =
a
k k dr = 3 2 0r 4 0
1 1  2 2 a b
.=
k b2  a2 . 4 0 b2 a2
The total charge on the annulus is
b
Q=
a
2k dr = 2k r2
1 1  a b
= 2k
ba . ba
Combining, V = P2811 Q a+b . 8 0 ab r.
Add the three contributions, and then do a series expansion for d V = = q 1 1 1 + + , 4 0 r + d r rd q 1 1 +1+ , 4 0 r 1 + d/r 1  d/r d d q 1 + + 1 + 1 + , 4 0 r r r q 2d 1+ . 4 0 r r
P2812
(a) Add the contributions from each differential charge: dq = dy. Then
y+L
V =
y
dy = ln 4 0 y 4 0
y+L y
.
(b) Take the derivative: Ey =  V y L L = = . y 4 0 y + L y 2 4 0 y(y + L)
(c) By symmetry it must be zero, since the system is invariant under rotations about the axis of the rod. Note that we can't determine E from derivatives because we don't have the functional form of V for points offaxis! P2813 (a) We follow the work done in Section 286 for a uniform line of charge, starting with Eq. 2826, dV dV = = 1 4 0 1 4 0 dx x2 + y 2
L 0
, ,
kx dx x2 + y 2
56
= =
k 4 0 k 4 0
x2 + y 2
L
,
0
L2 + y 2  y .
(b) The y component of the electric field can be found from Ey =  which (using a computeraided math program) is Ey = k 4 0 1 y L2 + y2 . V , y
(c) We could find Ex if we knew the x variation of V . But we don't; we only found the values of V along a fixed value of x. (d) We want to find y such that the ratio k 4 0 is onehalf. Simplifying, L2 + y 2  y / k (L) 4 0
L2 + y 2  y = L/2, which can be written as L2 + y 2 = L2 /4 + Ly + y 2 ,
or 3L2 /4 = Ly, with solution y = 3L/4. P2814 The spheres are small compared to the separation distance. Assuming only one sphere at a potential of 1500 V, the charge would be q = 4 0 rV = 4(8.851012 C2 /N m)(0.150 m)(1500 V) = 2.50108 C. The potential from the sphere at a distance of 10.0 m would be V = (1500 V) (0.150 m) = 22.5 V. (10.0 m)
This is small compared to 1500 V, so we will treat it as a perturbation. This means that we can assume that the spheres have charges of q = 4 0 rV = 4(8.851012 C2 /N m)(0.150 m)(1500 V + 22.5 V) = 2.54108 C. P2815 Calculating the fraction of excess electrons is the same as calculating the fraction of excess charge, so we'll skip counting the electrons. This problem is effectively the same as Exercise 2847; we have a total charge that is divided between two unequal size spheres which are at the same potential on the surface. Using the result from that exercise we have q1 = Qr1 , r2 + r1
where Q = 6.2 nC is the total charge available, and q1 is the charge left on the sphere. r1 is the radius of the small ball, r2 is the radius of Earth. Since the fraction of charge remaining is q1 /Q, we can write q1 r1 r1 = = 2.0 108 . Q r 2 + r1 r2 57
P2816
The positive charge on the sphere would be q = 4 0 rV = 4(8.851012 C2 /N m2 )(1.08102 m)(1000 V) = 1.20109 C.
The number of decays required to build up this charge is n = 2(1.20109 C)/(1.601019 C) = 1.501010 . The extra factor of two is because only half of the decays result in an increase in charge. The time required is t = (1.501010 )/(3.70108 s1 ) = 40.6 s. P2817 (a) None. (b) None. (c) None. (d) None. (e) No. P2818 (a) Outside of an isolated charged spherical object E = q/4 0 r2 and V = q/4 0 r. Then E = V /r. Consequently, the sphere must have a radius larger than r = (9.15106 V)/(100 106 V/m) = 9.15102 m. (b) The power required is (320106 C/s)(9.15106 V) = 2930 W. (c) wv = (320106 C/s), so = (320106 C/s) = 2.00105 C/m2 . (0.485 m)(33.0 m/s)
58
E291 (a) The charge which flows through a cross sectional surface area in a time t is given by q = it, where i is the current. For this exercise we have q = (4.82 A)(4.60 60 s) = 1330 C as the charge which passes through a cross section of this resistor. (b) The number of electrons is given by (1330 C)/(1.60 1019 C) = 8.31 1021 electrons. E292 Q/t = (200106 A/s)(60s/min)/(1.601019 C) = 7.51016 electrons per minute. E293 (a) j = nqv = (2.101014 /m3 )2(1.601019 C)(1.40105 m/s) = 9.41 A/m2 . Since the ions have positive charge then the current density is in the same direction as the velocity. (b) We need an area to calculate the current. E294 (a) j = i/A = (1231012 A)/(1.23103 m)2 = 2.59105 A/m2 . (b) v d = j/ne = (2.59105 A/m2 )/(8.491028 /m3 )(1.601019 C) = 1.911015 m/s. E295 The current rating of a fuse of cross sectional area A would be imax = (440 A/cm2 )A, and if the fuse wire is cylindrical A = d2 /4. Then d= 4 (0.552 A) = 4.00102 cm. (440 A/m2 )
E296 Current density is current divided by cross section of wire, so the graph would look like:
4
I (A/mil^2 x10^3)
3
2
1
50
100
59
150
200
d(mils)
E297 The current is in the direction of the motion of the positive charges. The magnitude of the current is i = (3.11018 /s + 1.11018 /s)(1.601019 C) = 0.672 A. E298 (a) The total current is i = (3.501015 /s + 2.251015 /s)(1.601019 C) = 9.20104 A. (b) The current density is j = (9.20104 A)/(0.165103 m)2 = 1.08104 A/m2 . E299 (a) j = (8.70106 /m3 )(1.601019 C)(470103 m/s) = 6.54107 A/m2 . (b) i = (6.54107 A/m2 )(6.37106 m)2 = 8.34107 A. E2910 i = wv, so = (95.0106 A)/(0.520 m)(28.0 m/s) = 6.52106 C/m2 . E2911 The drift velocity is given by Eq. 296, j i (115 A) = = = 2.71104 m/s. ne Ane (31.2106 m2 )(8.491028 /m3 )(1.601019 C)
vd =
The time it takes for the electrons to get to the starter motor is t= That's about 54 minutes. E2912 V = iR = (50103 A)(1800 ) = 90 V. E2913 The resistance of an object with constant cross section is given by Eq. 2913, R= L (11, 000 m) = (3.0 107 m) = 0.59 . A (0.0056 m2 ) x (0.855 m) = = 3.26103 s. v (2.71104 m/s)
E2914 The slope is approximately [(8.2  1.7)/1000] cm/ C, so = 1 6.5103 cm/ C 4103 /C 1.7 cm
E2915 (a) i = V /R = (23 V)/(15103 ) = 1500 A. (b) j = i/A = (1500 A)/(3.0103 m)2 = 5.3107 A/m2 . (c) = RA/L = (15103 )(3.0103 m)2 /(4.0 m) = 1.1107 m. The material is possibly platinum. E2916 Use the equation from Exercise 2917. R = 8 ; then T = (8 )/(50 )(4.3103 /C ) = 37 C . The final temperature is then 57 C. 60
E2917
Start with Eq. 2916,  0 = 0 av (T  T0 ),
and multiply through by L/A, L L (  0 ) = 0 av (T  T0 ), A A to get R  R0 = R0 av (T  T0 ). E2918 The wire has a length L = (250)2(0.122 m) = 192 m. The diameter is 0.129 inches; the cross sectional area is then A = (0.129 0.0254 m)2 /4 = 8.43106 m2 . The resistance is R = L/A = (1.69108 m)(192 m)/(8.43106 m2 ) = 0.385 . E2919 If the length of each conductor is L and has resistivity , then RA = and RB = The ratio of the resistances is then L 4L = D2 /4 D2
4L L = . (4D2 /4  D2 /4) 3D2 RA = 3. RB
E2920 R = R, so 1 L1 /(d1 /2)2 = 2 L2 /(d2 /2)2 . Simplifying, 1 /d2 = 2 /d2 . Then 1 2 d2 = (1.19103 m) (9.68108 m)/(1.69108 m) = 2.85103 m.
E2921 (a) (750103 A)/(125) = 6.00103 A. (b) V = iR = (6.00103 A)(2.65106 ) = 1.59108 V. (c) R = V /i = (1.59108 V)/(750103 A) = 2.12108 . E2922 Since V = iR, then if V and i are the same, then R must be the same. 2 2 2 2 (a) Since R = R, 1 L1 /r1 = 2 L2 /r2 , or 1 /r1 = 2 /r2 . Then riron /rcopper = (9.68108 m)(1.69108 m) = 2.39.
(b) Start with the definition of current density: j= i V V = = . A RA L
Since V and L is the same, but is different, then the current densities will be different.
61
E2923 Conductivity is given by Eq. 298, j = E. If the wire is long and thin, then the magnitude of the electric field in the wire will be given by E V /L = (115 V)/(9.66 m) = 11.9 V/m. We can now find the conductivity, = (1.42104 A/m2 ) j = = 1.19103 ( m)1 . E (11.9 V/m)
E2924 (a) v d = j/en = E/en. Then v d = (2.701014 / m)(120 V/m)/(1.601019 C)(620106 /m3 + 550106 /m3 ) = 1.73102 m/s. (b) j = E = (2.701014 / m)(120 V/m) = 3.241014 A/m2 . E2925 (a) R/L = /A, so j = i/A = (R/L)i/. For copper, j = (0.152103 /m)(62.3 A)/(1.69108 m) = 5.60105 A/m2 ; for aluminum, j = (0.152103 /m)(62.3 A)/(2.75108 m) = 3.44105 A/m2 . (b) A = L/R; if is density, then m = lA = l/(R/L). For copper, m = (1.0 m)(8960 kg/m3 )(1.69108 m)/(0.152103 /m) = 0.996 kg; for aluminum, m = (1.0 m)(2700 kg/m3 )(2.75108 m)/(0.152103 /m) = 0.488 kg. E2926 The resistance for potential differences less than 1.5 V are beyond the scale.
10 8 6 4 2
R (Kiloohms)
1
2
3
4
V(Volts)
62
E2927
(a) The resistance is defined as R= V (3.55 106 V/A2 )i2 = = (3.55 106 V/A2 )i. i i
When i = 2.40 mA the resistance would be R = (3.55 106 V/A2 )(2.40 103 A) = 8.52 k. (b) Invert the above expression, and i = R/(3.55 106 V/A2 ) = (16.0 )/(3.55 106 V/A2 ) = 4.51 A. E2928 First, n = 3(6.021023 )(2700 kg/m3 )(27.0103 kg) = 1.811029 /m3 . Then = m (9.111031 kg) = = 7.151015 s. 2 29 /m3 )(1.601019 C)2 (2.75108 m) ne (1.8110
E2929 (a) E = E0 /e = q/4 0 e R2 , so E= (1.00106 C) = 4(8.851012 C2 /N m2 )(4.7)(0.10 m)2
(b) E = E0 = q/4 0 R2 , so E= (c) ind =
0 (E0
(1.00106 C) = 4(8.851012 C2 /N m2 )(0.10 m)2
 E) = q(1  1/e )/4R2 . Then ind = (1.00106 C) 4(0.10 m)2 1 1 (4.7) = 6.23106 C/m2 .
E2930 Midway between the charges E = q/ 0 d, so q = (8.851012 C2 /N m2 )(0.10 m)(3106 V/m) = 8.3106 C. E2931 (a) At the surface of a conductor of radius R with charge Q the magnitude of the electric field is given by 1 E= QR2 , 4 0 while the potential (assuming V = 0 at infinity) is given by V = 1 QR. 4 0
The ratio is V /E = R. The potential on the sphere that would result in "sparking" is V = ER = (3106 N/C)R. (b) It is "easier" to get a spark off of a sphere with a smaller radius, because any potential on the sphere will result in a larger electric field. (c) The points of a lighting rod are like small hemispheres; the electric field will be large near these points so that this will be the likely place for sparks to form and lightning bolts to strike. 63
P291 If there is more current flowing into the sphere than is flowing out then there must be a change in the net charge on the sphere. The net current is the difference, or 2 A. The potential on the surface of the sphere will be given by the pointcharge expression, V = 1 q , 4 0 r
and the charge will be related to the current by q = it. Combining, V = or t= 1 it , 4 0 r
4 0 V r 4(8.85 1012 C2 /N m2 )(980 V)(0.13 m) = = 7.1 ms. i (2 A)
P292 The net current density is in the direction of the positive charges, which is to the east. There are two electrons for every alpha particle, and each alpha particle has a charge equal in magnitude to two electrons. The current density is then j = q e ne v e + q + n v , = (1.61019 C)(5.61021 /m3 )(88 m/s) + (3.21019 C)(2.81021 /m3 )(25 m/s), = 1.0105 C/m2 . (a) The resistance of the segment of the wire is R = L/A = (1.69108 m)(4.0102 m)/(2.6103 m)2 = 3.18105 . The potential difference across the segment is V = iR = (12 A)(3.18105 ) = 3.8104 V. (b) The tail is negative. (c) The drift speed is v = j/en = i/Aen, so v = (12 A)/(2.6103 m)2 (1.61019 C)(8.491028 /m3 ) = 4.16105 m/s. The electrons will move 1 cm in (1.0102 m)/(4.16105 m/s) = 240 s. P294 (a) N = it/q = (250109 A)(2.9 s)/(3.21019 C) = 2.271012 . (b) The speed of the particles in the beam is given by v = 2K/m, so v= 2(22.4 MeV)/4(932 MeV/c2 ) = 0.110c.
P293
It takes (0.180 m)/(0.110)(3.00108 m/s) = 5.45109 s for the beam to travel 18.0 cm. The number of charges is then N = it/q = (250109 A)(5.45109 s)/(3.21019 C) = 4260. (c) W = qV , so V = (22.4 MeV)/2e = 11.2 MV.
64
P295
(a) The time it takes to complete one turn is t = (250 m)/c. The total charge is q = it = (30.0 A)(950 m)/(3.00108 m/s) = 9.50105 C.
(b) The number of charges is N = q/e, the total energy absorbed by the block is then U = (28.0109 eV)(9.50105 C)/e = 2.66106 J. This will raise the temperature of the block by T = U/mC = (2.66106 J)/(43.5 kg)(385J/kgC ) = 159 C . P296 (a) i = j dA = 2 i = 2 (b) Integrate, again: i = 2 P297 0R j0 (r/R)r dr = 2j0 (R3 /3R) = j0 R2 /3. jr dr;
0R j0 (1  r/R)r dr = 2j0 (R2 /2  R3 /3R) = j0 R2 /6.
(a) Solve 20 = 0 [1 + (T  20 C)], or T = 20 C + 1/(4.3103 /C ) = 250 C.
(b) Yes, ignoring changes in the physical dimensions of the resistor. P298 The resistance when on is (2.90 V)/(0.310 A) = 9.35 . The temperature is given by T = 20 C + (9.35  1.12 )/(1.12 )(4.5103 / C) = 1650 C. P299 Originally we have a resistance R1 made out of a wire of length l1 and cross sectional area A1 . The volume of this wire is V1 = A1 l1 . When the wire is drawn out to the new length we have l2 = 3l1 , but the volume of the wire should be constant so A2 l2 = A1 l1 , A2 (3l1 ) = A1 l1 , A2 = A1 /3. The original resistance is R1 = The new resistance is R2 = or R2 = 54 . P2910 (a) i = (35.8 V)/(935 ) = 3.83102 A. (b) j = i/A = (3.83102 A)/(3.50104 m2 ) = 109 A/m2 . (c) v = (109 A/m2 )/(1.61019 C)(5.331022 /m3 ) = 1.28102 m/s. (d) E = (35.8 V)/(0.158 m) = 227 V/m. 65 l1 . A1
l2 3l1 = = 9R1 , A2 A1 /3
P2911 (a) = (1.09103 )(5.5103 m)2 /4(1.6 m) = 1.62108 m. This is possibly silver. (b) R = (1.62108 m)(1.35103 m)4/(2.14102 m)2 = 6.08108 . P2912 (a) L/L = 1.7105 for a temperature change of 1.0 C . Area changes are twice this, or A/A = 3.4105 . Take the differential of RA = L: R dA+A dR = dL+L d, or dR = dL/A+L d/AR dA/A. For finite changes this can be written as R L A = +  . R L A / = 4.3103 . Since this term is so much larger than the other two it is the only significant effect. P2913 We will use the results of Exercise 2917, R  R0 = R0 av (T  T0 ). To save on subscripts we will drop the "av" notation, and just specify whether it is carbon "c" or iron "i". The disks will be effectively in series, so we will add the resistances to get the total. Looking only at one disk pair, we have Rc + Ri = R0,c (c (T  T0 ) + 1) + R0,i (i (T  T0 ) + 1) , = R0,c + R0,i + (R0,c c + R0,i i ) (T  T0 ).
This last equation will only be constant if the coefficient for the term (T  T0 ) vanishes. Then R0,c c + R0,i i = 0, but R = L/A, and the disks have the same cross sectional area, so Lc c c + Li i i = 0, or Lc i i (9.68108 m)(6.5103 /C ) = = = 0.036. Li c c (3500108 m)(0.50103 /C )
P2914 The current entering the cone is i. The current density as a function of distance x from the left end is then i j= . [a + x(b  a)/L]2 The electric field is given by E = j. The potential difference between the ends is then
L L
V =
0
E dx =
0
i iL dx = 2 [a + x(b  a)/L] ab
The resistance is R = V /i = L/ab.
66
P2915
The current is found from Eq. 295, i= j dA,
where the region of integration is over a spherical shell concentric with the two conducting shells but between them. The current density is given by Eq. 2910, j = E/, and we will have an electric field which is perpendicular to the spherical shell. Consequently, i= 1 E dA = 1 E dA
By symmetry we expect the electric field to have the same magnitude anywhere on a spherical shell which is concentric with the two conducting shells, so we can bring it out of the integral sign, and then 1 4r2 E i = E dA = , where E is the magnitude of the electric field on the shell, which has radius r such that b > r > a. The above expression can be inverted to give the electric field as a function of radial distance, since the current is a constant in the above expression. Then E = i/4r2 The potential is given by
a
V = 
b
E ds,
we will integrate along a radial line, which is parallel to the electric field, so
a
V
= 
b a
E dr,
= 
i dr, 4r2 b i a dr =  , 4 b r i 1 1 =  . 4 a b
We divide this expression by the current to get the resistance. Then R= 4 1 1  a b
P2916 Since = d , v d . For an ideal gas the kinetic energy is proportional to the /v temperature, so K T .
67
E301
We apply Eq. 301, q = CV = (50 1012 F)(0.15 V) = 7.5 1012 C;
E302 (a) C = V /q = (73.01012 C)/(19.2 V) = 3.801012 F. (b) The capacitance doesn't change! (c) V = q/C = (2101012 C)/(3.801012 F) = 55.3 V. E303 q = CV = (26.0106 F)(125 V) = 3.25103 C. E304 (a) C = 0 A/d = (8.851012 F/m)(8.22102 m)2 /(1.31103 m) = 1.431010 F. (b) q = CV = (1.431010 F)(116 V) = 1.66108 C. E305 Eq. 3011 gives the capacitance of a cylinder, C = 2
0
L (0.0238 m) = 2(8.851012 F/m) = 5.461013 F. ln(b/a) ln((9.15mm)/(0.81mm))
E306 (a) A = Cd/ 0 = (9.701012 F)(1.20103 m)/(8.851012 F/m) = 1.32103 m2 . (b) C = C0 d0 /d = (9.701012 F)(1.20103 m)/(1.10103 m) = 1.061011 F. (c) V = q0 /C = [V ]0 C0 /C = [V ]0 d/d0 . Using this formula, the new potential difference would be [V ]0 = (13.0 V)(1.10103 m)/(1.20103 m) = 11.9 V. The potential energy has changed by (11.9 V)  (30.0 V) = 1.1 V. E307 (a) From Eq. 308, C = 4(8.851012 F/m) (b) A = Cd/
0
(0.040 m)(0.038 m) = 8.451011 F. (0.040 m)  (0.038 m)
= (8.451011 F)(2.00103 m)/(8.851012 F/m) = 1.91102 m2 .
E308 Let a = b + d, where d is the small separation between the shells. Then C = (b + d)b ab = 4 0 , ab d b2 4 0 = 0 A/d. d 4
0
E309 The potential difference across each capacitor in parallel is the same; it is equal to 110 V. The charge on each of the capacitors is then q = CV = (1.00 106 F)(110 V) = 1.10 104 C. If there are N capacitors, then the total charge will be N q, and we want this total charge to be 1.00 C. Then (1.00 C) (1.00 C) N= = = 9090. q (1.10 104 C)
68
E3010 First find the equivalent capacitance of the parallel part: C eq = C1 + C2 = (10.3106 F) + (4.80106 F) = 15.1106 F. Then find the equivalent capacitance of the series part: 1 1 1 = + = 3.23105 F1 . 6 F) C eq (15.110 (3.90106 F) Then the equivalent capacitance of the entire arrangement is 3.10106 F. E3011 First find the equivalent capacitance of the series part: 1 1 1 = + = 3.05105 F1 . C eq (10.3106 F) (4.80106 F) The equivalent capacitance is 3.28106 F. Then find the equivalent capacitance of the parallel part: C eq = C1 + C2 = (3.28106 F) + (3.90106 F) = 7.18106 F. This is the equivalent capacitance for the entire arrangement. E3012 For one capacitor q = CV = (25.0106 F)(4200 V) = 0.105 C. There are three capacitors, so the total charge to pass through the ammeter is 0.315 C. E3013 (a) The equivalent capacitance is given by Eq. 3021, 1 1 1 1 1 5 = + = + = C eq C1 C2 (4.0F) (6.0F) (12.0F) or C eq = 2.40F. (b) The charge on the equivalent capacitor is q = CV = (2.40F)(200 V) = 0.480 mC. For series capacitors, the charge on the equivalent capacitor is the same as the charge on each of the capacitors. This statement is wrong in the Student Solutions! (c) The potential difference across the equivalent capacitor is not the same as the potential difference across each of the individual capacitors. We need to apply q = CV to each capacitor using the charge from part (b). Then for the 4.0F capacitor, V = and for the 6.0F capacitor, q (0.480 mC) = = 80 V. C (6.0F) Note that the sum of the potential differences across each of the capacitors is equal to the potential difference across the equivalent capacitor. V = E3014 (a) The equivalent capacitance is C eq = C1 + C2 = (4.0F) + (6.0F) = (10.0F). (c) For parallel capacitors, the potential difference across the equivalent capacitor is the same as the potential difference across either of the capacitors. (b) For the 4.0F capacitor, q = CV = (4.0F)(200 V) = 8.0104 C; and for the 6.0F capacitor, q = CV = (6.0F)(200 V) = 12.0104 C. 69 q (0.480 mC) = = 120 V; C (4.0F)
E3015 (a) C eq = C + C + C = 3C; deq = (b) 1/C eq = 1/C + 1/C + 1/C = 3/C; deq =
0A 0A = = 3d. C eq C/3
d 0A 0A = = . C eq 3C 3
E3016 (a) The maximum potential across any individual capacitor is 200 V; so there must be at least (1000 V)/(200 V) = 5 series capacitors in any parallel branch. This branch would have an equivalent capacitance of C eq = C/5 = (2.0106 F)/5 = 0.40106 F. (b) For parallel branches we add, which means we need (1.2106 F)/(0.40106 F) = 3 parallel branches of the combination found in part (a). E3017 Look back at the solution to Ex. 3010. If C3 breaks down electrically then the circuit is effectively two capacitors in parallel. (b) V = 115 V after the breakdown. (a) q1 = (10.3106 F)(115 V) = 1.18103 C. E3018 The 108F capacitor originally has a charge of q = (108106 F)(52.4 V) = 5.66103 C. After it is connected to the second capacitor the 108F capacitor has a charge of q = (108 106 F)(35.8 V) = 3.87103 C. The difference in charge must reside on the second capacitor, so the capacitance is C = (1.79103 C)/(35.8 V) = 5.00105 F. E3019 Consider any junction other than A or B. Call this junction point 0; label the four nearest junctions to this as points 1, 2, 3, and 4. The charge on the capacitor that links point 0 to point 1 is q1 = CV01 , where V01 is the potential difference across the capacitor, so V01 = V0  V1 , where V0 is the potential at the junction 0, and V1 is the potential at the junction 1. Similar expressions exist for the other three capacitors. For the junction 0 the net charge must be zero; there is no way for charge to cross the plates of the capacitors. Then q1 + q2 + q3 + q4 = 0, and this means CV01 + CV02 + CV03 + CV04 = 0 or V01 + V02 + V03 + V04 = 0. Let V0i = V0  Vi , and then rearrange, 4V0 = V1 + V2 + V3 + V4 , or V0 = E3020 U = uV =
0E 2
1 (V1 + V2 + V3 + V4 ) . 4
V /2, where V is the volume. Then
U=
1 (8.851012 F/m)(150 V/m)2 (2.0 m3 ) = 1.99107 J. 2
70
E3021 The total capacitance is (2100)(5.0106 F) = 1.05102 F. The total energy stored is U= The cost is (1.59107 J) 1 1 C(V )2 = (1.05102 F)(55103 V)2 = 1.59107 J. 2 2 $0.03 3600103 J = $0.133.
1 E3022 (a) U = 2 C(V )2 = 1 (0.061 F)(1.0104 V)2 = 3.05106 J. 2 6 (b) (3.0510 J)/(3600103 J/kW h) = 0.847kW h.
E3023
(a) The capacitance of an air filled parallelplate capacitor is given by Eq. 305, C=
0A
d
=
(8.851012 F/m)(42.0 104 m2 ) = 2.861011 F. (1.30 103 m)
(b) The magnitude of the charge on each plate is given by q = CV = (2.861011 F)(625 V) = 1.79108 C. (c) The stored energy in a capacitor is given by Eq. 3025, regardless of the type or shape of the capacitor, so 1 1 U = C(V )2 = (2.861011 F)(625 V)2 = 5.59 J. 2 2 (d) Assuming a parallel plate arrangement with no fringing effects, the magnitude of the electric field between the plates is given by Ed = V , where d is the separation between the plates. Then E = V /d = (625 V)/(0.00130 m) = 4.81105 V/m. (e) The energy density is Eq. 3028, u= 1 1 2 12 F/m))(4.81105 V/m)2 = 1.02 J/m3 . 0 E = ((8.8510 2 2
E3024 The equivalent capacitance is given by 1/C eq = 1/(2.12106 F) + 1/(3.88106 F) = 1/(1.37106 F). The energy stored is U = 1 (1.37106 F)(328 V)2 = 7.37102 J. 2 E3025 V /r = q/4 0 r2 = E, so that if V is the potential of the sphere then E = V /r is the electric field on the surface. Then the energy density of the electric field near the surface is u= 1 (8.851012 F/m) 2 0E = 2 2 (8150 V) (0.063 m)
2
= 7.41102 J/m3 .
E3026 The charge on C3 can be found from considering the equivalent capacitance. q3 = (3.10 106 F)(112 V) = 3.47104 C. The potential across C3 is given by [V ]3 = (3.47104 C)/(3.90 106 F) = 89.0 V. The potential across the parallel segment is then (112 V)  (89.0 V) = 23.0 V. So [V ]1 = [V ]2 = 23.0 V. Then q1 = (10.3106 F)(23.0 V) = 2.37104 C and q2 = (4.80106 F)(23.0 V) = 1.10104 C.. 71
E3027 There is enough work on this problem without deriving once again the electric field between charged cylinders. I will instead refer you back to Section 264, and state E= 1 q , 2 0 Lr
where q is the magnitude of the charge on a cylinder and L is the length of the cylinders. The energy density as a function of radial distance is found from Eq. 3028, u= 1 1 2 0E = 2 8 2 q2 2 2 0 L r
The total energy stored in the electric field is given by Eq. 3024, U= 1 q2 q 2 ln(b/a) = , 2C 2 2 0 L
where we substituted into the last part Eq. 3011, the capacitance of a cylindrical capacitor. We want to show that integrating a volume integral from r = a to r = ab over the energy density function will yield U/2. Since we want to do this problem the hard way, we will pretend we don't know the answer, and integrate from r = a to r = c, and then find out what c is. Then 1 U 2 = =
a
u dV,
c 0 2 2 0 c L
1 8 2
2
q2 2 2 0 L r
L 0
r dr d dz,
= = =
q
8 2 0 L2 a 0 c q2 dr , 4 0 L a r c q2 ln . 4 0 L a
dr d dz, r
Now we equate this to the value for U that we found above, and we solve for c. 1 q 2 ln(b/a) 2 2 2 0 L ln(b/a) (b/a) ab E3028 (a) d =
0 A/C,
=
q2 c ln , 4 0 L a = 2 ln(c/a), = (c/a)2 ,
= c.
or
d = (8.851012 F/m)(0.350 m2 )/(51.31012 F) = 6.04103 m. (b) C = (5.60)(51.31012 F) = 2.871010 F. E3029 Originally, C1 = C2 /C1 = d1 /d2 , so
0 A/d1 .
After the changes, C2 = 0 A/d2 . Dividing C2 by C1 yields
= d2 C2 /d1 C1 = (2)(2.571012 F)/(1.321012 F) = 3.89. 72
E3030 The required capacitance is found from U = 1 C(V )2 , or 2 C = 2(6.61106 J)/(630 V)2 = 3.331011 F. The dielectric constant required is = (3.331011 F)/(7.401012 F) = 4.50. Try transformer oil. E3031 Capacitance with dielectric media is given by Eq. 3031, C=
e 0 A . d The various sheets have different dielectric constants and different thicknesses, and we want to maximize C, which means maximizing e /d. For mica this ratio is 54 mm1 , for glass this ratio is 35 mm1 , and for paraffin this ratio is 0.20 mm1 . Mica wins. E3032 The minimum plate separation is given by d = (4.13103 V)/(18.2106 V/m) = 2.27104 m. The minimum plate area is then A= dC (2.27104 m)(68.4109 F) = = 0.627 m2 . 0 (2.80)(8.851012 F/m)
E3033 The capacitance of a cylindrical capacitor is given by Eq. 3011, C = 2(8.851012 F/m)(2.6) 1.0103 m = 8.63108 F. ln(0.588/0.11)
E3034 (a) U = C (V )2 /2, C = e 0 A/d, and V /d is less than or equal to the dielectric strength (which we will call S). Then V = Sd and U= so the volume is given by V = 2U/e 0 S 2 . This quantity is a minimum for mica, so V = 2(250103 J)/(5.4)(8.851012 F/m)(160106 V/m)2 = 0.41 m3 . (b) e = 2U/V
0S 2
1 e 0 AdS 2 , 2
, so
e = 2(250103 J)/(0.087m3 )(8.851012 F/m)(160106 V/m)2 = 25. E3035 (a) The capacitance of a cylindrical capacitor is given by Eq. 3011, C = 2 0 e L . ln(b/a)
The factor of e is introduced because there is now a dielectric (the Pyrex drinking glass) between the plates. We can look back to Table 292 to get the dielectric properties of Pyrex. The capacitance of our "glass" is then C = 2(8.851012 F/m)(4.7) (0.15 m) = 7.31010 F. ln((3.8 cm)/(3.6 cm)
(b) The breakdown potential is (14 kV/mm)(2 mm) = 28 kV. 73
E3036 (a) C = e C = (6.5)(13.51012 F) = 8.81011 F. (b) Q = C V = (8.81011 F)(12.5 V) = 1.1109 C. (c) E = V /d, but we don't know d. (d) E = E/e , but we couldn't find E. E3037 (a) Insert the slab so that it is a distance a above the lower plate. Then the distance between the slab and the upper plate is d  a  b. Inserting the slab has the same effect as having two capacitors wired in series; the separation of the bottom capacitor is a, while that of the top capacitor is d  a  b. The bottom capacitor has a capacitance of C1 = 0 A/a, while the top capacitor has a capacitance of C2 = 0 A/(d  a  b). Adding these in series, 1 C eq = = = 1 1 + , C1 C2 a dab + , 0A 0A db . 0A
0 A/(d
So the capacitance of the system after putting the copper slab in is C = (b) The energy stored in the system before the slab is inserted is Ui = q2 d q2 = 2C i 2 0A
 b).
while the energy stored after the slab is inserted is Uf = q2 q2 d  b = 2C f 2 0A
The ratio is U i /U f = d/(d  b). (c) Since there was more energy before the slab was inserted, then the slab must have gone in willingly, it was pulled in!. To get the slab back out we will need to do work on the slab equal to the energy difference. q2 d q2 d  b q2 b Ui  Uf =  = . 2 0A 2 0A 2 0A E3038 (a) Insert the slab so that it is a distance a above the lower plate. Then the distance between the slab and the upper plate is d  a  b. Inserting the slab has the same effect as having two capacitors wired in series; the separation of the bottom capacitor is a, while that of the top capacitor is d  a  b. The bottom capacitor has a capacitance of C1 = 0 A/a, while the top capacitor has a capacitance of C2 = 0 A/(d  a  b). Adding these in series, 1 C eq = = = 1 1 + , C1 C2 a dab + , 0A 0A db . 0A
0 A/(d
So the capacitance of the system after putting the copper slab in is C = 74
 b).
(b) The energy stored in the system before the slab is inserted is Ui = C i (V )2 (V )2 0 A = 2 2 d
while the energy stored after the slab is inserted is Uf = C f (V )2 (V )2 0 A = 2 2 db
The ratio is U i /U f = (d  b)/d. (c) Since there was more energy after the slab was inserted, then the slab must not have gone in willingly, it was being repelled!. To get the slab in we will need to do work on the slab equal to the energy difference. Uf  Ui = (V )2 0 A (V )2 0 A (V )2 0 Ab  = . 2 db 2 d 2 d(d  b)
E3039 C = e 0 A/d, so d = e 0 A/C. (a) E = V /d = CV /e 0 A, or E= (1121012 F)(55.0 V) = 13400 V/m. (5.4)(8.851012 F/m)(96.5104 m2 )
(b) Q = CV = (1121012 F)(55.0 V) = 6.16109 C.. (c) Q = Q(1  1/e ) = (6.16109 C)(1  1/(5.4)) = 5.02109 C. E3040 (a) E = q/e 0 A, so e = (890109 C) = 6.53 (1.40106 V/m)(8.851012 F/m)(110104 m2 )
(b) q = q(1  1/e ) = (890109 C)(1  1/(6.53)) = 7.54107 C. P301 The capacitance of the cylindrical capacitor is from Eq. 3011, C= 2 0 L . ln(b/a)
If the cylinders are very close together we can write b = a + d, where d, the separation between the cylinders, is a small number, so C= Expanding according to the hint, C 2 0 L 2a 0 L = d/a d 2 0 L 2 0 L = . ln ((a + d)/a) ln (1 + d/a)
Now 2a is the circumference of the cylinder, and L is the length, so 2aL is the area of a cylindrical plate. Hence, for small separation between the cylinders we have C which is the expression for the parallel plates. 75
0A
d
,
P302
(a) C =
0 A/x;
take the derivative and dC dT
0 dA 0 A dx  2 , x dT x dT 1 dA 1 dx = C  A dT x dT
=
.
(b) Since (1/A)dA/dT = 2a and (1/x)dx/dT = s , we need s = 2a = 2(23106 /C ) = 46106 /C . P303 Insert the slab so that it is a distance d above the lower plate. Then the distance between the slab and the upper plate is abd. Inserting the slab has the same effect as having two capacitors wired in series; the separation of the bottom capacitor is d, while that of the top capacitor is abd. The bottom capacitor has a capacitance of C1 = 0 A/d, while the top capacitor has a capacitance of C2 = 0 A/(a  b  d). Adding these in series, 1 C eq = = = 1 1 + , C1 C2 d abd + , 0A 0A ab . 0A
0 A/(a
So the capacitance of the system after putting the slab in is C =
 b).
P304 The potential difference between any two adjacent plates is V . Each interior plate has a charge q on each surface; the exterior plate (one pink, one gray) has a charge of q on the interior surface only. The capacitance of one pink/gray plate pair is C = 0 A/d. There are n plates, but only n  1 plate pairs, so the total charge is (n  1)q. This means the total capacitance is C = 0 (n  1)A/d. P305 Let V0 = 96.6 V. As far as point e is concerned point a looks like it is originally positively charged, and point d is originally negatively charged. It is then convenient to define the charges on the capacitors in terms of the charges on the top sides, so the original charge on C1 is q 1,i = C1 V0 while the original charge on C2 is q 2,i = C2 V0 . Note the negative sign reflecting the opposite polarity of C2 . (a) Conservation of charge requires q 1,i + q 2,i = q 1,f + q 2,f , but since q = CV and the two capacitors will be at the same potential after the switches are closed we can write C1 V0  C2 V0 = C1 V + C2 V, (C1  C2 ) V0 = (C1 + C2 ) V, C1  C2 V0 = V. C1 + C2 With numbers, V = (96.6 V) (1.16 F)  (3.22 F) = 45.4 V. (1.16 F) + (3.22 F) 76
The negative sign means that the top sides of both capacitor will be negatively charged after the switches are closed. (b) The charge on C1 is C1 V = (1.16 F)(45.4 V) = 52.7C. (c) The charge on C2 is C2 V = (3.22 F)(45.4 V) = 146C. P306 C2 and C3 form an effective capacitor with equivalent capacitance Ca = C2 C3 /(C2 + C3 ). The charge on C1 is originally q0 = C1 V0 . After throwing the switch the potential across C1 is given by q1 = C1 V1 . The same potential is across Ca ; q2 = q3 , so q2 = Ca V1 . Charge is conserved, so q1 + q2 = q0 . Combining some of the above, V1 = and then q1 = Similarly, q2 = Ca C1 V0 = C1 + Ca 1 1 1 + + C1 C2 C3
1
C1 q0 = V0 , C1 + Ca C1 + Ca
2 2 C1 C1 (C2 + C3 ) V0 = V0 . C1 + Ca C1 C2 + C1 C3 + C2 C3
V0 .
q3 = q2 because they are in series. P307 (a) If terminal a is more positive than terminal b then current can flow that will charge the capacitor on the left, the current can flow through the diode on the top, and the current can charge the capacitor on the right. Current will not flow through the diode on the left. The capacitors are effectively in series. Since the capacitors are identical and series capacitors have the same charge, we expect the capacitors to have the same potential difference across them. But the total potential difference across both capacitors is equal to 100 V, so the potential difference across either capacitor is 50 V. The output pins are connected to the capacitor on the right, so the potential difference across the output is 50 V. (b) If terminal b is more positive than terminal a the current can flow through the diode on the left. If we assume the diode is resistanceless in this configuration then the potential difference across it will be zero. The net result is that the potential difference across the output pins is 0 V. In real life the potential difference across the diode would not be zero, even if forward biased. It will be somewhere around 0.5 Volts. P308 Divide the strip of width a into N segments, each of width x = a/N . The capacitance of each strip is C = 0 ax/y. If is small then 1 1 d 1 = 1  x/d). y d + x sin d + x ( Since parallel capacitances add, C= C =
0a a
d
(1  x/d)dx =
0
2 0a
d
1
a 2d
.
77
P309 (a) When S2 is open the circuit acts as two parallel capacitors. The branch on the left has an effective capacitance given by 1 1 1 1 = + = , Cl (1.0106 F) (3.0106 F) 7.5107 F while the branch on the right has an effective capacitance given by 1 1 1 1 = + = . Cl (2.0106 F) (4.0106 F) 1.33106 F The charge on either capacitor in the branch on the left is q = (7.5107 F)(12 V) = 9.0106 C, while the charge on either capacitor in the branch on the right is q = (1.33106 F)(12 V) = 1.6105 C. (b) After closing S2 the circuit is effectively two capacitors in series. The top part has an effective capacitance of C t = (1.0106 F) + (2.0106 F) = (3.0106 F), while the effective capacitance of the bottom part is C b = (3.0106 F) + (4.0106 F) = (7.0106 F). The effective capacitance of the series combination is given by 1 1 1 1 = + = . 6 F) 6 F) C eq (3.010 (7.010 2.1106 F The charge on each part is q = (2.1106 F)(12 V) = 2.52105 C. The potential difference across the top part is V t = (2.52105 C)/(3.0106 F) = 8.4 V, and then the charge on the top two capacitors is q1 = (1.0 106 F)(8.4 V) = 8.4 106 C and q2 = (2.0106 F)(8.4 V) = 1.68105 C. The potential difference across the bottom part is V t = (2.52105 C)/(7.0106 F) = 3.6 V, and then the charge on the top two capacitors is q1 = (3.0 106 F)(3.6 V) = 1.08 105 C and q2 = (4.0106 F)(3.6 V) = 1.44105 C. P3010 Let V = Vxy . By symmetry V2 = 0 and V1 = V4 = V5 = V3 = V /2. Suddenly the problem is very easy. The charges on each capacitor is q1 , except for q2 = 0. Then the equivalent capacitance of the circuit is C eq = q1 + q4 q = = C1 = 4.0106 F. V 2V1
78
P3011
(a) The charge on the capacitor with stored energy U0 = 4.0 J is q0 , where U0 =
2 q0 . 2C
When this capacitor is connected to an identical uncharged capacitor the charge is shared equally, so that the charge on either capacitor is now q = q0 /2. The stored energy in one capacitor is then U= q2 q 2 /4 1 = 0 = U0 . 2C 2C 4
But there are two capacitors, so the total energy stored is 2U = U0 /2 = 2.0 J. (b) Good question. Current had to flow through the connecting wires to get the charge from one capacitor to the other. Originally the second capacitor was uncharged, so the potential difference across that capacitor would have been zero, which means the potential difference across the connecting wires would have been equal to that of the first capacitor, and there would then have been energy dissipation in the wires according to P = i2 R. That's where the missing energy went. P3012 R = L/A and C =
0 A/L.
Combining, R = 0 /C, or
R = (9.40 m)(8.851012 F/m)/(1101012 F) = 0.756 .
1 P3013 (a) u = 2 0 E 2 = e2 /32 2 0 r4 . (b) U = u dV where dV = 4r2 dr. Then
U = 4pi
R
e2 e2 1 r2 dr = . 2 r4 32 0 8 0 R
(c) R = e2 /8 0 mc2 , or R= P3014 P3015 (1.601019 C)2 8(8.851012 F/m)(9.111031 kg)(3.00108 m/s)2 = 1.401015 m.
1 U = 2 q 2 /C = q 2 x/2A 0 . F = dU/dx = q 2 /2A 0 .
According to Problem 14, the force on a plate of a parallel plate capacitor is F = q2 . 2 0A
The force per unit area is then q2 2 F = = , A 2 0 A2 2 0 where = q/A is the surface charge density. But we know that the electric field near the surface of a conductor is given by E = / 0 , so F 1 = 0E2. A 2
79
P3016 A small surface area element dA carries a charge dq = q dA/4R2 . There are three forces on the elements which balance, so p(V0 /V )dA + q dq/4 0 R2 = p dA, or
3 pR0 + q 2 /16 2 0 R = pR3 .
This can be rearranged as
3 q 2 = 16 2 0 pR(R3  R0 ).
P3017 The magnitude of the electric field in the cylindrical region is given by E = /2 0 r, where is the linear charge density on the anode. The potential difference is given by V = (/2 0 ) ln(b/a), where a is the radius of the anode b the radius of the cathode. Combining, E = V /r ln(b/a), this will be a maximum when r = a, so V = (0.180103 m) ln[(11.0103 m)/(0.180103 m)](2.20106 V/m) = 1630 V. P3018 This is effectively two capacitors in parallel, each with an area of A/2. Then C eq = e1
0 A/2
d
+ e2
0 A/2
d
=
0A
d
e1 + e2 2
.
P3019 We will treat the system as two capacitors in series by pretending there is an infinitesimally thin conductor between them. The slabs are (I assume) the same thickness. The capacitance of one of the slabs is then given by Eq. 3031, C1 = e1 0 A , d/2
where d/2 is the thickness of the slab. There would be a similar expression for the other slab. The equivalent series capacitance would be given by Eq. 3021, 1 C eq = = = C eq = 1 1 + , C1 C2 d/2 d/2 + , e1 0 A e2 0 A d e2 + e1 , 2 0 A e1 e2 2 0 A e1 e2 . d e2 + e1
P3020 Treat this as three capacitors. Find the equivalent capacitance of the series combination on the right, and then add on the parallel part on the left. The right hand side is 1 d d 2d = + = C eq e2 0 A/2 e3 0 A/2 0A Add this to the left hand side, and C eq = = e1 0 A/2 e2 e3 0A + 2d 2d e2 + e3 A e1 e2 e3 0 + . 2d 2 e2 + e3 80 , e2 + e3 e2 e3 .
P3021 (a) q doesn't change, but C = C/2. Then V = q/C = 2V . (b) U = C(V )2 /2 = 0 A(V )2 /2d. U = C (V )2 /2 = 0 A(2V )2 /4d = 2U . (c) W = U  U = 2U  U = U = 0 A(V )2 /2d. P3022 The total energy is U = qV /2 = (7.021010 C)(52.3 V)/2 = 1.84108 J. (a) In the air gap we have Ua =
2 0 E0 V
2
=
(8.851012 F/m)(6.9103 V/m)2 (1.15102 m2 )(4.6103 m) = 1.11108 J. 2
That is (1.11/1.85) = 60% of the total. (b) The remaining 40% is in the slab. P3023 (a) C = 0 A/d = (8.851012 F/m)(0.118 m2 )/(1.22102 m) = 8.561011 F. (b) Use the results of Problem 3024. C = (4.8)(8.851012 F/m)(0.118 m2 ) = 1.191010 F (4.8)(1.22102 m)  (4.3103 m)(4.8  1)
(c) q = CV = (8.561011 F)(120 V) = 1.03108 C; since the battery is disconnected q = q. (d) E = q/ 0 A = (1.03108 C)/(8.851012 F/m)(0.118 m2 ) = 9860 V/m in the space between the plates. (e) E = E/e = (9860 V/m)/(4.8) = 2050 V/m in the dielectric. (f) V = q/C = (1.03108 C)/(1.191010 F) = 86.6 V. (g) W = U  U = q 2 (1/C  1/C )/2, or W = (1.03108 C)2 [1/(8.561011 F)  1/(1.191010 F)] = 1.73107 J. 2
P3024 The result is effectively three capacitors in series. Two are air filled with thicknesses of x and d  b  x, the third is dielectric filled with thickness b. All have an area A. The effective capacitance is given by 1 C = = C = = x dbx b + + , e 0 A 0A 0A 1 b (d  b) + , A e 0 0A , d  b + b/e e 0 A . e  b(e  1)
81
E311 (5.12 A)(6.00 V)(5.75 min)(60 s/min) = 1.06104 J. E312 (a) (12.0 V)(1.601019 C) = 1.921018 J. (b) (1.921018 J)(3.401018 /s) = 6.53 W. E313 If the energy is delivered at a rate of 110 W, then the current through the battery is i= P (110 W) = = 9.17 A. V (12 V)
Current is the flow of charge in some period of time, so t = q (125 A h) = = 13.6 h, i (9.2 A)
which is the same as 13 hours and 36 minutes. E314 (100 W)(8 h) = 800 W h. (a) (800 W h)/(2.0 W h) = 400 batteries, at a cost of (400)($0.80) = $320. (b) (800 W h)($0.12103 W h) = $0.096. E315 Go all of the way around the circuit. It is a simple one loop circuit, and although it does not matter which way we go around, we will follow the direction of the larger emf. Then (150 V)  i(2.0 )  (50 V)  i(3.0 ) = 0, where i is positive if it is counterclockwise. Rearranging, 100 V = i(5.0 ), or i = 20 A. Assuming the potential at P is VP = 100 V, then the potential at Q will be given by VQ = VP  (50 V)  i(3.0 ) = (100 V)  (50 V)  (20 A)(3.0 ) = 10 V. E316 (a) Req = (10 ) + (140 ) = 150 . i = (12.0 V)/(150 ) = 0.080 A. (b) Req = (10 ) + (80 ) = 90 . i = (12.0 V)/(90 ) = 0.133 A. (c) Req = (10 ) + (20 ) = 30 . i = (12.0 V)/(30 ) = 0.400 A. E317 (a) Req = (3.0 V  2.0 V)/(0.050 A) = 20 . Then R = (20 )  (3.0 )  (3.0 ) = 14 . (b) P = iV = i2 R = (0.050 A)2 (14 ) = 3.5102 W. E318 (5.0 A)R1 = V . (4.0 A)(R1 +2.0 ) = V . Combining, 5R1 = 4R1 +8.0 , or R1 = 8.0 . E319 (a) (53.0 W)/(1.20 A) = 44.2 V. (b) (1.20 A)(19.0 ) = 22.8 V is the potential difference across R. Then an additional potential difference of (44.2 V)  (22.8 V) = 21.4 V must exist across C. (c) The left side is positive; it is a reverse emf. E3110 (a) The current in the resistor is (9.88 W)/(0.108 ) = 9.56 A. The total resistance of the circuit is (1.50 V)/(9.56 A) = 0.157 . The internal resistance of the battery is then (0.157 )  (0.108 ) = 0.049 . (b) (9.88 W)/(9.56 A) = 1.03 V. 82
E3111
We assign directions to the currents through the four resistors as shown in the figure.
1 a 3
2 b 4
Since the ammeter has no resistance the potential at a is the same as the potential at b. Consequently the potential difference (V b ) across both of the bottom resistors is the same, and the potential difference (V t ) across the two top resistors is also the same (but different from the bottom). We then have the following relationships: V t + V b i1 + i2 Vj = E, = i3 + i4 , = i j Rj ,
where the j subscript in the last line refers to resistor 1, 2, 3, or 4. For the top resistors, V1 = V2 implies 2i1 = i2 ; while for the bottom resistors, V3 = V4 implies i3 = i4 . Then the junction rule requires i4 = 3i1 /2, and the loop rule requires (i1 )(2R) + (3i1 /2)(R) = E or i1 = 2E/(7R). The current that flows through the ammeter is the difference between i2 and i4 , or 4E/(7R)  3E/(7R) = E/(7R). E3112 (a) Define the current i1 as moving to the left through r1 and the current i2 as moving to the left through r2 . i3 = i1 + i2 is moving to the right through R. Then there are two loop equations: E1 E2 = i1 r1 + i3 R, = (i3  i1 )r2 + i3 R.
Multiply the top equation by r2 and the bottom by r1 and then add: r2 E1 + r1 E2 = i3 r1 r2 + i3 R(r1 + r2 ), which can be rearranged as i3 = (b) There is only one current, so E1 + E2 = i(r1 + r2 + R), or i= E1 + E2 . r1 + r 2 + R 83 r2 E1 + r1 E2 . r1 r2 + Rr1 + Rr2
E3113 (a) Assume that the current flows through each source of emf in the same direction as the emf. The the loop rule will give us three equations E1  i1 R1 + i2 R2  E2  i1 R1 E2  i2 R2 + i3 R1  E3 + i3 R1 E1  i1 R1 + i3 R1  E3 + i3 R1  i1 R1 = 0, = 0, = 0.
The junction rule (looks at point a) gives us i1 + i2 + i3 = 0. Use this to eliminate i2 from the second loop equation, E2 + i1 R2 + i3 R2 + 2i3 R1  E3 = 0, and then combine this with the the third equation to eliminate i3 ,
2 E1 R2  E3 R2 + 2i3 R1 R2 + 2E2 R1 + 2i3 R1 R2 + 4i3 R1  2E3 R1 = 0,
or i3 = Then we can find i1 from
2E3 R1 + E3 R2  E1 R2  2E2 R1 = 0.582 A. 2 4R1 R2 + 4R1 E3  E2  i3 R2  2i3 R1 = 0.668 A, R2
i1 =
where the negative sign indicates the current is down. Finally, we can find i2 = (i1 + i3 ) = 0.0854 A. (b) Start at a and go to b (final minus initial!), +i2 R2  E2 = 3.60 V. E3114 (a) The current through the circuit is i = E/(r + R). The power delivered to R is then P = iV = i2 R = E 2 R/(r + R)2 . Evaluate dP/dR and set it equal to zero to find the maximum. Then dP rR 0= = E 2R , dR (r + R)3 which has the solution r = R. (b) When r = R the power is P = E 2R 1 E2 = . (R + R)2 4r
E3115 (a) We first use P = F v to find the power output by the electric motor. Then P = (2.0 N)(0.50 m/s) = 1.0 W. The potential difference across the motor is V m = E  ir. The power output from the motor is the rate of energy dissipation, so P m = V m i. Combining these two expressions, Pm = (E  ir) i, = Ei  i2 r, 0 = i2 r + Ei  P m , 0 = (0.50 )i2  (2.0 V)i + (1.0 W).
Rearrange and solve for i, i= (2.0 V) (2.0 V)2  4(0.50 )(1.0 W) , 2(0.50 ) 84
which has solutions i = 3.4 A and i = 0.59 A. (b) The potential difference across the terminals of the motor is V m = E  ir which if i = 3.4 A yields V m = 0.3 V, but if i = 0.59 A yields V m = 1.7 V. The battery provides an emf of 2.0 V; it isn't possible for the potential difference across the motor to be larger than this, but both solutions seem to satisfy this constraint, so we will move to the next part and see what happens. (c) So what is the significance of the two possible solutions? It is a consequence of the fact that power is related to the current squared, and with any quadratics we expect two solutions. Both are possible, but it might be that only one is stable, or even that neither is stable, and a small perturbation to the friction involved in turning the motor will cause the system to break down. We will learn in a later chapter that the effective resistance of an electric motor depends on the speed at which it is spinning, and although that won't affect the problem here as worded, it will affect the physical problem that provided the numbers in this problem! E3116 req = 4r = 4(18 ) = 72 . The current is i = (27 V)/(72 ) = 0.375 A. E3117 In parallel connections of two resistors the effective resistance is less than the smaller resistance but larger than half the smaller resistance. In series connections of two resistors the effective resistance is greater than the larger resistance but less than twice the larger resistance. Since the effective resistance of the parallel combination is less than either single resistance and the effective resistance of the series combinations is larger than either single resistance we can conclude that 3.0 must have been the parallel combination and 16 must have been the series combination. The resistors are then 4.0 and 12 resistors. E3118 Points B and C are effectively the same point! (a) The three resistors are in parallel. Then req = R/3. (b) See (a). (c) 0, since there is no resistance between B and C. E3119 Focus on the loop through the battery, the 3.0 , and the 5.0 resistors. The loop rule yields (12.0 V) = i[(3.0 ) + (5.0 )] = i(8.0 ). The potential difference across the 5.0 resistor is then V = i(5.0 ) = (5.0 )(12.0 V)/(8.0 ) = 7.5 V. E3120 Each lamp draws a current of (500 W)/(120 V) = 4.17 A. Furthermore, the fuse can support (15 A)/(4.17 A) = 3.60 lamps. That is a maximum of 3. E3121 The current in the series combination is is = E/(R1 + R2 ). The power dissipated is P s = iE = E 2 /(R1 + R2 ). In a parallel arrangement R1 dissipates P1 = i1 E = E 2 /R1 . A similar expression exists for R2 , so the total power dissipated is P p = E 2 (1/R1 + 1/R2 ). The ratio is 5, so 5 = P p /P s = (1/R1 + 1/R2 )(R1 + R2 ), or 5R1 R2 = (R1 + R2 )2 . Solving for R2 yields 2.618R1 or 0.382R1 . Then R2 = 262 or R2 = 38.2 .
85
E3122 Combining n identical resistors in series results in an equivalent resistance of req = nR. Combining n identical resistors in parallel results in an equivalent resistance of req = R/n. If the resistors are arranged in a square array consisting of n parallel branches of n series resistors, then the effective resistance is R. Each will dissipate a power P , together they will dissipate n2 P . So we want nine resistors, since four would be too small. E3123 parallel: (a) Work through the circuit one step at a time. We first "add" R2 , R3 , and R4 in
1 1 1 1 1 = + + = Reff 42.0 61.6 75.0 18.7 We then "add" this resistance in series with R1 , Reff = (112 ) + (18.7 ) = 131 . (b) The current through the battery is i = E/R = (6.22 V)/(131 ) = 47.5 mA. This is also the current through R1 , since all the current through the battery must also go through R1 . The potential difference across R1 is V1 = (47.5 mA)(112 ) = 5.32 V. The potential difference across each of the three remaining resistors is 6.22 V  5.32 V = 0.90 V. The current through each resistor is then i2 i3 i4 = (0.90 V)/(42.0 ) = 21.4 mA, = (0.90 V)/(61.6 ) = 14.6 mA, = (0.90 V)/(75.0 ) = 12.0 mA.
E3124 The equivalent resistance of the parallel part is r = R2 R/(R2 + R). The equivalent resistance for the circuit is r = R1 + R2 R/(R2 + R). The current through the circuit is i = E/r. The potential difference across R is V = E  i R1 , or V = E(1  R1 /r), R2 + R R1 R2 + R1 R + RR2 RR2 = E . R1 R2 + R1 R + RR2 = E 1  R1 Since P = iV = (V )2 /R, P = E2
2 RR2 . (R1 R2 + R1 R + RR2 )2
,
Set dP/dR = 0, the solution is R = R1 R2 /(R1 + R2 ). E3125 (a) First "add" the left two resistors in series; the effective resistance of that branch is 2R. Then "add" the right two resistors in series; the effective resistance of that branch is also 2R. Now we combine the three parallel branches and find the effective resistance to be 1 1 1 1 4 = + + = , Reff 2R R 2R 2R or Reff = R/2. (b) First we "add" the right two resistors in series; the effective resistance of that branch is 2R. We then combine this branch with the resistor which connects points F and H. This is a parallel connection, so the effective resistance is 1 1 1 3 = + = , Reff 2R R 2R 86
or 2R/3. This value is effectively in series with the resistor which connects G and H, so the "total" is 5R/3. Finally, we can combine this value in parallel with the resistor that directly connects F and G according to 1 1 3 8 = + = , Reff R 5R 5R or Reff = 5R/8. E3126 The resistance of the second resistor is r2 = (2.4 V)/(0.001 A) = 2400 . The potential difference across the first resistor is (12 V)  (2.4 V) = 9.6 V. The resistance of the first resistor is (9.6 V)/(0.001 A) = 9600 . E3127 See Exercise 3126. The resistance ratio is (0.95 0.1 V) r1 = , r 1 + r2 (1.50 V) or r2 (1.50 V) =  1. r1 (0.95 0.1 V)
The allowed range for the ratio r2 /r1 is between 0.5625 and 0.5957. We can choose any standard resistors we want, and we could use any tolerance, but then we will need to check our results. 22 and 39 would work; as would 27 and 47. There are other choices. E3128 Consider any junction other than A or B. Call this junction point 0; label the four nearest junctions to this as points 1, 2, 3, and 4. The current through the resistor that links point 0 to point 1 is i1 = V01 /R, where V01 is the potential difference across the resistor, so V01 = V0  V1 , where V0 is the potential at the junction 0, and V1 is the potential at the junction 1. Similar expressions exist for the other three resistor. For the junction 0 the net current must be zero; there is no way for charge to accumulate on the junction. Then i1 + i2 + i3 + i4 = 0, and this means V01 /R + V02 /R + V03 /R + V04 /R = 0 or V01 + V02 + V03 + V04 = 0. Let V0i = V0  Vi , and then rearrange, 4V0 = V1 + V2 + V3 + V4 , or V0 = 1 (V1 + V2 + V3 + V4 ) . 4
E3129 The current through the radio is i = P/V = (7.5 W)/(9.0 V) = 0.83 A. The radio was left one for 6 hours, or 2.16104 s. The total charge to flow through the radio in that time is (0.83 A)(2.16104 s) = 1.8104 C. E3130 The power dissipated by the headlights is (9.7 A)(12.0 V) = 116 W. The power required by the engine is (116 W)/(0.82) = 142 W, which is equivalent to 0.190 hp. 87
E3131 (a) P = (120 V)(120 V)/(14.0 ) = 1030 W. (b) W = (1030 W)(6.42 h) = 6.61 kW h. The cost is $0.345. E3132 E3133 We want to apply either Eq. 3121, PR = i2 R, or Eq. 3122, PR = (VR )2 /R, depending on whether we are in series (the current is the same through each bulb), or in parallel (the potential difference across each bulb is the same. The brightness of a bulb will be measured by P , even though P is not necessarily a measure of the rate radiant energy is emitted from the bulb. (b) If the bulbs are in parallel then PR = (VR )2 /R is how we want to compare the brightness. The potential difference across each bulb is the same, so the bulb with the smaller resistance is brighter. (b) If the bulbs are in series then PR = i2 R is how we want to compare the brightness. Both bulbs have the same current, so the larger value of R results in the brighter bulb. One direct consequence of this can be tried at home. Wire up a 60 W, 120 V bulb and a 100 W, 120 V bulb in series. Which is brighter? You should observe that the 60 W bulb will be brighter. E3134 (a) j = i/A = (25 A)/(0.05 in) = 3180 A/in = 4.93106 A/m2 . (b) E = j = (1.69108 m)(4.93106 A/m2 ) = 8.33102 V/m. (c) V = Ed = (8.33102 V/m)(305 m) = 25 V. (d) P = iV = (25 A)(25 V) = 625 W. E3135 (a) The bulb is on for 744 hours. The energy consumed is (100 W)(744 h) = 74.4 kW h, at a cost of (74.4)(0.06) = $4.46. (b) r = V 2 /P = (120 V)2 /(100 W) = 144 . (c) i = P/V = (100 W)/(120 V) = 0.83 A. E3136 P = (V )2 /r and r = r0 (1 + T ). Then P = (500 W) P0 = = 660 W 1 + T 1 + (4.0104 /C )(600C )
2
E3137 (a) n = q/e = it/e, so n = (485103 A)(95109 s)/(1.61019 C) = 2.881011 . (b) iav = (520/s)(485103 A)(95109 s) = 2.4105 A. (c) P p = ip V = (485103 A)(47.7106 V) = 2.3106 W; while P a = ia V = (2.4105 A)(47.7 6 10 V) = 1.14103 W. E3138 r = L/A = (3.5105 m)(1.96102 m)/(5.12103 m)2 = 8.33103 . (a) i = P/r = (1.55 W)/(8.33103 ) = 13.6 A, so j = i/A = (13.6 A)/(5.12103 m)2 = 1.66105 A/m2 . (b) V = Pr = (1.55 W)(8.33103 ) = 0.114 V. 88
E3139
(a) The current through the wire is i = P/V = (4800 W)/(75 V) = 64 A,
The resistance of the wire is R = V /i = (75 V)/(64 A) = 1.17 . The length of the wire is then found from L= RA (1.17 )(2.6106 m2 ) = = 6.1 m. (5.0107 m)
One could easily wind this much nichrome to make a toaster oven. Of course allowing 64 Amps to be drawn through household wiring will likely blow a fuse. (b) We want to combine the above calculations into one formula, so L= then L= RA AV /i A(V )2 = = , P
(2.6106 m2 )(110 V)2 = 13 m. (4800 W)(5.0107 m)
Hmm. We need more wire if the potential difference is increased? Does this make sense? Yes, it does. We need more wire because we need more resistance to decrease the current so that the same power output occurs. E3140 (a) The energy required to bring the water to boiling is Q = mCT . The time required is Q (2.1 kg)(4200 J/kg)(100 C  18.5 C) t= = = 2.22103 s 0.77P 0.77(420 W) (b) The additional time required to boil half of the water away is t= mL/2 (2.1 kg)(2.26106 J/kg)/2 = = 7340 s. 0.77P 0.77(420 W)
E3141
(a) Integrate both sides of Eq. 3126;
q 0
dq q  EC
q
t
= 
0
dt , RC
t
ln(q  EC)0 ln q  EC EC q  EC EC q That wasn't so bad, was it?
t , RC 0 t =  , RC =  = et/RC , = EC 1  et/RC .
89
(b) Rearrange Eq. 3126 in order to get q terms on the left and t terms on the right, then integrate;
q q0
dq q
q
t
= 
0
dt , RC
t
ln qq0 ln q q0 q q0 q That wasn't so bad either, was it?
t , RC 0 t =  , RC =  = et/RC , = q0 et/RC .
E3142 (a) C = RC = (1.42106 )(1.80106 F) = 2.56 s. (b) q0 = CV = (1.80106 F)(11.0 V) = 1.98105 C. (c) t = C ln(1  q/q0 ), so t = (2.56 s) ln(1  15.5106 C/1.98105 C) = 3.91 s. E3143 Solve n = t/C =  ln(1  0.99) = 4.61. E3144 (a) V = E(1  et/C ), so C = (1.28106 s)/ ln(1  5.00 V/13.0 V) = 2.64106 s (b) C = C /R = (2.64106 s)/(15.2103 ) = 1.731010 F E3145 (a) V = Eet/C , so C = (10.0 s)/ ln(1.06 V/100 V) = 2.20 s (b) V = (100 V)e17 s/2.20 s = 4.4102 V. E3146 V = Eet/C and C = RC, so t t t R= = = . C ln(V /V0 ) (220109 F) ln(0.8 V/5 V) 4.03107 F If t is between 10.0 s and 6.0 ms, then R is between R = (10106 s)/(4.03107 F) = 24.8, and R = (6103 s)/(4.03107 F) = 14.9103 . E3147 The charge on the capacitor needs to build up to a point where the potential across the capacitor is VL = 72 V, and this needs to happen within 0.5 seconds. This means that we want to solve CVL = CE 1  eT /RC for R knowing that T = 0.5 s. This expression can be written as R= T (0.5 s) = = 2.35106 . C ln(1  VL /E) (0.15 C) ln(1  (72 V)/(95 V)) 90
E3148 (a) q0 = 2U C = 2(0.50 J)(1.0106 F) = 1103 C. (b) i0 = V0 /R = q0 /RC = (1103 C)/(1.0106 )(1.0106 F) = 1103 A. (c) VC = V0 et/C , so VC = (1103 C) t/(1.0106 )(1.0106 F) e = (1000 V)et/(1.0 s) (1.0106 F)
Note that VR = VC . (d) PR = (VR )2 /R, so PR = (1000 V)2 e2t/(1.0 s) /(1106 ) = (1 W)e2t/(1.0 s) . E3149 (a) i = dq/dt = Eet/C /R, so i=
6 6 (4.0 V) e(1.0 s)/(3.010 )(1.010 F) = 9.55107 A. (3.0106 )
(b) PC = iV = (E 2 /R)et/C (1  et/C ), so PC =
6 6 (4.0 V)2 (1.0 s)/(3.0106 )(1.0106 F) e 1  e(1.0 s)/(3.010 )(1.010 F) = 1.08106 W. (3.0106 )
(c) PR = i2 R = (E 2 /R)e2t/C , so PR = (d) P = PR + PC , or P = 2.74106 W + 1.08106 W = 3.82106 W E3150 The rate of energy dissipation in the resistor is PR = i2 R = (E 2 /R)e2t/C . Evaluating E 2 2t/RC E2 e dt = C, R 0 2 0 but that is the original energy stored in the capacitor. PR dt = P311 The terminal voltage of the battery is given by V = E  ir, so the internal resistance is r= E V (12.0 V)  (11.4 V) = = 0.012 , i (50 A)
(4.0 V)2 2(1.0 s)/(3.0106 )(1.0106 F) e = 2.74106 W. (3.0106 )
so the battery appears within specs. The resistance of the wire is given by R= so the cable appears to be bad. What about the motor? Trying it, R= so it appears to be within spec. 91 V (11.4 V)  (3.0 V) = = 0.168 , i (50 A) V (3.0 V) = = 0.06 , i (50 A)
P312
Traversing the circuit we have E  ir1 + E  ir2  iR = 0,
so i = 2E/(r1 + r2 + R). The potential difference across the first battery is then V1 = E  ir1 = E 1  2r1 r 1 + r2 + R =E r2  r 1 + R r1 + r 2 + R
This quantity will only vanish if r2  r1 + R = 0, or r1 = R + r2 . Since r1 > r2 this is actually possible; R = r1  r2 . P313 V = E  iri and i = E/(ri + R), so V = E There are then two simultaneous equations: (0.10 V)(500 ) + (0.10 V)ri = E(500 ) and (0.16 V)(1000 ) + (0.16 V)ri = E(1000 ), with solution (a) ri = 1.5103 and (b) E = 0.400 V. 2 (c) The cell receives energy from the sun at a rate (2.0 mW/cm )(5.0 cm2 ) = 0.010 W. The cell 2 2 converts energy at a rate of V /R = (0.16 V) /(1000 ) = 0.26 % P314 (a) The emf of the battery can be found from E = iri + V l = (10 A)(0.05 ) + (12 V) = 12.5 V (b) Assume that resistance is not a function of temperature. The resistance of the headlights is then rl = (12.0 V)/(10.0 A) = 1.2 . The potential difference across the lights when the starter motor is on is V l = (8.0 A)(1.2 ) = 9.6 V, and this is also the potential difference across the terminals of the battery. The current through the battery is then E  V (12.5 V)  (9.6 V) i= = = 58 A, ri (0.05 ) so the current through the motor is 50 Amps. P315 (a) The resistivities are A = rA A/L = (76.2106 )(91.0104 m2 )/(42.6 m) = 1.63108 m, and B = rB A/L = (35.0106 )(91.0104 m2 )/(42.6 m) = 7.48109 m. (b) The current is i = V /(rA + rB ) = (630 V)/(111.2 ) = 5.67106 A. The current density is then j = (5.67106 A)/(91.0104 m2 ) = 6.23108 A/m2 . (c) EA = A j = (1.63108 m)(6.23108 A/m2 ) = 10.2 V/m and EB = B j = (7.48109 m)(6.23108 A/m2 ) = 4.66 V/m. (d) VA = EA L = (10.2 V/m)(42.6 m) = 435 V and VB = EB L = (4.66 V/m)(42.6 m) = 198 V. 92 R , ri + R
P316 Set up the problem with the traditional presentation of the Wheatstone bridge problem. Then the symmetry of the problem (flip it over on the line between x and y) implies that there is no current through r. As such, the problem is equivalent to two identical parallel branches each with two identical series resistances. Each branch has resistance R + R = 2R, so the overall circuit has resistance 1 1 1 1 = + = , Req 2R 2R R so Req = R. P317 P318 (a) The loop through R1 is trivial: i1 = E2 /R1 = (5.0 V)/(100 ) = 0.05 A. The loop through R2 is only slightly harder: i2 = (E2 + E3  E1 )/R2 = 0.06 A. (b) Vab = E3 + E2 = (5.0 V) + (4.0 V) = 9.0 V. P319 (a) The three way lightbulb has two filaments (or so we are told in the question). There are four ways for these two filaments to be wired: either one alone, both in series, or both in parallel. Wiring the filaments in series will have the largest total resistance, and since P = V 2 /R this arrangement would result in the dimmest light. But we are told the light still operates at the lowest setting, and if a filament burned out in a series arrangement the light would go out. We then conclude that the lowest setting is one filament, the middle setting is another filament, and the brightest setting is both filaments in parallel. (b) The beauty of parallel settings is that then power is additive (it is also addictive, but that's a different field.) One filament dissipates 100 W at 120 V; the other filament (the one that burns out) dissipates 200 W at 120 V, and both together dissipate 300 W at 120 V. The resistance of one filament is then R= The resistance of the other filament is R= (V )2 (120 V)2 = = 72 . P (200 W) (120 V)2 (V )2 = = 144 . P (100 W)
P3110 We can assume that R "contains" all of the resistance of the resistor, the battery and the ammeter, then R = (1.50 V)/(1.0 m/A) = 1500 . For each of the following parts we apply R + r = V /i, so (a) r = (1.5 V)/(0.1 mA)  (1500 ) = 1.35104 , (b) r = (1.5 V)/(0.5 mA)  (1500 ) = 1.5103 , (c) r = (1.5 V)/(0.9 mA)  (1500 ) = 167. (d) R = (1500 )  (18.5 ) = 1482 P3111 (a) The effective resistance of the parallel branches on the middle and the right is R2 R 3 . R2 + R3
93
The effective resistance of the circuit as seen by the battery is then R1 + The current through the battery is i=E R 2 + R3 , R1 R 2 + R1 R3 + R2 R3 R2 R3 R1 R 2 + R1 R3 + R2 R3 = , R2 + R3 R 2 + R3
The potential difference across R1 is then V1 = E while V3 = E  V1 , or V3 = E so the current through the ammeter is i3 = or i3 = (5.0 V) V3 R2 =E , R3 R1 R2 + R 1 R3 + R 2 R 3 R2 + R 3 R1 , R 1 R2 + R 1 R 3 + R 2 R 3 R 2 R3 , R1 R2 + R 1 R3 + R 2 R 3
(4 ) = 0.45 A. (2 )(4 ) + (2 )(6 ) + (4 )(6 )
(b) Changing the locations of the battery and the ammeter is equivalent to swapping R1 and R3 . But since the expression for the current doesn't change, then the current is the same. P3112 V1 + V2 = VS + VX ; if Va = Vb , then V1 = VS . Using the first expression, ia (R1 + R2 ) = ib (RS + RX ), using the second, i a R1 = i b R2 . Dividing the first by the second, 1 + R2 /R1 = 1 + RX /RS , or RX = RS (R2 /R1 ). P3113 P3114 Lv = Q/m and Q/t = P = iV , so Lv = iV (5.2 A)(12 V) = = 2.97106 J/kg. m/t (21106 kg/s)
P3115 P = i2 R. W = pV , where V is volume. p = mg/A and V = Ay, where y is the height of the piston. Then P = dW/dt = mgv. Combining all of this, v= i2 R (0.240 A)2 (550 ) = = 0.274 m/s. mg (11.8 kg)(9.8 m/s2 ) 94
P3116
(a) Since q = CV , then q = (32106 F) (6 V) + (4 V/s)(0.5 s)  (2 V/s2 )(0.5 s)2 = 2.4104 C.
(b) Since i = dq/dt = C dV /dt, then i = (32106 F) (4 V/s)  2(2 V/s2 )(0.5 s) = 6.4105 A. (c) Since P = iV , P = [ (4 V/s)  2(2 V/s2 )(0.5 s) (6 V) + (4 V/s)(0.5 s)  (2 V/s2 )(0.5 s)2 = 4.8104 W. P3117 (a) We have P = 30P0 and i = 4i0 . Then R= P 30P0 30 = = R0 . i2 (4i0 )2 16
We don't really care what happened with the potential difference, since knowing the change in resistance of the wire should give all the information we need. The volume of the wire is a constant, even upon drawing the wire out, so LA = L0 A0 ; the product of the length and the cross sectional area must be a constant. Resistance is given by R = L/A, but A = L0 A0 /L, so the length of the wire is L= A0 L0 R = 30 A0 L0 R0 = 1.37L0 . 16
(b) We know that A = L0 A0 /L, so A= P3118 A0 L A0 = = 0.73A0 . L0 1.37
(a) The capacitor charge as a function of time is given by Eq. 3127, q = CE 1  et/RC ,
while the current through the circuit (and the resistor) is given by Eq. 3128, i= The energy supplied by the emf is U= Ei dt = E dq = Eq; E t/RC e . R
but the energy in the capacitor is UC = qV /2 = Eq/2. (b) Integrating, E2 E2 Eq UR = i2 Rdt = e2t/RC dt = = . R 2C 2
95
P3119
The capacitor charge as a function of time is given by Eq. 3127, q = CE 1  et/RC ,
while the current through the circuit (and the resistor) is given by Eq. 3128, i= E t/RC e . R
The energy stored in the capacitor is given by U= q2 , 2C
so the rate that energy is being stored in the capacitor is PC = dU q dq q = = i. dt C dt C
The rate of energy dissipation in the resistor is PR = i2 R, so the time at which the rate of energy dissipation in the resistor is equal to the rate of energy storage in the capacitor can be found by solving PC i R iRC ECet/RC et/RC t
2
= PR , q = i, C = q, = CE 1  et/RC , = 1/2, = RC ln 2.
96
E321 Apply Eq. 323, F = qv B. All of the paths which involve left hand turns are positive particles (path 1); those paths which involve right hand turns are negative particle (path 2 and path 4); and those paths which don't turn involve neutral particles (path 3). E322 (a) The greatest magnitude of force is F = qvB = (1.61019 C)(7.2106 m/s)(83103 T) = 9.61014 N. The least magnitude of force is 0. (b) The force on the electron is F = ma; the angle between the velocity and the magnetic field is , given by ma = qvB sin . Then = arcsin (9.11031 kg)(4.91016 m/s2 ) (1.61019 C)(7.2106 m/s)(83103 T) = 28 .
E323 (a) v = E/B = (1.5103 V/m)/(0.44 T) = 3.4103 m/s. E324 (a) v = F/qB sin = (6.481017 N/(1.601019 C)(2.63103 T) sin(23.0 ) = 3.94105 m/s. (b) K = mv 2 /2 = (938 MeV/c2 )(3.94105 m/s)2 /2 = 809 eV. E325 The magnetic force on the proton is FB = qvB = (1.61019 C)(2.8107 m/s)(30eex6 T) = 1.31016 N. The gravitational force on the proton is mg = (1.71027 kg)(9.8 m/s2 ) = 1.71026 N. The ratio is then 7.6109 . If, however, you carry the number of significant digits for the intermediate answers farther you will get the answer which is in the back of the book. E326 The speed of the electron is given by v = v= 2qV /m, or
2(1000 eV)/(5.1105 eV/c2 ) = 0.063c.
The electric field between the plates is E = (100 V)/(0.020 m) = 5000 V/m. The required magnetic field is then B = E/v = (5000 V/m)/(0.063c) = 2.6104 T. E327 Both have the same velocity. Then K p /K e = mp v 2 /me v 2 = mp /me =. E328 The speed of the ion is given by v = v= 2qV /m, or
2(10.8 keV)/(6.01)(932 MeV/c2 ) = 1.96103 c.
The required electric field is E = vB = (1.96103 c)(1.22 T) = 7.17105 V/m. E329 (a) For a charged particle moving in a circle in a magnetic field we apply Eq. 3210; r= mv (9.111031 kg)(0.1)(3.00108 m/s) = = 3.4104 m. qB (1.61019 C)(0.50 T)
(b) The (nonrelativistic) kinetic energy of the electron is K= 1 1 mv 2 = (0.511 MeV)(0.10c)2 = 2.6103 MeV. 2 2 97
E3210 (a) v = 2K/m = 2(1.22 keV)/(511 keV/c2 ) = 0.0691c. (b) B = mv/qr = (9.111031 kg)(0.0691c)/(1.601019 C)(0.247 m) = 4.78104 T. (c) f = qB/2m = (1.601019 C)(4.78104 T)/2(9.111031 kg) = 1.33107 Hz. (d) T = 1/f = 1/(1.33107 Hz) = 7.48108 s. E3211 (a) v = 2K/m = 2(350 eV)/(511 keV/c2 ) = 0.037c. (b) r = mv/qB = (9.111031 kg)(0.037c)/(1.601019 C)(0.20T) = 3.16104 m. E3212 The frequency is f = (7.00)/(1.29103 s) = 5.43103 Hz. The mass is given by m = qB/2f , or (1.601019 C)(45.0103 T) m= = 2.111025 kg = 127 u. 2(5.43103 Hz) E3213 (a) Apply Eq. 3210, but rearrange it as v= qrB 2(1.61019 C)(0.045 m)(1.2 T) = = 2.6106 m/s. m 4.0(1.661027 kg)
(b) The speed is equal to the circumference divided by the period, so T = 2r 2m 24.0(1.661027 kg) = = = 1.1107 s. v qB 2(1.6 1019 C)(1.2 T)
(c) The (nonrelativistic) kinetic energy is K= q2 r2 B (21.61019 C)2 (0.045 m)2 (1.2 T)2 = = 2.241014 J. 2m 2(4.01.661027 kg))
To change to electron volts we need merely divide this answer by the charge on one electron, so K= (d) V =
K q
(2.241014 J) = 140 keV. (1.61019 C)
= (140 keV)/(2e) = 70 V.
E3214 (a) R = mv/qB = (938 MeV/c2 )(0.100c)/e(1.40 T) = 0.223 m. (b) f = qB/2m = e(1.40 T)/2(938 MeV/c2 ) = 2.13107 Hz.
2 E3215 (a) K /K p = (q /m )/(q p 2 /mp ) = 22 /4 = 1. 2 (b) K d /K p = (q d /md )/(q p 2 /mp ) = 12 /2 = 1/2.
E3216 (a) K = qV . Then K p = eV , K d = eV , and K = 2eV . (b) r = sqrt2mK/qB. Then rd /rp = (2/1)(1/1)/(1/1) = 2. (c) r = sqrt2mK/qB. Then r /rp = (4/1)(2/1)/(2/1) = 2. E3217 r = 2mK/qB = ( m/q)( 2K/B). All three particles are traveling with the same kinetic energy in the same magnetic field. The relevant factors are in front; we just need to compare the mass and charge of each of the three particles. (a) The radius of the deuteron path is 12 rp . (b) The radius of the alpha particle path is 24 rp = rp . 98
E3218 The neutron, being neutral, is unaffected by the magnetic field and moves off in a line tangent to the original path. The proton moves at the same original speed as the deuteron and has the same charge, but since it has half the mass it moves in a circle with half the radius. E3219 (a) The proton momentum would be pc = qcBR = e(3.0108 m/s)(41106 T)(6.4106 m) = 7.9104 MeV. Since 79000 MeV is much, much greater than 938 MeV the proton is ultrarelativistic. Then E pc, and since = E/mc2 we have = p/mc. Inverting, v = c E3220 (a) Classically, R = R= 1 1 = 2 1 m2 c2 m2 c2 1 0.99993. 2 p 2p2
2mK/qB, or
2(0.511 MeV/c2 )(10.0 MeV)/e(2.20 T) = 4.84103 m.
(b) This would be an ultrarelativistic electron, so K E pc, then R = p/qB = K/qBc, or R = (10.0 MeV)/e(2.2 T)(3.00108 m/s) = 1.52102 m. (c) The electron is effectively traveling at the speed of light, so T = 2R/c, or T = 2(1.52102 m)/(3.00108 m/s) = 3.181010 s. This result does depend on the speed! E3221 Use Eq. 3210, except we rearrange for the mass, m= qrB 2(1.601019 C)(4.72 m)(1.33 T) = = 9.431027 kg v 0.710(3.00108 m/s)
However, if it is moving at this velocity then the "mass" which we have here is not the true mass, but a relativistic correction. For a particle moving at 0.710c we have = 1 1 v 2 /c2 = 1 1  (0.710)2 = 1.42,
so the true mass of the particle is (9.431027 kg)/(1.42) = 6.641027 kg. The number of nucleons present in this particle is then (6.641027 kg)/(1.671027 kg) = 3.97 4. The charge was +2, which implies two protons, the other two nucleons would be neutrons, so this must be an alpha particle. E3222 (a) Since 950 GeV is much, much greater than 938 MeV the proton is ultrarelativistic. = E/mc2 , so v 1 m2 c4 m2 c4 = 1 2 = 1 1 0.9999995. c E2 2E 2 (b) Ultrarelativistic motion requires pc E, so B = pc/qRc = (950 GeV)/e(750 m)(3.00108 m/s) = 4.44 T.
99
E3223 First use 2f = qB/m. The use K = q 2 B 2 R2 /2m = mR2 (2f )2 /2. The number of turns is n = K/2qV , on average the particle is located at a distance R/ 2 from the center, so the distance traveled is x = n2R/ 2 = n 2R. Combining, 3 3 3 2 R mf 2 2 (0.53 m)3 (2 932103 keV/c2 )(12106 /s)2 x= = = 240 m. qV e(80 kV) E3224 The particle moves in a circle. x = R sin t and y = R cos t. E3225 We will use Eq. 3220, E H = v d B, except we will not take the derivation through to Eq. 3221. Instead, we will set the drift velocity equal to the speed of the strip. We will, however, set E H = V H /w. Then v= EH V H /w (3.9106 V)/(0.88102 m) = = = 3.7101 m/s. B B (1.2103 T)
E3226 (a) v = E/B = (40106 V)/(1.2102 m)/(1.4 T) = 2.4103 m/s. (b) n = (3.2 A)(1.4 T)/(1.61019 C)(9.5106 m)(40106 V) = 7.41028 /m3 .; Silver. E3227 E H = v d B and v d = j/ne. Combine and rearrange. E3228 (a) Use the result of the previous exercise and E c = j. (b) (0.65 T)/(8.491028 /m3 )(1.601019 C)(1.69108 m) = 0.0028. E3229 Since L is perpendicular to B can use FB = iLB. Equating the two forces, iLB i = mg, (0.0130 kg)(9.81 m/s2 ) mg = = = 0.467 A. LB (0.620 m)(0.440 T)
Use of an appropriate right hand rule will indicate that the current must be directed to the right in order to have a magnetic force directed upward. E3230 F = iLB sin = (5.12 103 A)(100 m)(58 106 T) sin(70 ) = 27.9 N. The direction is horizontally west. E3231 (a) We use Eq. 3226 again, and since the (horizontal) axle is perpendicular to the vertical component of the magnetic field, i= F (10, 000 N) = = 3.3108 A. BL (10 T)(3.0 m)
(b) The power lost per ohm of resistance in the rails is given by P/r = i2 = (3.3108 A)2 = 1.11017 W. (c) If such a train were to be developed the rails would melt well before the train left the station. 100
E3232 F = idB, so a = F/m = idB/m. Since a is constant, v = at = idBt/m. The direction is to the left. E3233 Only the ^ component of B is of interest. Then F = j
3.2
dF = i
By dx, or
F = (5.0 A)(8103 T/m2 )
1.2
x2 dx = 0.414 N.
^ The direction is k. E3234 The magnetic force will have two components: one will lift vertically (Fy = F sin ), the other push horizontally (Fx = F cos ). The rod will move when Fx > (W  Fy ). We are interested in the minimum value for F as a function of . This occurs when d dF = d d W cos + sin = 0.
This happens when = tan . Then = arctan(0.58) = 30 , and F = (0.58)(1.15 kg)(9.81 m/s2 ) = 5.66 N cos(30 ) + (0.58) sin(30 )
is the minimum force. Then B = (5.66 N)/(53.2 A)(0.95 m) = 0.112 T. E3235 We choose that the field points from the shorter side to the longer side. (a) The magnetic field is parallel to the 130 cm side so there is no magnetic force on that side. The magnetic force on the 50 cm side has magnitude FB = iLB sin , where is the angle between the 50 cm side and the magnetic field. This angle is larger than 90 , but the sine can be found directly from the triangle, sin = (120 cm) = 0.923, (130 cm)
and then the force on the 50 cm side can be found by FB = (4.00 A)(0.50 m)(75.0103 T) and is directed out of the plane of the triangle. The magnetic force on the 120 cm side has magnitude FB = iLB sin , where is the angle between the 1200 cm side and the magnetic field. This angle is larger than 180 , but the sine can be found directly from the triangle, sin = (50 cm) = 0.385, (130 cm) (120 cm) = 0.138 N, (130 cm)
and then the force on the 50 cm side can be found by FB = (4.00 A)(1.20 m)(75.0103 T) and is directed into the plane of the triangle. (b) Look at the three numbers above. 101 (50 cm) = 0.138 N, (130 cm)
E3236 = N iAB sin , so = (20)(0.1 A)(0.12 m)(0.05 m)(0.5 T) sin(90  33 ) = 5.0103 N m. E3237 The external magnetic field must be in the plane of the clock/wire loop. The clockwise current produces a magnetic dipole moment directed into the plane of the clock. (a) Since the magnetic field points along the 1 pm line and the torque is perpendicular to both the external field and the dipole, then the torque must point along either the 4 pm or the 10 pm line. Applying Eq. 3235, the direction is along the 4 pm line. It will take the minute hand 20 minutes to get there. (b) = (6)(2.0 A)(0.15 m)2 (0.07 T) = 0.059 N m. ^ P321 Since F must be perpendicular to B then B must be along k. The magnitude of v is 2 + (35)2 km/s = 53.1 km/s; the magnitude of F is 2 + (4.8)2 fN = 6.38 fN. Then (40) (4.2) B = F/qv = (6.381015 N)/(1.61019 C)(53.1103 m/s) = 0.75 T. ^ or B = 0.75 T k. P322 a = (q/m)(E + v B). For the initial velocity given, ^ v B = (15.0103 m/s)(400106 T)^  (12.0103 m/s)(400106 T)k. j ^ But since there is no acceleration in the ^ or k direction this must be offset by the electric field. j Consequently, two of the electric field components are Ey = 6.00 V/m and Ez = 4.80 V/m. The third component of the electric field is the source of the acceleration, so Ex = max /q = (9.111031 kg)(2.001012 m/s2 )/(1.601019 C) = 11.4 V/m. P323 (a) Consider first the cross product, v B. The electron moves horizontally, there is a component of the B which is down, so the cross product results in a vector which points to the left of the electron's path. But the force on the electron is given by F = qv B, and since the electron has a negative charge the force on the electron would be directed to the right of the electron's path. (b) The kinetic energy of the electrons is much less than the rest mass energy, so this is nonrelativistic motion. The speed of the electron is then v = 2K/m, and the magnetic force on the electron is FB = qvB, where we are assuming sin = 1 because the electron moves horizontally through a magnetic field with a vertical component. We can ignore the effect of the magnetic field's horizontal component because the electron is moving parallel to this component. The acceleration of the electron because of the magnetic force is then a = = qvB qB = m m 2K , m 2(1.921015 J) = 6.271014 m/s2 . (9.111031 kg)
(1.601019 C)(55.0106 T) (9.111031 kg)
(c) The electron travels a horizontal distance of 20.0 cm in a time of t= (20.0 cm) 2K/m = (20.0 cm) 2(1.921015 J)/(9.111031 kg) = 3.08109 s.
In this time the electron is accelerated to the side through a distance of d= 1 1 2 at = (6.271014 m/s2 )(3.08109 s)2 = 2.98 mm. 2 2 102
P324 (a) d needs to be larger than the turn radius, so R d; but 2mK/q 2 B 2 = R2 d2 , or B 2mK/q 2 d2 . (b) Out of the page. P325 Only undeflected ions emerge from the velocity selector, so v = E/B. The ions are then deflected by B with a radius of curvature of r = mv/qB; combining and rearranging, q/m = E/rBB . P326 The ions are given a kinetic energy K = qV ; they are then deflected with a radius of curvature given by R2 = 2mK/q 2 B 2 . But x = 2R. Combine all of the above, and m = B 2 qx2 /8V. P327 (a) Start with the equation in Problem 6, and take the square root of both sides to get m= B2q 8V
1 2
x,
and then take the derivative of x with respect to m, 1 dm = 2 m B2q 8V
1 2
dx,
and then consider finite differences instead of differential quantities, m = (b) Invert the above expression, x = and then put in the given values, x = = 2(7.33103 V) 27 kg)(0.520 T)2 (1.601019 C) (35.0)(1.6610 8.02 mm.
1 2
mB 2 q 2V
1 2
x,
2V mB 2 q
1 2
m,
(2.0)(1.661027 kg),
Note that we used 35.0 u for the mass; if we had used 37.0 u the result would have been closer to the answer in the back of the book. P328 (a) B = 2V m/qr2 = 2(0.105 MV)(238)(932 MeV/c2 )/2e(0.973 m)2 = 5.23107 T. (b) The number of atoms in a gram is 6.021023 /238 = 2.531021 . The current is then (0.090)(2.531021 )(2)(1.61019 C)/(3600 s) = 20.2 mA. P329 (a) q. (b) Regardless of speed, the orbital period is T = 2m/qB. But they collide halfway around a complete orbit, so t = m/qB. P3210
103
P3211
(a) The period of motion can be found from the reciprocal of Eq. 3212, T = 2m 2(9.111031 kg) = = 7.86108 s. qB (1.601019 C)(455106 T)
(b) We need to find the velocity of the electron from the kinetic energy, v= 2K/m = 2(22.5 eV)(1.601019 J/eV)/(9.111031 kg) = 2.81106 m/s.
The velocity can written in terms of components which are parallel and perpendicular to the magnetic field. Then v = v cos and v = v sin . The pitch is the parallel distance traveled by the electron in one revolution, so p = v T = (2.81106 m/s) cos(65.5 )(7.86108 s) = 9.16 cm. (c) The radius of the helical path is given by Eq. 3210, except that we use the perpendicular velocity component, so R=
b
(9.111031 kg)(2.81106 m/s) sin(65.5 ) mv = = 3.20 cm qB (1.601019 C)(455106 T)
P3212 F = i a dl B. dl has two components, those parallel to the path, say dx and those perpendicular, say dy. Then the integral can be written as
b b
F=
a
dx B +
a
dy B.
b
But B is constant, and can be removed from the integral. a dx = l, a vector that points from a to b b. a dy = 0, because there is no net motion perpendicular to l. P3213 qvy B = Fx = m dvx /dt; qvx B = Fy = m dvy /dt. Taking the time derivative of the second expression and inserting into the first we get qvy B = m  m qB d2 vy , dt2
which has solution vy = v sin(mt/qB), where v is a constant. Using the second equation we find that there is a similar solution for vx , except that it is out of phase, and so vx = v cos(mt/qB). Integrating, qBv x = vx dt = v cos(mt/qB) = sin(mt/qB). m Similarly, qBv y = vy dt = v sin(mt/qB) = cos(mt/qB). m This is the equation of a circle. P3214 dL = ^ + ^ + kdz. B is uniform, so that the integral can be written as idx jdy ^ F=i but since dx = (^ + ^ + kdz) B = i^ B idx jdy ^ i dy = dx + i^ B j ^ dy + ik B dz,
dz = 0, the entire expression vanishes. 104
P3215
The current pulse provides an impulse which is equal to F dt = BiL dt = BL i dt = BLq.
This gives an initial velocity of v0 = BLq/m, which will cause the rod to hop to a height of
2 h = v0 /2g = B 2 L2 q 2 /2m2 g.
Solving for q, q= P3216 P3217 The torque on a current carrying loop depends on the orientation of the loop; the maximum torque occurs when the plane of the loop is parallel to the magnetic field. In this case the magnitude of the torque is from Eq. 3234 with sin = 1 = N iAB. The area of a circular loop is A = r2 where r is the radius, but since the circumference is C = 2r, we can write C2 A= . 4 The circumference is not the length of the wire, because there may be more than one turn. Instead, C = L/N , where N is the number of turns. Finally, we can write the torque as = Ni L2 iL2 B B= , 4N 2 4N m BL 2gh = (0.013 kg) (0.12 T)(0.20 m) 2(9.8 m/s2 )(3.1 m) = 4.2 C.
which is a maximum when N is a minimum, or N = 1. P3218 dF = i dL B; the direction of dF will be upward and somewhat toward the center. L and B are a right angles, but only the upward component of dF will survive the integration as the central components will cancel out by symmetry. Hence F = iB sin P3219 dL = 2riB sin .
The torque on the cylinder from gravity is g = mgr sin ,
where r is the radius of the cylinder. The torque from magnetism needs to balance this, so mgr sin = N iAB sin = N i2rLB sin , or i= mg (0.262 kg)(9.8 m/s2 ) = = 1.63 A. 2N LB 2(13)(0.127 m)(0.477 T)
105
E331 (a) The magnetic field from a moving charge is given by Eq. 335. If the protons are moving side by side then the angle is = /2, so B= 0 qv 4 r2
and we are interested is a distance r = d. The electric field at that distance is E= 1 q , 4 0 r2
where in both of the above expressions q is the charge of the source proton. On the receiving end is the other proton, and the force on that proton is given by F = q(E + v B). The velocity is the same as that of the first proton (otherwise they wouldn't be moving side by side.) This velocity is then perpendicular to the magnetic field, and the resulting direction for the cross product will be opposite to the direction of E. Then for balance, E 1 q 4 0 r2 1 0 0 = vB, 0 qv = v , 4 r2 = v2 .
We can solve this easily enough, and we find v 3 108 m/s. (b) This is clearly a relativistic speed! E332 B = 0 i/2d = (4 107 T m/A)(120 A)/2(6.3 m) = 3.8106 T. This will deflect the compass needle by as much as one degree. However, there is unlikely to be a place on the Earth's surface where the magnetic field is 210 T. This was likely a typo, and should probably have been 21.0 T. The deflection would then be some ten degrees, and that is significant. E333 B = 0 i/2d = (4107 T m/A)(50 A)/2(1.3103 m) = 37.7103 T. E334 (a) i = 2dB/0 = 2(8.13102 m)(39.0106 T)/(4107 T m/A) = 15.9 A. (b) Due East. E335 Use B= 0 i (4107 N/A2 )(1.6 1019 C)(5.6 1014 s1 ) = = 1.2108 T. 2d 2(0.0015 m)
E336 Zero, by symmetry. Any contributions from the top wire are exactly canceled by contributions from the bottom wire. E337 B = 0 i/2d = (4107 T m/A)(48.8 A)/2(5.2102 m) = 1.88104 T. F = qv B. All cases are either parallel or perpendicular, so either F = 0 or F = qvB. (a) F = qvB = (1.601019 C)(1.08107 m/s)(1.88104 T) = 3.241016 N. The direction of F is parallel to the current. (b) F = qvB = (1.601019 C)(1.08107 m/s)(1.88104 T) = 3.241016 N. The direction of F is radially outward from the current. (c) F = 0. 106
E338 We want B1 = B2 , but with opposite directions. Then i1 /d1 = i2 /d2 , since all constants cancel out. Then i2 = (6.6 A)(1.5 cm)/(2.25 cm) = 4.4 A, directed out of the page. E339 For a single long straight wire, B = 0 i/2d but we need a factor of "2" since there are two wires, then i = dB/0 . Finally i= dB (0.0405 m)(296, T) = = 30 A 0 (4107 N/A2 )
E3310 (a) The semicircle part contributes half of Eq. 3321, or 0 i/4R. Each long straight wire contributes half of Eq. 3313, or 0 i/4R. Add the three contributions and get Ba = 0 i 4R 2 +1 = (4107 N/A2 )(11.5 A) 4(5.20103 m) 2 +1 = 1.14103 T.
The direction is out of the page. (b) Each long straight wire contributes Eq. 3313, or 0 i/2R. Add the two contributions and get 0 i (4107 N/A2 )(11.5 A) = = 8.85104 T. Ba = R (5.20103 m) The direction is out of the page. E3311 z 3 = 0 iR2 /2B = (4 107 N/A2 )(320)(4.20 A)(2.40102 m)2 /2(5.0106 T) = 9.73 102 m3 . Then z = 0.46 m. E3312 The circular part contributes a fraction of Eq. 3321, or 0 i/4R. Each long straight wire contributes half of Eq. 3313, or 0 i/4R. Add the three contributions and get B= 0 i (  2). 4R
The goal is to get B = 0 that will happen if = 2 radians. E3313 There are four current segments that could contribute to the magnetic field. The straight segments, however, contribute nothing because the straight segments carry currents either directly toward or directly away from the point P . That leaves the two rounded segments. Each contribution to B can be found by starting with Eq. 3321, or 0 i/4b. The direction is out of the page. There is also a contribution from the top arc; the calculations are almost identical except that this is pointing into the page and r = a, so 0 i/4a. The net magnetic field at P is then B = B1 + B2 = 0 i 4 1 1  b a .
E3314 For each straight wire segment use Eq. 3312. When the length of wire is L, the distance to the center is W/2; when the length of wire is W the distance to the center is L/2. There are four terms, but they are equal in pairs, so B = = 0 i 4 4L W L2 /4 + W 2 /4 + , + W 2 /4 20 i L2 + W 2 = . WL L2 /4 4W
L
20 i L2 + W 2
L2 W2 + WL WL 107
E3315 We imagine the ribbon conductor to be a collection of thin wires, each of thickness dx and carrying a current di. di and dx are related by di/dx = i/w. The contribution of one of these thin wires to the magnetic field at P is dB = 0 di/2x, where x is the distance from this thin wire to the point P . We want to change variables to x and integrate, so B= dB = 0 i dx 0 i = 2wx 2w d+w d dx . x
The limits of integration are from d to d + w, so B= 0 i ln 2w .
E3316 The fields from each wire are perpendicular at P . Each contributes an amount B = 0 i/2d, but since they are perpendicular there is a net field of magnitude B = 2B 2 = 20 i/2d. Note that a = 2d, so B = 0 i/a. (a) B = (4107 T m/A)(115 A)/(0.122 m) = 3.77104 T. The direction is to the left. (b) Same numerical result, except the direction is up. E3317 Follow along with Sample Problem 334. Reversing the direction of the second wire (so that now both currents are directed out of the page) will also reverse the direction of B2 . Then B = B1  B2 = = = 0 i 2 0 i 0 i 1 1  2 b + x b  x (b  x)  (b + x) , b2  x2 x . 2  b2 x ,
E3318 (b) By symmetry, only the horizontal component of B survives, and must point to the right. (a) The horizontal component of the field contributed by the top wire is given by B= 0 i b/2 0 ib 0 i sin = = , 2h 2h h (4R2 + b2 )
since h is the hypotenuse, or h = R2 + b2 /4. But there are two such components, one from the top wire, and an identical component from the bottom wire. E3319 loop, (a) We can use Eq. 3321 to find the magnetic field strength at the center of the large B=
0 i (4107 T m/A)(13 A) = = 6.8105 T. 2R 2(0.12 m) (b) The torque on the smaller loop in the center is given by Eq. 3234, = N iA B, but since the magnetic field from the large loop is perpendicular to the plane of the large loop, and the plane of the small loop is also perpendicular to the plane of the large loop, the magnetic field is in the plane of the small loop. This means that A B = AB. Consequently, the magnitude of the torque on the small loop is = N iAB = (50)(1.3 A)()(8.2103 m)2 (6.8105 T) = 9.3107 N m. 108
E3320 (a) There are two contributions to the field. One is from the circular loop, and is given by 0 i/2R. The other is from the long straight wire, and is given by 0 i/2R. The two fields are out of the page and parallel, so 0 i B= (1 + 1/). 2R (b) The two components are now at right angles, so B= 0 i 2R 1 + 1/ 2 .
The direction is given by tan = 1/ or = 18 . E3321 The force per meter for any pair of parallel currents is given by Eq. 3325, F/L = 0 i2 /2d, where d is the separation. The direction of the force is along the line connecting the intersection of the currents with the perpendicular plane. Each current experiences three forces; two are at right 2 2 angles and equal in magnitude, so F12 + F14 /L = F12 + F14 /L = 20 i2 /2a. The third force points parallel to this sum, but d = a, so the resultant force is 20 i2 0 i2 4 107 N/A2 (18.7 A)2 F = + = ( 2 + 1/ 2) = 6.06104 N/m. L 2a 2(0.245 m) 2 2a It is directed toward the center of the square. E3322 By symmetry we expect the middle wire to have a net force of zero; the two on the outside will each be attracted toward the center, but the answers will be symmetrically distributed. For the wire which is the farthest left, F 0 i2 = L 2 1 1 1 1 + + + a 2a 3a 4a = 4 107 N/A2 (3.22 A)2 2(0.083 m) 1+ 1 1 1 + + 2 3 4 = 5.21105 N/m.
For the second wire over, the contributions from the two adjacent wires should cancel. This leaves F 0 i2 = L 2 E3323 1 1 + + 2a 3a = 4 107 N/A2 (3.22 A)2 2(0.083 m) 1 1 + 2 3 = 2.08105 N/m.
(a) The force on the projectile is given by the integral of dF = i dl B
over the length of the projectile (which is w). The magnetic field strength can be found from adding together the contributions from each rail. If the rails are circular and the distance between them is small compared to the length of the wire we can use Eq. 3313, B= 0 i , 2x
where x is the distance from the center of the rail. There is one problem, however, because these are not wires of infinite length. Since the current stops traveling along the rail when it reaches the projectile we have a rod that is only half of an infinite rod, so we need to multiply by a factor of 1/2. But there are two rails, and each will contribute to the field, so the net magnetic field strength between the rails is 0 i 0 i B= + . 4x 4(2r + w  x) 109
In that last term we have an expression that is a measure of the distance from the center of the lower rail in terms of the distance x from the center of the upper rail. The magnitude of the force on the projectile is then
r+w
F
= i
r
B dx, dx,
= =
0 i2 r+w 1 1 + 4 r x 2r + w  x 0 i2 r+w 2 ln 4 r
The current through the projectile is down the page; the magnetic field through the projectile is into the page; so the force on the projectile, according to F = il B, is to the right. (b) Numerically the magnitude of the force on the rail is F = (450103 A)2 (4107 N/A2 ) ln 2 (0.067 m) + (0.012 m) (0.067 m) = 6.65103 N
The speed of the rail can be found from either energy conservation so we first find the work done on the projectile, W = F d = (6.65103 N)(4.0 m) = 2.66104 J. This work results in a change in the kinetic energy, so the final speed is v= 2K/m = 2(2.66104 J)/(0.010 kg) = 2.31103 m/s.
E3324 The contributions from the left end and the right end of the square cancel out. This leaves the top and the bottom. The net force is the difference, or F = = (4107 N/A2 )(28.6 A)(21.8 A)(0.323 m) 2 3.27103 N. 1 1  2 m) (1.1010 (10.30102 m) ,
E3325 The magnetic force on the upper wire near the point d is FB = 0 ia ib L 0 ia ib L 0 ia ib L  x, 2(d + x) 2d 2d2
where x is the distance from the equilibrium point d. The equilibrium magnetic force is equal to the force of gravity mg, so near the equilibrium point we can write x FB = mg  mg . d There is then a restoring force against small perturbations of magnitude mgx/d which corresponds to a spring constant of k = mg/d. This would give a frequency of oscillation of f= which is identical to the pendulum. E3326 B = (4107 N/A2 )(3.58 A)(1230)/(0.956m) = 5.79103 T. 1 2 k/m = 1 2 g/d,
110
E3327 The magnetic field inside an ideal solenoid is given by Eq. 3328 B = 0 in, where n is the turns per unit length. Solving for n, n= B (0.0224 T) = = 1.00103 /m1 . 0 i (4107 N/A2 )(17.8 A)
The solenoid has a length of 1.33 m, so the total number of turns is N = nL = (1.00103 /m1 )(1.33 m) = 1330, and since each turn has a length of one circumference, then the total length of the wire which makes up the solenoid is (1330)(0.026 m) = 109 m. E3328 From the solenoid we have B s = 0 nis = 0 (11500/m)(1.94 mA) = 0 (22.3A/m). From the wire we have 0 iw 0 (6.3 A) 0 = = (1.002 A) 2r 2r r These fields are at right angles, so we are interested in when tan(40 ) = B w /B s , or Bw = r= E3329 Let u = z  d. Then B = = = 0 niR2 2
2 d+L/2 dL/2
(1.002 A) = 5.35102 m. tan(40 )(22.3 A/m)
du , [R2 + u2 ]3/2
d+L/2
u 0 niR 2 R 2 R 2 + u2 0 ni 2 d + L/2 R2 + (d +
,
dL/2
L/2)2

d  L/2 R2 + (d  L/2)2
.
If L is much, much greater than R and d then L/2 d >> R, and R can be ignored in the denominator of the above expressions, which then simplify to B = 0 ni 2 0 ni 2 d + L/2 R2 + (d + L/2)2   d  L/2 R2 + (d  L/2)2 . .
=
d + L/2 (d + L/2)2
d  L/2 (d  L/2)2
= 0 in. It is important that we consider the relative size of L/2 and d! E3330 The net current in the loop is 1i0 + 3i0 + 7i0  6i0 = 5i0 . Then B ds = 50 i0 .
E3331 (a) The path is clockwise, so a positive current is into page. The net current is 2.0 A out, so B ds = 0 i0 = 2.5106 T m. (b) The net current is zero, so B ds = 0. 111
E3332 Let R0 be the radius of the wire. On the surface of the wire B0 = 0 i/2R0 . Outside the wire we have B = 0 i/2R, this is half B0 when R = 2R0 . 2 Inside the wire we have B = 0 iR/2R0 , this is half B0 when R = R0 /2. E3333 looks like (a) We don't want to reinvent the wheel. The answer is found from Eq. 3334, except it B=
0 ir . 2c2 (b) In the region between the wires the magnetic field looks like Eq. 3313, B= 0 i . 2r
This is derived on the right hand side of page 761. (c) Ampere's law (Eq. 3329) is B ds = 0 i, where i is the current enclosed. Our Amperian loop will still be a circle centered on the axis of the problem, so the left hand side of the above equation will reduce to 2rB, just like in Eq. 3332. The right hand side, however, depends on the net current enclosed which is the current i in the center wire minus the fraction of the current enclosed in the outer conductor. The cross sectional area of the outer conductor is (a2  b2 ), so the fraction of the outer current enclosed in the Amperian loop is i The net current in the loop is then ii so the magnetic field in this region is B= 0 i a2  r2 . 2r a2  b2 r 2  b2 a2  r2 =i 2 , a2  b2 a  b2 (r2  b2 ) r 2  b2 =i 2 . 2  b2 ) (a a  b2
(d) This part is easy since the net current is zero; consequently B = 0. E3334 (a) Ampere's law (Eq. 3329) is B ds = 0 i, where i is the current enclosed. Our Amperian loop will still be a circle centered on the axis of the problem, so the left hand side of the above equation will reduce to 2rB, just like in Eq. 3332. The right hand side, however, depends on the net current enclosed which is the fraction of the current enclosed in the conductor. The cross sectional area of the conductor is (a2  b2 ), so the fraction of the current enclosed in the Amperian loop is (r2  b2 ) r 2  b2 i =i 2 . (a2  b2 ) a  b2 The magnetic field in this region is B= (b) If r = a, then B= which is what we expect. 0 i a2  b2 0 i = , 2a a2  b2 2a 0 i r2  b2 . 2r a2  b2
112
If r = b, then B= which is what we expect. If b = 0, then B= which is what I expected. E3335 The magnitude of the magnetic field due to the cylinder will be zero at the center of the cylinder and 0 i0 /2(2R) at point P . The magnitude of the magnetic field field due to the wire will be 0 i/2(3R) at the center of the cylinder but 0 i/2R at P . In order for the net field to have different directions in the two locations the currents in the wire and pipe must be in different direction. The net field at the center of the pipe is 0 i/2(3R), while that at P is then 0 i0 /2(2R)  0 i/2R. Set these equal and solve for i; i/3 = i0 /2  i, or i = 3i0 /8. E3336 (a) B = (4107 N/A2 )(0.813 A)(535)/2(0.162 m) = 5.37104 T. (b) B = (4107 N/A2 )(0.813 A)(535)/2(0.162 m + 0.052 m) = 4.07104 T. E3337 (a) A positive particle would experience a magnetic force directed to the right for a magnetic field out of the page. This particle is going the other way, so it must be negative. (b) The magnetic field of a toroid is given by Eq. 3336, 0 iN , 2r while the radius of curvature of a charged particle in a magnetic field is given by Eq. 3210 mv R= . qB B= We use the R to distinguish it from r. Combining, R= 2mv r, 0 iN q 0 i r2  02 0 ir = 2r a2  02 2a2 0 i b2  b2 = 0, 2b a2  b2
so the two radii are directly proportional. This means R/(11 cm) = (110 cm)/(125 cm), so R = 9.7 cm. P331 The field from one coil is given by Eq. 3319 B= 0 iR2 . 2(R2 + z 2 )3/2
There are N turns in the coil, so we need a factor of N . There are two coils and we are interested in the magnetic field at P , a distance R/2 from each coil. The magnetic field strength will be twice the above expression but with z = R/2, so B= 20 N iR2 80 N i = . 2 + (R/2)2 )3/2 2(R (5)3/2 R 113
P332
(a) Change the limits of integration that lead to Eq. 3312: B = = = 0 id 4
L 0
(z 2
dz , + d2 )3/2
L
z 0 id , 4 (z 2 + d2 )1/2 0 0 id L . 4 (L2 + d2 )1/2
(b) The angle in Eq. 3311 would always be 0, so sin = 0, and therefore B = 0. P333 This problem is the all important derivation of the Helmholtz coil properties. (a) The magnetic field from one coil is B1 = 0 N iR2 . 2(R2 + z 2 )3/2
The magnetic field from the other coil, located a distance s away, but for points measured from the first coil, is 0 N iR2 B2 = . 2(R2 + (z  s)2 )3/2 The magnetic field on the axis between the coils is the sum, B= 0 N iR2 0 N iR2 + . 2(R2 + z 2 )3/2 2(R2 + (z  s)2 )3/2
Take the derivative with respect to z and get 30 N iR2 30 N iR2 dB = z (z  s). 2 + z 2 )5/2 2 + (z  s)2 )5/2 dz 2(R 2(R At z = s/2 this expression vanishes! We expect this by symmetry, because the magnetic field will be strongest in the plane of either coil, so the midpoint should be a local minimum. (b) Take the derivative again and d2 B dz 2 =  30 N iR2 150 N iR2 2 + z 2 + z 2 )5/2 2(R 2(R2 + z 2 )5/2 30 N iR2 150 N iR2  + (z  s)2 . 2 + (z  s)2 )5/2 2 + (z  s)2 )5/2 2(R 2(R
We could try and simplify this, but we don't really want to; we instead want to set it equal to zero, then let z = s/2, and then solve for s. The second derivative will equal zero when 3(R2 + z 2 ) + 15z 2  3(R2 + (z  s)2 ) + 15(z  s)2 = 0, and is z = s/2 this expression will simplify to 30(s/2)2 = 6(R2 + (s/2)2 ), 4(s/2)2 = R2 , s = R.
114
P334 (a) Each of the side of the square is a straight wire segment of length a which contributes a field strength of a 0 i , B= 4r a2 /4 + r2 where r is the distance to the point on the axis of the loop, so r= a2 /4 + z 2 .
This field is not parallel to the z axis; the z component is Bz = B(a/2)/r. There are four of these contributions. The off axis components cancel. Consequently, the field for the square is B = = = = (b) When z = 0 this reduces to B= 40 i a2 40 i = . (a2 ) 2a2 2 a 4 0 i 4r a a2 /4 a
2
+
r2
a/2 , r , a2 ,
0 i 2r2
a2 /4 + r2
0 i 2 /4 + z 2 ) 2(a (a2
a2 /2 + z 2
40 i a2 . 2) + 4z 2a2 + 4z 2
P335 (a) The polygon has n sides. A perpendicular bisector of each side can be drawn to the center and has length x where x/a = cos(/n). Each side has a length L = 2a sin(/n). Each of the side of the polygon is a straight wire segment which contributes a field strength of B= 0 i 4x L L2 /4 + x2 ,
This field is parallel to the z axis. There are n of these contributions. The off axis components cancel. Consequently, the field for the polygon B = n = n = n since (L/2)2 + x2 = a2 . (b) Evaluate:
n
0 i 4x 0 i 4
L L2 /4 2 L2 /4 + x2 + x2
, tan(/n),
0 i 1 tan(/n), 2 a
lim n tan(/n) = lim n sin(/n) n/n = .
n
Then the answer to part (a) simplifies to B= 0 i . 2a
115
P336 For a square loop of wire we have four finite length segments each contributing a term which looks like Eq. 3312, except that L is replaced by L/4 and d is replaced by L/8. Then at the center, L/4 160 i 0 i . = B=4 2 /64 + L2 /64 4L/8 L 2L For a circular loop R = L/2 so 0 i 0 = . 2R L Since 16/ 2 > , the square wins. But only by some 7%! B= P337 We want to use the differential expression in Eq. 3311, except that the limits of integration are going to be different. We have four wire segments. From the top segment, B1 = = 0 i d 4 z 2 + d2 0 i 4d
3L/4
,
L/4
3L/4 (3L/4)2 + d2

L/4 (L/4)2 + d2
.
For the top segment d = L/4, so this simplifies even further to 0 i B1 = 2(3 5 + 5) . 10L The bottom segment has the same integral, but d = 3L/4, so 0 i B3 = 2( 5 + 5) . 30L By symmetry, the contribution from the right hand side is the same as the bottom, so B2 = B3 , and the contribution from the left hand side is the same as that from the top, so B4 = B1 . Adding all four terms, 20 i 3 2(3 5 + 5) + 2( 5 + 5) , B = 30L 20 i = (2 2 + 10). 3L P338 Assume a current ring has a radius r and a width dr, the charge on the ring is dq = 2r dr, where = q/R2 . The current in the ring is di = dq/2 = r dr. The ring contributes a field dB = 0 di/2r. Integrate over all the rings:
R
B=
0
0 r dr/2r = 0 R/2 = q/2R.
P339
B = 0 in and mv = qBr. Combine, and i= mv (5.11105 eV/c2 )(0.046c) = = 0.271 A. 0 qrn (4107 N/A2 )e(0.023 m)(10000/m)
P3310
This shape is a triangle with area A = (4d)(3d)/2 = 6d2 . The enclosed current is then i = jA = (15 A/m2 )6(0.23 m)2 = 4.76 A
The line integral is then 0 i = 6.0106 T m. 116
P3311 Assume that B does vary as the picture implies. Then the line integral along the path shown must be nonzero, since B l on the right is not zero, while it is along the three other sides. Hence B dl is non zero, implying some current passes through the dotted path. But it doesn't, so B cannot have an abrupt change. P3312 (a) Sketch an Amperian loop which is a rectangle which enclosed N wires, has a vertical sides with height h, and horizontal sides with length L. Then B dl = 0 N i. Evaluate the integral along the four sides. The vertical side contribute nothing, since B is perpendicular to h, and then B h = 0. If the integral is performed in a counterclockwise direction (it must, since the sense of integration was determined by assuming the current is positive), we get BL for each horizontal section. Then 1 0 iN = 0 in. B= 2L 2 (b) As a then tan1 (a/2R) /2. Then B 0 i/2a. If we assume that i is made up of several wires, each with current i0 , then i/a = i0 n. P3313 Apply Ampere's law with an Amperian loop that is a circle centered on the center of the wire. Then B ds = B ds = B ds = 2rB, because B is tangent to the path and B is uniform along the path by symmetry. The current enclosed is ienc = j dA. This integral is best done in polar coordinates, so dA = (dr)(r d), and then
r 2
ienc
=
0 0
(j0 r/a) rdr d,
r
= = When r = a the current enclosed is i, so i=
2j0 /a
0
r2 dr,
2j0 3 r . 3a
2j0 a2 3i or j0 = . 3 2a2
The magnetic field strength inside the wire is found by gluing together the two parts of Ampere's law, 2rB B = 0 = = 2j0 3 r , 3a 0 j0 r2 , 3a 2 0 ir . 2a3
117
P3314 (a) According to Eq. 3334, the magnetic field inside the wire without a hole has magnitude B = 0 ir/2R2 = 0 jr/2 and is directed radially. If we superimpose a second current to create the hole, the additional field at the center of the hole is zero, so B = 0 jb/2. But the current in the remaining wire is i = jA = j(R2  a2 ), so B= 0 ib . 2(R2  a2 )
118
E341 B = B A = (42106 T)(2.5 m2 ) cos(57 ) = 5.7105 Wb. E342 E = dB /dt = A dB/dt = (/4)(0.112 m)2 (0.157 T/s) = 1.55 mV. E343 (a) The magnitude of the emf induced in a loop is given by Eq. 344, E = N dB , dt
= N (12 mWb/s2 )t + (7 mWb/s) There is only one loop, and we want to evaluate this expression for t = 2.0 s, so E = (1) (12 mWb/s2 )(2.0 s) + (7 mWb/s) = 31 mV. (b) This part isn't harder. The magnetic flux through the loop is increasing when t = 2.0 s. The induced current needs to flow in such a direction to create a second magnetic field to oppose this increase. The original magnetic field is out of the page and we oppose the increase by pointing the other way, so the second field will point into the page (inside the loop). By the right hand rule this means the induced current is clockwise through the loop, or to the left through the resistor. E344 E = dB /dt = A dB/dt. (a) E = (0.16 m)2 (0.5 T)/(2 s) = 2.0102 V. (b) E = (0.16 m)2 (0.0 T)/(2 s) = 0.0102 V. (c) E = (0.16 m)2 (0.5 T)/(4 s) = 1.0102 V. E345 (a) R = L/A = (1.69108 m)[()(0.104 m)]/[(/4)(2.50103 m)2 ] = 1.12103 . (b) E = iR = (9.66 A)(1.12103 ) = 1.08102 V. The required dB/dt is then given by dB E = = (1.08102 V)/(/4)(0.104 m)2 = 1.27 T/s. dt A E346 E = A B/t = AB/t. The power is P = iE = E 2 /R. The energy dissipated is E = P t = E 2 t A2 B 2 = . R Rt
E347 (a) We could rederive the steps in the sample problem, or we could start with the end result. We'll start with the result, di E = N A0 n , dt except that we have gone ahead and used the derivative instead of the . The rate of change in the current is di = (3.0 A/s) + (1.0 A/s2 )t, dt so the induced emf is E = = (130)(3.46104 m2 )(4107 Tm/A)(2.2104 /m) (3.0A/s) + (2.0A/s2 )t , (3.73103 V) + (2.48103 V/s)t.
(b) When t = 2.0 s the induced emf is 8.69103 V, so the induced current is i = (8.69103 V)/(0.15 ) = 5.8102 A. 119
E348 (a) i = E/R = N A dB/dt. Note that A refers to the area enclosed by the outer solenoid where B is nonzero. This A is then the cross sectional area of the inner solenoid! Then i= 1 di (120)(/4)(0.032 m)2 (4107 N/A2 )(220102 /m) (1.5 A) N A0 n = = 4.7103 A. R dt (5.3 ) (0.16 s)
E349 P = Ei = E 2 /R = (A dB/dt)2 /(L/a), where A is the area of the loop and a is the cross sectional area of the wire. But a = d2 /4 and A = L2 /4, so P = L3 d2 64 dB dt
2
=
(0.525 m)3 (1.1103 m)2 (9.82103 T/s)2 = 4.97106 W. 64(1.69108 m)
E3410 B = BA = B(2.3 m)2 /2. EB = dB /dt = AdB/dt, or EB =  so E = (2.0 V) + (2.3 V) = 4.3 V. E3411 (a) The induced emf, as a function of time, is given by Eq. 345, E(t) = dB (t)/dt This emf drives a current through the loop which obeys E(t) = i(t)R Combining, i(t) =  1 dB (t) . R dt (2.3 m)2 [(0.87 T/s)] = 2.30 V, 2
Since the current is defined by i = dq/dt we can write dq(t) 1 dB (t) = . dt R dt Factor out the dt from both sides, and then integrate: 1 dB (t), R 1 dq(t) =  dB (t), R 1 q(t)  q(0) = (B (0)  B (t)) R dq(t) =  (b) No. The induced current could have increased from zero to some positive value, then decreased to zero and became negative, so that the net charge to flow through the resistor was zero. This would be like sloshing the charge back and forth through the loop. E3412 P hiB = 2B = 2N BA. Then the charge to flow through is q = 2(125)(1.57 T)(12.2104 m2 )/(13.3 ) = 3.60102 C. E3413 The part above the long straight wire (a distance b  a above it) cancels out contributions below the wire (a distance b  a beneath it). The flux through the loop is then
a
B =
2ab
0 i 0 ib b dr = ln 2r 2
a 2a  b
.
120
The emf in the loop is then E = Evaluating, E= 4107 N/A2 (0.16 m) ln 2 (0.12 m) 2(0.12 m)  (0.16 m) [2(4.5 A/s2 )(3.0 s)(10 A/s)] = 2.20107 V. dB 0 b = ln dt 2 a 2a  b [2(4.5 A/s2 )t  (10 A/s)].
E3414 Use Eq. 346: E = BDv = (55106 T)(1.10 m)(25 m/s) = 1.5103 V. E3415 If the angle doesn't vary then the flux, given by =BA is constant, so there is no emf. E3416 (a) Use Eq. 346: E = BDv = (1.18T)(0.108 m)(4.86 m/s) = 0.619 V. (b) i = (0.619 V)/(0.415 ) = 1.49 A. (c) P = (0.619 V)(1.49 A) = 0.922 W. (d) F = iLB = (1.49 A)(0.108 m)(1.18T) = 0.190 N. (e) P = F v = (0.190 V)(4.86 m/s) = 0.923 W. E3417 The magnetic field is out of the page, and the current through the rod is down. Then Eq. 3226 F = iL B shows that the direction of the magnetic force is to the right; furthermore, since everything is perpendicular to everything else, we can get rid of the vector nature of the problem and write F = iLB. Newton's second law gives F = ma, and the acceleration of an object from rest results in a velocity given by v = at. Combining, v(t) = iLB t. m
E3418 (b) The rod will accelerate as long as there is a net force on it. This net force comes from F = iLB. The current is given by iR = E  BLv, so as v increases i decreases. When i = 0 the rod stops accelerating and assumes a terminal velocity. (a) E = BLv will give the terminal velocity. In this case, v = E/BL. E3419 E3420 The acceleration is a = R 2 ; since E = BR2 /2, we can find a = 4E 2 /B 2 R3 = 4(1.4 V)2 /(1.2 T)2 (5.3102 m)3 = 3.7104 m/s2 . E3421 We will use the results of Exercise 11 that were worked out above. All we need to do is find the initial flux; flipping the coil upsidedown will simply change the sign of the flux. So B (0) = B A = (59 T)()(0.13 m)2 sin(20 ) = 1.1106 Wb.
121
Then using the results of Exercise 11 we have q N (B (0)  B (t)), R 950 = ((1.1106 Wb)  (1.1106 Wb)), 85 = 2.5105 C. =
E3422 (a) The flux through the loop is
vt a+L
B =
0
dx
a
dr
0 i 0 ivt a + L = ln . 2r 2 a
The emf is then E = Putting in the numbers, E=
0 iv a + L dB = ln . dt 2 a
(4107 N/A2 )(110 A)(4.86 m/s) (0.0102 m) + (0.0983 m) ln = 2.53104 V. 2 (0.0102 m)
(b) i = E/R = (2.53104 V)/(0.415 ) = 6.10104 A. (c) P = i2 R = (6.10104 A)2 (0.415 ) = 1.54107 W. (d) F = Bil dl, or a+L 0 i 0 i a + L = il ln . F = il dr 2r 2 a a Putting in the numbers, F = (6.10104 A) (4107 N/A2 )(110 A) (0.0102 m) + (0.0983 m) ln = 3.17108 N. 2 (0.0102 m)
(e) P = F v = (3.17108 N)(4.86 m/s) = 1.54107 W. E3423 (a) Starting from the beginning, Eq. 3313 gives B= The flux through the loop is given by B = B dA, 0 i . 2y
but since the magnetic field from the long straight wire goes through the loop perpendicular to the plane of the loop this expression simplifies to a scalar integral. The loop is a rectangular, so use dA = dx dy, and let x be parallel to the long straight wire. Combining the above,
D+b a 0 D+b
B
=
D
0 i 2y
dx dy,
= =
0 i dy a , 2 y D 0 i D+b a ln 2 D 122
(b) The flux through the loop is a function of the distance D from the wire. If the loop moves away from the wire at a constant speed v, then the distance D varies as vt. The induced emf is then E =  = dB , dt 0 i b a . 2 t(vt + b)
The current will be this emf divided by the resistance R. The "backofthebook" answer is somewhat different; the answer is expressed in terms of D instead if t. The two answers are otherwise identical. E3424 (a) The area of the triangle is A = x2 tan /2. In this case x = vt, so B = B(vt)2 tan /2, and then E = 2Bv 2 t tan /2, (b) t = E/2Bv 2 tan /2, so t= E3425 E = N BA, so = That's 6.3 rev/second. E3426 (a) The frequency of the emf is the same as the frequency of rotation, f . (b) The flux changes by BA = Ba2 during a half a revolution. This is a sinusoidal change, so the amplitude of the sinusoidal variation in the emf is E = B /2. Then E = B 2 a2 f . E3427 We can use Eq. 3410; the emf is E = BA sin t, This will be a maximum when sin t = 1. The angular frequency, is equal to = (1000)(2)/(60) rad/s = 105 rad/s The maximum emf is then E = (3.5 T) [(100)(0.5 m)(0.3 m)] (105 rad/s) = 5.5 kV. E3428 (a) The amplitude of the emf is E = BA, so A = E/2f B = (150 V)/2(60/s)(0.50 T) = 0.798m2 . (b) Divide the previous result by 100. A = 79.8 cm2 . E3429 dB /dt = A dB/dt = A(8.50 mT/s). (a) For this path E ds = dB /dt =   (0.212 m)2 (8.50 mT/s) = 1.20 mV. (b) For this path E ds = dB /dt =   (0.323 m)2 (8.50 mT/s) = 2.79 mV. 123 (24 V) = 39.4 rad/s. (97)(0.33 T)(0.0190 m2 ) (56.8 V) = 2.08 s. 2(0.352 T)(5.21 m/s)2 tan(55 )
(c) For this path E ds = dB /dt =   (0.323 m)2 (8.50 mT/s)  (0.323 m)2 (8.50 mT/s) = 1.59 mV. E3430 dB /dt = A dB/dt = A(6.51 mT/s), while E ds = 2rE. (a) The path of integration is inside the solenoid, so E= (0.022 m)(6.51 mT/s) r2 (6.51 mT/s) = = 7.16105 V/m. 2r 2
(b) The path of integration is outside the solenoid, so E= r2 (6.51 mT/s) (0.063 m)2 (6.51 mT/s) = = 1.58104 V/m 2R 2(0.082 m)
E3431
The induced electric field can be found from applying Eq. 3413, E ds =  dB . dt
We start with the left hand side of this expression. The problem has cylindrical symmetry, so the induced electric field lines should be circles centered on the axis of the cylindrical volume. If we choose the path of integration to lie along an electric field line, then the electric field E will be parallel to ds, and E will be uniform along this path, so E ds = E ds = E ds = 2rE,
where r is the radius of the circular path. Now for the right hand side. The flux is contained in the path of integration, so B = Br2 . All of the time dependence of the flux is contained in B, so we can immediately write 2rE = r2 dB r dB or E =  . dt 2 dt
What does the negative sign mean? The path of integration is chosen so that if our right hand fingers curl around the path our thumb gives the direction of the magnetic field which cuts through the path. Since the field points into the page a positive electric field would have a clockwise orientation. Since B is decreasing the derivative is negative, but we get another negative from the equation above, so the electric field has a positive direction. Now for the magnitude. E = (4.82102 m)(10.7103 T /s)/2 = 2.58104 N/C. The acceleration of the electron at either a or c then has magnitude a = Eq/m = (2.58104 N/C)(1.601019 C)/(9.111031 kg) = 4.53107 m/s2 . P341 The induced current is given by i = E/R. The resistance of the loop is given by R = L/A, where A is the cross sectional area. Combining, and writing in terms of the radius of the wire, we have r2 E i= . L 124
The length of the wire is related to the radius of the wire because we have a fixed mass. The total volume of the wire is r2 L, and this is related to the mass and density by m = r2 L. Eliminating r we have mE i= . L2 The length of the wire loop is the same as the circumference, which is related to the radius R of the loop by L = 2R. The emf is related to the changing flux by E = dB /dt, but if the shape of the loop is fixed this becomes E = A dB/dt. Combining all of this, i= mA dB . (2R)2 dt
We dropped the negative sign because we are only interested in absolute values here. Now A = R2 , so this expression can also be written as i= mR2 dB m dB = . (2R)2 dt 4 dt
P342 For the lower surface B A = (76103 T)(/2)(0.037 m)2 cos(62 ) = 7.67105 Wb. For the upper surface B A = (76103 T)(/2)(0.037 m)2 cos(28 ) = 1.44104 Wb.. The induced emf is then E = (7.67105 Wb + 1.44104 Wb)/(4.5103 s) = 4.9102 V. P343 (a) We are only interested in the portion of the ring in the yz plane. Then E = (3.32 103 T/s)(/4)(0.104 m)2 = 2.82105 V. (b) From c to b. Point your right thumb along x to oppose the increasing B field. Your right fingers will curl from c to b. P344 E N A, but A = r2 and N 2r = L, so E 1/N . This means use only one loop to maximize the emf. P345 This is a integral best performed in rectangular coordinates, then dA = (dx)(dy). The magnetic field is perpendicular to the surface area, so B dA = B dA. The flux is then B = =
0 0
B dA =
a a
B dA,
(4 T/m s2 )t2 y dy dx, 1 2 a a, 2
= (4 T/m s2 )t2 = But a = 2.0 cm, so this becomes
(2 T/m s2 )a3 t2 .
B = (2 T/m s2 )(0.02 m)3 t2 = (1.6105 Wb/s2 )t2 . The emf around the square is given by dB = (3.2105 Wb/s2 )t, dt and at t = 2.5 s this is 8.0105 V. Since the magnetic field is directed out of the page, a positive emf would be counterclockwise (hold your right thumb in the direction of the magnetic field and your fingers will give a counter clockwise sense around the loop). But the answer was negative, so the emf must be clockwise. E = 125
P346 then
(a) Far from the plane of the large loop we can approximate the large loop as a dipole, and B= 0 iR2 . 2x3 0 i 2 r2 R2 . 2x3
The flux through the small loop is then B = r2 B = (b) E = dB /dt, so
30 i 2 r2 R2 v. 2x4 (c) Anticlockwise when viewed from above. E= P347 then The magnetic field is perpendicular to the surface area, so B dA = B dA. The flux is B = B dA = B dA = BA,
since the magnetic field is uniform. The area is A = r2 , where r is the radius of the loop. The induced emf is dB dr E = = 2rB . dt dt It is given that B = 0.785 T, r = 1.23 m, and dr/dt = 7.50102 m/s. The negative sign indicate a decreasing radius. Then E = 2(1.23 m)(0.785 T)(7.50102 m/s) = 0.455 V. P348 (a) dB /dt = B dA/dt, but dA/dt is A/t, where A is the area swept out during one rotation and t = 1/f . But the area swept out is R2 , so E = dB = f BR2 . dt
(b) If the output current is i then the power is P = Ei. But P = = 2f , so = P349 P = iBR2 /2. 2f
(a) E = dB /dt, and B = B A,so E = BLv cos .
The component of the force of gravity on the rod which pulls it down the incline is FG = mg sin . The component of the magnetic force on the rod which pulls it up the incline is FB = BiL cos . Equating, BiL cos = mg sin , and since E = iR, v= E mgR sin = 2 2 . BL cos B L cos2
(b) P = iE = E 2 /R = B 2 L2 v 2 cos2 /R = mgv sin . This is identical to the rate of change of gravitational potential energy. 126
P3410 Let the cross section of the wire be a. (a) R = L/a = (r + 2r)/a; with numbers, R = (3.4103 )(2 + ). (b) B = Br2 /2; with numbers, B = (4.32103 Wb). (c) i = E/R = Br2 /2R = Bar/2( + 2), or i= Take the derivative and set it equal to zero, 0= so at2 = 4, or = 1 at2 = 2 rad. 2 (d) = 2, so (0.15 T)(1.2106 m2 ) 2(12 rad/s )(2 rad)(0.24 m) i= (1.7108 m)(6 rad) = 2.2 A.
2
Batr . (t2 + 4)
4  at2 , (t2 + 4)2
P3411 It does say approximate, so we will be making some rather bold assumptions here. First we will find an expression for the emf. Since B is constant, the emf must be caused by a change in the area; in this case a shift in position. The small square where B = 0 has a width a and sweeps around the disk with a speed r. An approximation for the emf is then E = Bar. This emf causes a current. We don't know exactly where the current flows, but we can reasonably assume that it occurs near the location of the magnetic field. Let us assume that it is constrained to that region of the disk. The resistance of this portion of the disk is the approximately R= 1L 1 a 1 = = , A at t
where we have assumed that the current is flowing radially when defining the cross sectional area of the "resistor". The induced current is then (on the order of) E Bar = = Bart. R 1/(t) This current experiences a breaking force according to F = BIl, so F = B 2 a2 rt, where l is the length through which the current flows, which is a. Finally we can find the torque from = rF , and = B 2 a2 r2 t.
127
P3412 The induced electric field in the ring is given by Eq. 3411: 2RE = dB /dt. This electric field will result in a force on the free charge carries (electrons?), given by F = Ee. The acceleration of the electrons is then a = Ee/me . Then a= dB e . 2Rme dt
Integrate both sides with respect to time to find the speed of the electrons. a dt v = = = e dB dt, 2Rme dt dB e 2Rme , e B . 2Rme
The current density is given by j = nev, and the current by iA = ia2 . Combining, i= ne2 a2 P hiB . 2Rme
Actually, it should be pointed out that P hiB refers to the change in flux from external sources. The current induced in the wire will produce a flux which will exactly offset P hiB so that the net flux through the superconducting ring is fixed at the value present when the ring became superconducting. P3413 Assume that E does vary as the picture implies. Then the line integral along the path shown must be nonzero, since E l on the right is not zero, while it is along the three other sides. Hence E dl is non zero, implying a change in the magnetic flux through the dotted path. But it doesn't, so E cannot have an abrupt change. P3414 The electric field a distance r from the center is given by E= r2 dB/dT r dB = . 2r 2 dt
This field is directed perpendicular to the radial lines. Define h to be the distance from the center of the circle to the center of the rod, and evaluate E = E ds, E = = But h2 = R2  (L/2)2 , so E= P3415 (a) B = r2 B av , so E= E (0.32 m) = 2(0.28 T)(120 ) = 34 V/m. 2r 2 dB L dt 2 R2  (L/2)2 . dB rh dx, dt 2r dB L h. dt 2
(b) a = F/m = Eq/m = (33.8 V/m)(1.61019 C)/(9.11031 kg) = 6.01012 m/s2 . 128
E351 If the Earth's magnetic dipole moment were produced by a single current around the core, then that current would be i= (8.0 1022 J/T) = = 2.1109 A A (3.5 106 m)2
E352 (a) i = /A = (2.33 A m2 )/(160)(0.0193 m)2 = 12.4 A. (b) = B = (2.33 A m2 )(0.0346 T) = 8.06102 N m. E353 (a) Using the right hand rule a clockwise current would generate a magnetic moment which would be into the page. Both currents are clockwise, so add the moments: = (7.00 A)(0.20 m)2 + (7.00 A)(0.30 m)2 = 2.86 A m2 . (b) Reversing the current reverses the moment, so = (7.00 A)(0.20 m)2  (7.00 A)(0.30 m)2 = 1.10 A m2 . E354 (a) = iA = (2.58 A)(0.16 m)2 = 0.207 A m2 . (b) = B sin = (0.207 A m2 )(1.20 T) sin(41 ) = 0.163 N m. E355 (a) The result from Problem 334 for a square loop of wire was B(z) = 40 ia2 . (4z 2 + a2 )(4z 2 + 2a2 )1/2
For z much, much larger than a we can ignore any a terms which are added to or subtracted from z terms. This means that 4z 2 + a2 4z 2 and (4z 2 + 2a2 )1/2 2z, but we can't ignore the a2 in the numerator. The expression for B then simplifies to B(z) = which certainly looks like Eq. 354. (b) We can rearrange this expression and get B(z) = 0 ia2 , 2z 3 0 ia2 , 2z 3
where it is rather evident that ia2 must correspond to , the dipole moment, in Eq. 354. So that must be the answer. E356 = iA = (0.2 A)(0.08 m)2 = 4.02103 A m2 ; = ^ . n (a) For the torque, ^ = B = (9.65104 N m)^ + (7.24104 N m)^ + (8.08104 N m)k. i j (b) For the magnetic potential energy, U = B = [(0.60)(0.25 T)] = 0.603103 J. 129
E357 = iA = i(a2 + b2 /2) = i(a2 + b2 )/2. E358 If the distance to P is very large compared to a or b we can write the Law of Biot and Savart as 0 i s r B= . 4 r3 s is perpendicular to r for the left and right sides, so the left side contributes B1 = and the right side contributes B3 =  0 i b . 4 (x  a/2)2 0 i b , 4 (x + a/2)2
The top and bottom sides each contribute an equal amount B2 = B4 = 0 i a sin 0 i a(b/2) . 4 x2 + b2 /4 4 x3
Add the four terms, expand the denominators, and keep only terms in x3 , B= 0 i ab 0 = . 3 4 x 4 x3
The negative sign indicates that it is into the page. E359 (a) The electric field at this distance from the proton is E= 1 4(8.851012 C2 /N m2 ) (1.601019 C) = 5.141011 N/C. (5.291011 m)2
(b) The magnetic field at this from the proton is given by the dipole approximation, B(z) = = = 0 , 2z 3 (4107 N/A2 )(1.411026 A/m2 ) , 2(5.291011 m)3 1.90102 T
E3510 1.50 g of water has (2)(6.02 1023 )(1.5)/(18) = 1.00 1023 hydrogen nuclei. If all are aligned the net magnetic moment would be = (1.001023 )(1.411026 J/T) = 1.41103 J/T. The field strength is then B= 0 (1.41103 J/T) = (1.00107 N/A2 ) = 9.31013 T. 4 x3 (5.33 m)3
E3511 (a) There is effectively a current of i = f q = q/2. The dipole moment is then = iA = (q/2)(r2 ) = 1 qr2 . 2 (b) The rotational inertia of the ring is mr2 so L = I = mr2 . Then (1/2)qr2 q = = . L mr2 2m 130
E3512 The mass of the bar is m = V = (7.87 g/cm )(4.86 cm)(1.31 cm2 ) = 50.1 g. The number of atoms in the bar is N = (6.021023 )(50.1 g)/(55.8 g) = 5.411023 . The dipole moment of the bar is then = (5.411023 )(2.22)(9.271024 J/T) = 11.6 J/T. (b) The torque on the magnet is = (11.6 J/T)(1.53 T) = 17.7 N m. E3513 The magnetic dipole moment is given by = M V , Eq. 3513. Then = (5, 300 A/m)(0.048 m)(0.0055 m)2 = 0.024 A m2 . E3514 (a) The original field is B0 = 0 in. The field will increase to B = m B0 , so the increase is B = (1  1)0 in = (3.3104 )(4107 N/A2 )(1.3 A)(1600/m) = 8.6107 T. (b) M = (1  1)B0 /0 = (1  1)in = (3.3104 )(1.3 A)(1600/m) = 0.69 A/m. E3515 The energy to flip the dipoles is given by U = 2B. The temperature is then T = 2B 4(1.21023 J/T)(0.5 T) = = 0.58 K. 3k/2 3(1.381023 J/K)
3
E3516 The Curie temperature of iron is 770 C, which is 750 C higher than the surface temperature. This occurs at a depth of (750 C)/(30 C /km) = 25 km. E3517 (a) Look at the figure. At 50% (which is 0.5 on the vertical axis), the curve is at B0 /T 0.55 T/K. Since T = 300 K, we have B0 165 T. (b) Same figure, but now look at the 90% mark. B0 /T 1.60 T/K, so B0 480 T. (c) Good question. I think both fields are far beyond our current abilities. E3518 (a) Look at the figure. At 50% (which is 0.5 on the vertical axis), the curve is at B0 /T 0.55 T/K. Since B0 = 1.8 T, we have T (1.8 T)/(0.55 T/K) = 3.3 K. (b) Same figure, but now look at the 90% mark. B0 /T 1.60 T/K, so T (1.8 T)/(1.60 T/K) = 1.1 K. E3519 Since (0.5 T)/(10 K) = 0.05 T/K, and all higher temperatures have lower values of the ratio, and this puts all points in the region near where Curie's Law (the straight line) is valid, then the answer is yes. E3520 Using Eq. 3519, n = Mr M (108g/mol)(511103 A/m) VM = = = 8.741021 A/m2 N A (10490 kg/m3 )(6.021023 /mol)
131
E3521 (a) B = 0 /2z 3 , so B= (4107 N/A2 )(1.51023 J/T) = 9.4106 T. 2(10109 m)3
(b) U = 2B = 2(1.51023 J/T)(9.4106 T) = 2.821028 J. E3522 B = (43106 T)(295, 000106 m2 ) = 1.3107 Wb. E3523 (a) We'll assume, however, that all of the iron atoms are perfectly aligned. Then the dipole moment of the earth will be related to the dipole moment of one atom by Earth = N Fe , where N is the number of iron atoms in the magnetized sphere. If mA is the relative atomic mass of iron, then the total mass is N mA mA Earth m= = , A A Fe where A is Avogadro's number. Next, the volume of a sphere of mass m is m mA Earth V = = , A Fe where is the density. And finally, the radius of a sphere with this volume would be r= 3V 4
1/3
=
3Earth mA 4Fe A
1/3
.
Now we find the radius by substituting in the known values, r= 3(8.01022 J/T)(56 g/mol) 4(14106 g/m )(2.11023 J/T)(6.01023 /mol)
3 1/3
= 1.8105 m.
(b) The fractional volume is the cube of the fractional radius, so the answer is (1.8105 m/6.4106 )3 = 2.2105 . E3524 (a) At magnetic equator Lm = 0, so B= 0 (1.00107 N/A2 )(8.01022 J/T) = = 31T. 4r3 (6.37106 m)3
There is no vertical component, so the inclination is zero. (b) Here Lm = 60 , so B= 0 4r3 1 + 3 sin2 Lm = (1.00107 N/A2 )(8.01022 J/T) (6.37106 m)3 1 + 3 sin2 (60 ) = 56T.
The inclination is given by arctan(B v /B h ) = arctan(2 tan Lm ) = 74 . (c) At magnetic north pole Lm = 90 , so B= 0 2(1.00107 N/A2 )(8.01022 J/T) = = 62T. 3 2r (6.37106 m)3
There is no horizontal component, so the inclination is 90 . 132
E3525 This problem is effectively solving 1/r3 = 1/2 for r measured in Earth radii. Then r = 1.26rE , and the altitude above the Earth is (0.26)(6.37106 m) = 1.66106 m. E3526 The radial distance from the center is r = (6.37106 m)  (2900103 m) = 3.47106 m. The field strength is B= 0 2(1.00107 N/A2 )(8.01022 J/T) = = 380T. 3 2r (3.47106 m)3
E3527 Here Lm = 90  11.5 = 78.5 , so B= 0 4r3 1 + 3 sin2 Lm = (1.00107 N/A2 )(8.01022 J/T) (6.37106 m)3 1 + 3 sin2 (78.5 ) = 61T.
The inclination is given by arctan(B v /B h ) = arctan(2 tan Lm ) = 84 . E3528 The flux out the "other" end is (1.6103 T)(0.13 m)2 = 85Wb. The net flux through the surface is zero, so the flux through the curved surface is 0  (85Wb)  (25Wb) = 60Wb.. The negative indicates inward. E3529 The total magnetic flux through a closed surface is zero. There is inward flux on faces one, three, and five for a total of 9 Wb. There is outward flux on faces two and four for a total of +6 Wb. The difference is +3 Wb; consequently the outward flux on the sixth face must be +3 Wb. E3530 The stable arrangements are (a) and (c). The torque in each case is zero. E3531 The field on the x axis between the wires is B= 0 i 2 1 1 + 2r + x 2r  x .
Since B dA = 0, we can assume the flux through the curved surface is equal to the flux through the xz plane within the cylinder. This flux is
r
B
= L
r
0 i 2 0 i = L ln 3. = L
0 i 1 1 + 2 2r + x 2r  x 3r r ln  ln , r 3r
dx,
P351 We can imagine the rotating disk as being composed of a number of rotating rings of radius r, width dr, and circumference 2r. The surface charge density on the disk is = q/R2 , and consequently the (differential) charge on any ring is dq = (2r)(dr) = 2qr dr R2
The rings "rotate" with angular frequency , or period T = 2/. The effective (differential) current for each ring is then dq qr di = = dr. T R2 133
Each ring contributes to the magnetic moment, and we can glue all of this together as = = = = d, r2 di, qr3 dr, R2 0 qR2 . 4
R
P352 (a) The sphere can be sliced into disks. The disks can be sliced into rings. Each ring has some charge qi , radius ri , and mass mi ; the period of rotation for a ring is T = 2/, so the current in the ring is qi /T = qi /2. The magnetic moment is
2 2 i = (qi /2)ri = qi ri /2. 2 Note that this is closely related to the expression for angular momentum of a ring: li = mi ri . Equating, i = qi li /2mi .
If both mass density and charge density are uniform then we can write qi /mi = q/m, = d = (q/2m) dl = qL/2m
For a solid sphere L = I = 2mR2 /5, so = qR2 /5. (b) See part (a) P353 (a) The orbital speed is given by K = mv 2 /2. The orbital radius is given by mv = qBr, or r = mv/qB. The frequency of revolution is f = v/2r. The effective current is i = qf . Combining all of the above to find the dipole moment, = iA = q v vr mv 2 K r2 = q =q = . 2r 2 2qB B
(b) Since q and m cancel out of the above expression the answer is the same! (c) Work it out: M= (5.281021 /m3 )(6.211020 J) (5.281021 /m3 )(7.581021 J) = + = 312 A/m. V (1.18 T) (1.18 T)
P354 (b) Point the thumb or your right hand to the right. Your fingers curl in the direction of the current in the wire loop. (c) In the vicinity of the wire of the loop B has a component which is directed radially outward. Then B ds has a component directed to the left. Hence, the net force is directed to the left. P355 (b) Point the thumb or your right hand to the left. Your fingers curl in the direction of the current in the wire loop. (c) In the vicinity of the wire of the loop B has a component which is directed radially outward. Then B ds has a component directed to the right. Hence, the net force is directed to the right. 134
P356 (a) Let x = B/kT . Adopt the convention that N+ refers to the atoms which have parallel alignment and N those which are antiparallel. Then N+ + N = N , so N+ = N ex /(ex + ex ), and N = N ex /(ex + ex ), Note that the denominators are necessary so that N+ + N = N . Finally, M = (N+  N ) = N (b) If B ex  ex . ex + ex
kT then x is very small and ex 1 x. The above expression reduces to M = N (1 + x)  (1  x) 2 B = N x = . (1 + x) + (1  x) kT
(c) If B to
kT then x is very large and ex while ex 0. The above expression reduces N = N.
P357
(a) Centripetal acceleration is given by a = r 2 . Then a  a0
2 = r(0 + )2  r0 , = 2r0 + r(0 )2 , 2r0 .
(b) The change in centripetal acceleration is caused by the additional magnetic force, which has magnitude FB = qvB = erB. Then = a  a0 eB = . 2r0 2m
Note that we boldly canceled against 0 in this last expression; we are assuming that is small, and for these problems it is. P358 (a) i = /A = (8.01022 J/T)/(6.37106 m)2 = 6.3108 A. (b) Far enough away both fields act like perfect dipoles, and can then cancel. (c) Close enough neither field acts like a perfect dipole and the fields will not cancel. P359 (a) B = B h 2 + B v 2 , so B= 0 4r3 cos2 Lm + 4 sin2 Lm = 0 4r3 1 + 3 sin2 Lm .
(b) tan i = B v /B h = 2 sin Lm / cos Lm = 2 tan Lm .
135
E361
The important relationship is Eq. 364, written as B = (5.0 mA)(8.0 mH) iL = = 1.0107 Wb N (400)
E362 (a) = (34)(2.62103 T)(0.103 m)2 = 2.97103 Wb. (b) L = /i = (2.97103 Wb)/(3.77 A) = 7.88104 H. E363 n = 1/d, where d is the diameter of the wire. Then 0 A (4107 H/m)(/4)(4.10102 m)2 L = 0 n2 A = 2 = = 2.61104 H/m. l d (2.52103 m)2 E364 (a) The emf supports the current, so the current must be decreasing. (b) L = E/(di/dt) = (17 V)/(25103 A/s) = 6.8104 H. E365 (a) Eq. 361 can be used to find the inductance of the coil. L= EL (3.0 mV) = = 6.0104 H. di/dt (5.0 A/s)
(b) Eq. 364 can then be used to find the number of turns in the coil. N= iL (8.0 A)(6.0104 H) = = 120 B (40Wb)
E366 Use the equation between Eqs. 369 and 3610. B = = (4107 H/m)(0.81 A)(536)(5.2102 m) (5.2102 m) + (15.3102 m) ln , 2 (15.3102 m) 1.32106 Wb.
E367 L = m 0 n2 Al = m 0 N 2 A/l, or L = (968)(4107 H/m)(1870)2 (/4)(5.45102 m)2 /(1.26 m) = 7.88 H. E368 In each case apply E = Li/t. (a) E = (4.6 H)(7 A)/(2103 s) = 1.6104 V. (b) E = (4.6 H)(2 A)/(3103 s) = 3.1103 V. (c) E = (4.6 H)(5 A)/(1103 s) = 2.3104 V. E369 (a) If two inductors are connected in parallel then the current through each inductor will add to the total current through the circuit, i = i1 + i2 , Take the derivative of the current with respect to time and then di/dt = di1 /dt + di2 /dt, The potential difference across each inductor is the same, so if we divide by E and apply we get di/dt di1 /dt di2 /dt = + , E E E But di/dt 1 = , E L 136
so the previous expression can also be written as 1 1 1 = + . Leq L1 L2 (b) If the inductors are close enough together then the magnetic field from one coil will induce currents in the other coil. Then we will need to consider mutual induction effects, but that is a topic not covered in this text. E3610 (a) If two inductors are connected in series then the emf across each inductor will add to the total emf across both, E = E1 + E2 , Then the current through each inductor is the same, so if we divide by di/dt and apply we get E1 E2 E = + , di/dt di/dt di/dt But E = L, di/dt
so the previous expression can also be written as Leq = L1 + L2 . (b) If the inductors are close enough together then the magnetic field from one coil will induce currents in the other coil. Then we will need to consider mutual induction effects, but that is a topic not covered in this text. E3611 Use Eq. 3617, but rearrange: L = t (1.50 s) = = 0.317 s. ln[i0 /i] ln[(1.16 A)/(10.2103 A)]
Then R = L/L = (9.44 H)/(0.317 s) = 29.8 . E3612 (a) There is no current through the resistor, so ER = 0 and then EL = E. (b) EL = Ee2 = (0.135)E. (c) n =  ln(EL /E) = ln(1/2) = 0.693. E3613 (a) From Eq. 364 we find the inductance to be L= N B (26.2103 Wb) = = 4.78103 H. i (5.48 A)
Note that B is the flux, while the quantity N B is the number of flux linkages. (b) We can find the time constant from Eq. 3614, L = L/R = (4.78103 H)/(0.745 ) = 6.42103 s. The we can invert Eq. 3613 to get t = L ln 1  Ri(t) E , (0.745 A)(2.53 A) (6.00 V) 137 = 2.42103 s.
= (6.42103 s) ln 1 
E3614 (a) Rearrange: E E i R R dt L (b) Integrate:
t
= iR + L = =
di , dt
L di , R dt di . E/R  i
i

0
R dt L R  t L
= =
di , i  E/R 0 i + E/R ln , E/R
E t/L e R E 1  et/L R E3615 di/dt = (5.0 A/s). Then E = iR + L
= i + E/R, = i.
di = (3.0 A)(4.0 ) + (5.0 A/s)t(4.0 ) + (6.0 H)(5.0 A/s) = 42 V + (20 V/s)t. dt
E3616 (1/3) = (1  et/L ), so L =  E3617 (5.22 s) t = = 12.9 s. ln(2/3) ln(2/3)
We want to take the derivative of the current in Eq. 3613 with respect to time, di E 1 t/L E = e = et/L . dt R L L
Then L = (5.0102 H)/(180 ) = 2.78104 s. Using this we find the rate of change in the current when t = 1.2 ms to be
3 4 di (45 V) = e(1.210 s)/(2.7810 s) = 12 A/s. 2 H) dt ((5.010
E3618 (b) Consider some time ti : EL (ti ) = Eeti /L . Taking a ratio for two different times, EL (t1 ) = e(t2 t1 )/L , EL (t2 ) or L = t2  t1 (2 ms)  (1 ms) = = 3.58 ms ln[EL (t1 )/EL (t2 )] ln[(18.24 V)/(13.8 V)] E = EL et/L = (18.24 V)e(1 ms)/(3.58 ms) = 24 V. 138
(a) Choose any time, and
E3619 (a) When the switch is just closed there is no current through the inductor. So i1 = i2 is given by E (100 V) i1 = = = 3.33 A. R1 + R2 (10 ) + (20 ) (b) A long time later there is current through the inductor, but it is as if the inductor has no effect on the circuit. Then the effective resistance of the circuit is found by first finding the equivalent resistance of the parallel part 1/(30 ) + 1/(20 ) = 1/(12 ), and then finding the equivalent resistance of the circuit (10 ) + (12 ) = 22 . Finally, i1 = (100 V)/(22 ) = 4.55 A and V2 = (100 V)  (4.55 A)(10 ) = 54.5 V; consequently, i2 = (54.5 V)/(20 ) = 2.73 A. It didn't ask, but i2 = (4.55 A)  (2.73 A) = 1.82 A. (c) After the switch is just opened the current through the battery stops, while that through the inductor continues on. Then i2 = i3 = 1.82 A. (d) All go to zero. E3620 (a) For toroids L = 0 N 2 h ln(b/a)/2. The number of turns is limited by the inner radius: N d = 2a. In this case, N = 2(0.10 m)/(0.00096 m) = 654. The inductance is then L= (4107 H/m)(654)2 (0.02 m) (0.12 m) ln = 3.1104 H. 2 (0.10 m)
(b) Each turn has a length of 4(0.02 m) = 0.08 m. The resistance is then R = N (0.08 m)(0.021 /m) = 1.10 The time constant is L = L/R = (3.1104 H)/(1.10 ) = 2.8104 s. E3621 (I) When the switch is just closed there is no current through the inductor or R2 , so the potential difference across the inductor must be 10 V. The potential difference across R1 is always 10 V when the switch is closed, regardless of the amount of time elapsed since closing. (a) i1 = (10 V)/(5.0 ) = 2.0 A. (b) Zero; read the above paragraph. (c) The current through the switch is the sum of the above two currents, or 2.0 A. (d) Zero, since the current through R2 is zero. (e) 10 V, since the potential across R2 is zero. (f) Look at the results of Exercise 3617. When t = 0 the rate of change of the current is di/dt = E/L. Then di/dt = (10 V)/(5.0 H) = 2.0 A/s. (II) After the switch has been closed for a long period of time the currents are stable and the inductor no longer has an effect on the circuit. Then the circuit is a simple two resistor parallel network, each resistor has a potential difference of 10 V across it. 139
(a) Still 2.0 A; nothing has changed. (b) i2 = (10 V)/(10 ) = 1.0 A. (c) Add the two currents and the current through the switch will be 3.0 A. (d) 10 V; see the above discussion. (e) Zero, since the current is no longer changing. (f) Zero, since the current is no longer changing. E3622 U = (71 J/m3 )(0.022 m3 ) = 1.56 J. Then using U = i2 L/2 we get i= 2U/L = 2(1.56 J)/(0.092 H) = 5.8 A.
E3623 (a) L = 2U/i2 = 2(0.0253 J)/(0.062 A)2 = 13.2 H. (b) Since the current is squared in the energy expression, doubling the current would quadruple the energy. Then i = 2i0 = 2(0.062 A) = 0.124 A. E3624 (a) B = 0 in and u = B 2 /20 , or u = 0 i2 n2 /2 = (4107 N/A2 )(6.57 A)2 (950/0.853 m)2 /2 = 33.6 J/m3 . (b) U = uAL = (33.6 J/m3 )(17.2104 m2 )(0.853 m) = 4.93102 J. E3625 uB = B 2 /20 , and from Sample Problem 332 we know B, hence uB = E3626 (a) uB = B 2 /20 , so uB = (1001012 T)2 1 3 = 2.5102 eV/cm . 2(4107 N/A2 ) (1.61019 J/eV) (12.6 T)2 = 6.32107 J/m3 . 2(4107 N/A2 )
(b) x = (10)(9.461015 m) = 9.461016 m. Using the results from part (a) expressed in J/m3 we find the energy contained is U = (3.981015 J/m3 )(9.461016 m)3 = 3.41036 J E3627 The energy density of an electric field is given by Eq. 3623; that of a magnetic field is given by Eq. 3622. Equating,
0
2
E2 E
= =
1 2 B , 20 B . 0 0
The answer is then E = (0.50 T)/ (8.851012 C2 /N m2 )(4107 N/A2 ) = 1.5108 V/m. E3628 The rate of internal energy increase in the resistor is given by P = iVR . The rate of energy storage in the inductor is dU/dt = Li di/dt = iVL . Since the current is the same through both we want to find the time when VR = VL . Using Eq. 3615 we find 1  et/L = et/L , ln 2 = t/L , so t = (37.5 ms) ln 2 = 26.0 ms. 140
E3629 (a) Start with Eq. 3613: i iR 1 E L = E(1  et/L )/R, = et/L , = = = t , ln(1  iR/E) (5.20103 s) , ln[1  (1.96103 A)(10.4103 )/(55.0 V)] 1.12102 s.
Then L = L R = (1.12102 s)(10.4103 ) = 116 H. (b) U = (1/2)(116 H)(1.96103 A)2 = 2.23104 J. E3630 (a) U = Eq; q = idt. U = E = = Using the numbers provided, L = (5.48 H)/(7.34 ) = 0.7466 s. Then U= (12.2 V)2 (2 s) + (0.7466 s)(e(2 s)/0.7466 s)  1) = 26.4 J (7.34 ) E 1  et/L dt, R
2 E2 t + L et/L , R 0 E2 E 2 L t/L t + 2 (e  1). R R
(b) The energy stored in the inductor is UL = Li2 /2, or UL = = (c) UR = U  UL = 19.8 J. E3631 This shell has a volume of V = 4 (RE + a)3  RE 3 . 3 LE 2 2R2 6.57 J. 1  et/L
2
dt,
Since a << RE we can expand the polynomials but keep only the terms which are linear in a. Then V 4RE 2 a = 4(6.37106 m)2 (1.6104 m) = 8.21018 m3 . The magnetic energy density is found from Eq. 3622, uB = 1 2 (60106 T)2 B = = 1.43103 J/m3 . 20 2(4107 N/A2 )
The total energy is then (1.43103 J/m3 )(8.2eex18m3 ) = 1.21016 J. 141
E3632 (a) B = 0 i/2r and uB = B 2 /20 = 0 i2 /8 2 r2 , or uB = (4107 H/m)(10 A)2 /8 2 (1.25103 m)2 = 1.0 J/m3 . (b) E = V /l = iR/l and uE =
0E 2
/2 =
0i
2
(R/l)2 /2. Then
uE = (8.851012 F/m)(10 A)2 (3.3103 /m)2 /2 = 4.81015 J/m3 . E3633 i = 2U/L = 2(11.2106 J)/(1.48103 H) = 0.123 A.
E3634 C = q 2 /2U = (1.63106 C)2 /2(142106 J) = 9.36109 F. E3635 1/2f = LC so L = 1/4 2 f 2 C, or L = 1/4 2 (10103 Hz)2 (6.7106 F) = 3.8105 H. E3636 qmax 2 /2C = Limax 2 /2, or imax = qmax / LC = (2.94106 C)/ (1.13103 H)(3.88106 F) = 4.44102 A. E3637 Closing a switch has the effect of "shorting" out the relevant circuit element, which effectively removes it from the circuit. If S1 is closed we have C = RC or C = C /R, if instead S2 is closed we have L = L/R or L = RL , but if instead S3 is closed we have a LC circuit which will oscillate with period 2 T = = 2 LC. Substituting from the expressions above, T = 2 = 2 L C .
E3638 The capacitors can be used individually, or in series, or in parallel. The four possible capacitances are then 2.00F, 5.00F, 2.00F + 5.00F = 7.00F, and (2.00F )(5.00F)(2.00F + 5.00F) = 1.43F. The possible resonant frequencies are then 1 2 1 2 1 2 1 2 1 2 1 LC = f, = 1330 Hz,
1 (10.0 mH)(1.43F ) 1 (10.0 mH)(2.00F ) 1 (10.0 mH)(5.00F ) 1 (10.0 mH)(7.00F )
=
1130 Hz,
=
712 Hz,
=
602 Hz.
142
E3639 (a) k = (8.13 N)/(0.0021 m) = 3.87103 N/m. = k/m = 89.3 rad/s. (b) T = 2/ = 2/(89.3 rad/s) = 7.03102 s. (c) LC = 1/ 2 , so C = 1/(89.3 rad/s)2 (5.20 H) = 2.41105 F.
(3870 N/m)/(0.485 kg) =
E3640 The period of oscillation is T = 2 LC = 2 (52.2mH)(4.21F) = 2.95 ms. It requires onequarter period for the capacitor to charge, or 0.736 ms. E3641 (a) An LC circuit oscillates so that the energy is converted from all magnetic to all electrical twice each cycle. It occurs twice because once the energy is magnetic with the current flowing in one direction through the inductor, and later the energy is magnetic with the current flowing the other direction through the inductor. The period is then four times 1.52s, or 6.08s. (b) The frequency is the reciprocal of the period, or 164000 Hz. (c) Since it occurs twice during each oscillation it is equal to half a period, or 3.04s. E3642 (a) q = CV = (1.13109 F)(2.87 V) = 3.24109 C. (c) U = q 2 /2C = (3.24109 C)2 /2(1.13109 F) = 4.64109 J. (b) i = 2U/L = 2(4.64109 J)/(3.17103 H) = 1.71103 A. E3643 (a) im = q m and q m = CV m . Multiplying the second expression by L we get Lq m = V m / 2 . Combining, Lim = V m . Then f= (50 V) = = 6.1103 /s. 2 2(0.042 H)(0.031 A)
(b) See (a) above. (c) C = 1/ 2 L = 1/(26.1103 /s)2 (0.042 H) = 1.6108 F. E3644 (a) f = 1/2 LC = 1/2 (6.2106 F)(54103 H) = 275 Hz. (b) Note that from Eq. 3632 we can deduce imax = qmax . The capacitor starts with a charge q = CV = (6.2106 F)(34 V) = 2.11104 C. Then the current amplitude is imax = qmax / LC = (2.11104 C)/ (6.2106 F)(54103 H) = 0.365 A. E3645 (a) = 1/ LC = 1/ (10106 F)(3.0103 H) = 5800 rad/s. (b) T = 2/ = 2/(5800 rad/s) = 1.1103 s. E3646 f = (2105 Hz)(1 + /180 ). C = 4 2 /f 2 L, so C= 4 2 (9.9107 F) = . (2105 Hz)2 (1 + /180 )2 (1 mH) (1 + /180 )2
2 E3647 (a) UE = UB /2 and UE + UB = U , so 3UE = U , or 3(q 2 /2C) = qmax /2C, so q = qmax / 3. (b) Solve q = qmax cos t, or t= T arccos 1/ 3 = 0.152T. 2
143
E3648 (a) Add the contribution from the inductor and the capacitor, U= (b) q m = (c) im = (3.83106 C)2 (24.8103 H)(9.16103 A)2 + = 1.99106 J. 2 2(7.73106 F)
2(7.73106 F)(1.99106 J) = 5.55106 C. 2(1.99106 J)/(24.8103 H) = 1.27102 A.
E3649 (a) The frequency of such a system is given by Eq. 3626, f = 1/2 LC. Note that maximum frequency occurs with minimum capacitance. Then f1 = f2 C2 = C1 (365 pF) = 6.04. (10 pF)
(b) The desired ratio is 1.60/0.54 = 2.96 Adding a capacitor in parallel will result in an effective capacitance given by C 1,eff = C1 + C add , with a similar expression for C2 . We want to choose C add so that f1 = f2 Solving, C 2,eff C2 + C add C add = C 1,eff (2.96)2 , = (C1 + C add )8.76, C2  8.76C1 = , 7.76 (365 pF)  8.76(10 pF) = = 36 pF. 7.76 1 4 2 (0.54106 Hz)2 (4011012 F) C 2,eff = 2.96. C 1,eff
The necessary inductance is then L= 1 4 2 f 2 C = = 2.2104 H.
E3650 The key here is that UE = C(V )2 /2. We want to charge a capacitor with oneninth the capacitance to have three times the potential difference. Since 32 = 9, it is reasonable to assume that we want to take all of the energy from the first capacitor and give it to the second. Closing S1 and S2 will not work, because the energy will be shared. Instead, close S2 until the capacitor has completely discharged into the inductor, then simultaneously open S2 while closing S1 . The inductor will then discharge into the second capacitor. Open S1 when it is "full". E3651 (a) = 1/ LC. qm = im = (2.0 A) (3.0103 H)(2.7106 F) = 1.80104 C
(b) dUC /dt = qi/C. Since q = q m sin t and i = im cos t then dUC /dt is a maximum when sin t cos t is a maximum, or when sin 2t is a maximum. This happens when 2t = /2, or t = T /8. (c) dUC /dt = q m im /2C, or dUC /dt = (1.80104 C)(2.0 A)/2(2.7106 F) = 67 W. 144
E3652 After only complete cycles q = qmax eRt/2L . Not only that, but t = N , where = 2/ . Finally, = (1/LC)  (R/2L)2 . Since the first term under the square root is so much larger than the second, we can ignore the effect of damping on the frequency, and simply use = 1/ LC. Then q = qmax eN R /2L = qmax eN R LC/L = qmax eN R C/L . Finally, R C/L = (7.22 ) (3.18 F)/(12.3 H) = 1.15102 . Then N =5 N =5 N =5 : : : q = (6.31C)e5(0.0115) = 5.96C, q = (6.31C)e10(0.0115) = 5.62C, q = (6.31C)e100(0.0115) = 1.99C.
E3653 Use Eq. 3640, and since U q 2 , we want to solve eRt/L = 1/2, then t= L ln 2. R
E3654 Start by assuming that the presence of the resistance does not significantly change the frequency. Then = 1/ LC, q = qmax eRt/2L , t = N , and = 2/. Combining, q = qmax eN R /2L = qmax eN R LC/L = qmax eN R C/L . Then R= L/C ln(q/qmax ) =  N (220mH)/(12F) ln(0.99) = 8700 . (50)
It remains to be verified that 1/LC E3655 be
(R/2L)2 .
The damped (angular) frequency is given by Eq. 3641; the fractional change would then 1  (R2 C/4L).
 = 1  1  (R/2L)2 = 1  Setting this equal to 0.01% and then solving for R, R= 4L (1  (1  0.0001)2 ) = C
4(12.6103 H) (1.9999104 ) = 2.96 . (1.15106 F)
P361
The inductance of a toroid is L= 0 N 2 h b ln . 2 a
If the toroid is very large and thin then we can write b = a + , where << a. The natural log then can be approximated as b ln = ln 1 + . a a a The product of and h is the cross sectional area of the toroid, while 2a is the circumference, which we will call l. The inductance of the toroid then reduces to L 0 N 2 A 0 N 2 = . 2 a l
But N is the number of turns, which can also be written as N = nl, where n is the turns per unit length. Substitute this in and we arrive at Eq. 367. 145
P362 (a) Since ni is the net current per unit length and is this case i/W , we can simply write B = 0 i/W . (b) There is only one loop of wire, so L = B /i = BA/i = 0 iR2 /W i = 0 R2 /W. P363 Choose the y axis so that it is parallel to the wires and directly between them. The field in the plane between the wires is B= The flux per length l of the wires is
d/2a
0 i 2
1 1 + d/2 + x d/2  x
.
B
= l
d/2+a
B dx = l
0 i 2
d/2a d/2+a
1 1 + d/2 + x d/2  x
dx,
= = The inductance is then
2l
0 i d/2a 1 2 d/2+a d/2 + x 0 i d  a 2l ln . 2 a L=
dx,
B 0 l d  a = ln . i a
P364 (a) Choose the y axis so that it is parallel to the wires and directly between them. The field in the plane between the wires is B= 0 i 2 1 1 + d/2 + x d/2  x .
The flux per length l between the wires is
d/2a
1
=
d/2+a
B dx = 2
0 i 2
d/2a d/2+a
1 1 + d/2 + x d/2  x
dx,
= =
0 i d/2a 1 2 d/2+a d/2 + x 0 i d  a 2 ln . 2 a
dx,
The field in the plane inside one of the wires, but still between the centers is B= The additional flux is then
d/2
0 i 2
1 d/2  x + d/2 + x a2
.
2
= =
2
d/2a
B dx = 2 0 i 2 ln
0 i 2 .
d/2 d/2a
1 d/2  x + d/2 + x a2
dx,
2
d 1 + da 2
146
The flux per meter between the axes of the wire is the sum, or B = = = 0 i d 1 ln + , a 2 (4107 H/m)(11.3 A) 1.5105 Wb/m.
ln
(21.8, mm) 1 + (1.3 mm) 2
,
(b) The fraction f inside the wires is f = = = d 1 d 1 + / ln + , da 2 a 2 (21.8, mm) 1 + / (21.8, mm)  (1.3 mm) 2 0.09. ln
(21.8, mm) 1 + (1.3 mm) 2
,
(c) The net flux is zero for parallel currents. P365 The magnetic field in the region between the conductors of a coaxial cable is given by B= 0 i , 2r
so the flux through an area of length l, width b  a, and perpendicular to B is B = = = B dA =
b l
B dA,
0 i dz dr, a 0 2r 0 il b ln . 2 a
We evaluated this integral is cylindrical coordinates: dA = (dr)(dz). As you have been warned so many times before, learn these differentials! The inductance is then 0 l b B = ln . L= i 2 a P366 (a) So long as the fuse is not blown there is effectively no resistance in the circuit. Then the equation for the current is E = L di/dt, but since E is constant, this has a solution i = Et/L. The fuse blows when t = imax L/E = (3.0 A)(5.0 H)/(10 V) = 1.5 s. (b) Note that once the fuse blows the maximum steady state current is 2/3 A, so there must be an exponential approach to that current. P367 The initial rate of increase is di/dt = E/L. Since the steady state current is E/R, the current will reach the steady state value in a time given by E/R = i = Et/L, or t = L/R. But that's L .
1 P368 (a) U = 2 Li2 = (152 H)(32 A)2 /2 = 7.8104 J. (b) If the coil develops at finite resistance then all of the energy in the field will be dissipated as heat. The mass of Helium that will boil off is
m = Q/Lv = (7.8104 J)/(85 J/mol)/(4.00g/mol) = 3.7 kg. 147
P369
(a) B = (0 N i)/(2r), so u= B2 0 N 2 i2 = . 20 8 2 r2
(b) U =
u dV =
urdr d dz. The field inside the toroid is uniform in z and , so U = 2h = 0 N 2 i2 r dr, 8 2 r2 a h0 N 2 i2 b ln . 4 a
b
(c) The answers are the same! P3610 The energy in the inductor is originally U = Li2 /2. The internal energy in the resistor 0 increases at a rate P = i2 R. Then
P dt = R
0 0
i2 e2t/L dt = 0
Li2 Ri2 L 0 = 0. 2 2
P3611 density is
(a) In Chapter 33 we found the magnetic field inside a wire carrying a uniform current B= 0 ir . 2R2
The magnetic energy density in this wire is uB = 1 2 0 i2 r2 B = . 20 8 2 R4
We want to integrate in cylindrical coordinates over the volume of the wire. Then the volume element is dV = (dr)(r d)(dz), so UB = =
0 0
uB dV,
R l 2 0 R 0
0 i2 r2 d dz rdr, 8 2 R4
= = (b) Solve
0 i2 l 4R4 0 i2 l . 16
r3 dr,
UB = for L, and L= P3612
L 2 i 2
2UB 0 l = . 2 i 8
1/C = 1/C1 + 1/C2 and L = L1 + L2 . Then 1 = LC = (L1 + L2 ) C1 C2 = C1 + C2 148
2 2 C2 /0 + C1 /0 1 = . C1 + C2 0
P3613
(a) There is no current in the middle inductor; the loop equation becomes L d2 q q d2 q q + +L 2 + = 0. dt2 C dt C
Try q = q m cos t as a solution: L 2 + 1 1  L 2 + = 0; C C
which requires = 1/ LC. (b) Look at only the left hand loop; the loop equation becomes L Try q = q m cos t as a solution: L 2 + which requires = 1/ 3LC. P3614 q d2 q d2 q + + 2L 2 = 0. 2 dt C dt 1  2L 2 = 0; C
(b) (  )/ is the fractional shift; this can also be written as 1 = = = 1  (LC)(R/2L)2  1, 1  R2 C/4L  1, 1 (100 )2 (7.3106 F)  1 = 2.1103 . 4(4.4 H)
P3615
We start by focusing on the charge on the capacitor, given by Eq. 3640 as q = q m eRt/2L cos( t + ).
After one oscillation the cosine term has returned to the original value but the exponential term has attenuated the charge on the capacitor according to q = q m eRT /2L , where T is the period. The fractional energy loss on the capacitor is then U0  U q2 = 1  2 = 1  eRT /L . U0 qm For small enough damping we can expand the exponent. Not only that, but T = 2/, so U 2R/L. U
149
P3616
We are given 1/2 = et/2L when t = 2n/ . Then = 2n nR 2n = = . t 2(L/R) ln 2 L ln 2
From Eq. 3641, 2  2 (  )( + ) (  )2  = (R/2L)2 , = (R/2L)2 , (R/2L)2 , (R/2L)2 = , 2 2 2 (ln 2) = , 8 2 n2 0.0061 = . n2
150
E371
The frequency, f , is related to the angular frequency by = 2f = 2(60 Hz) = 377 rad/s
The current is alternating because that is what the generator is designed to produce. It does this through the configuration of the magnets and coils of wire. One complete turn of the generator will (could?) produce one "cycle"; hence, the generator is turning 60 times per second. Not only does this set the frequency, it also sets the emf, since the emf is proportional to the speed at which the coils move through the magnetic field. E372 (a) XL = L, so f = XL /2L = (1.28103 )/2(0.0452 H) = 4.51103 /s. (b) XC = 1/C, so C = 1/2f XC = 1/2(4.51103 /s)(1.28103 ) = 2.76108 F. (c) The inductive reactance doubles while the capacitive reactance is cut in half. E373 (a) XL = XC implies L = 1/C or = 1/ LC, so = 1/ (6.23103 H)(11.4106 F) = 3750 rad/s. (b) XL = L = (3750 rad/s)(6.23103 H) = 23.4 (c) See (a) above. E374 (a) im = E/XL = E/L, so im = (25.0 V)/(377 rad/s)(12.7 H) = 5.22103 A. (b) The current and emf are 90 out of phase. When the current is a maximum, E = 0. (c) t = arcsin[E(t)/E m ], so t = arcsin and i = (5.22103 A) cos(0.585) = 4.35103 A. (d) Taking energy. E375 (a) The reactance of the capacitor is from Eq. 3711, XC = 1/C. The AC generator from Exercise 4 has E = (25.0 V) sin(377 rad/s)t. So the reactance is XC = 1 1 = = 647 . C (377 rad/s)(4.1F) (13.8 V) = 0.585 rad. (25.0 V)
The maximum value of the current is found from Eq. 3713, im = (VC )max ) (25.0 V) = = 3.86102 A. XC (647 )
(b) The generator emf is 90 out of phase with the current, so when the current is a maximum the emf is zero. 151
(c) The emf is 13.8 V when t = arcsin (13.8 V) = 0.585 rad. (25.0 V)
The current leads the voltage by 90 = /2, so i = im sin(t  ) = (3.86102 A) sin(0.585  /2) = 3.22102 A. (d) Since both the current and the emf are negative the product is positive and the generator is supplying energy to the circuit. E376 R = (L  1/omegaC)/ tan and = 2f = 2(941/s) = 5910 rad/s , so R= E377 E378 (a) XL doesn't change, so XL = 87 . (b) XC = 1/C = 1/2(60/s)(70106 F) = 37.9. (c) Z = (160 )2 + (87  37.9 )2 = 167 . (d) im = (36 V)/(167 ) = 0.216 A. (e) tan = (87  37.9 )/(160 ) = 0.3069, so = arctan(0.3069) = 17 . E379 A circuit is considered inductive if XL > XC , this happens when im lags E m . If, on the other hand, XL < XC , and im leads E m , we refer to the circuit as capacitive. This is discussed on page 850, although it is slightly hidden in the text of column one. (a) At resonance, XL = XC . Since XL = L and XC = 1/C we expect that XL grows with increasing frequency, while XC decreases with increasing frequency. Consequently, at frequencies above the resonant frequency XL > XC and the circuit is predominantly inductive. But what does this really mean? It means that the inductor plays a major role in the current through the circuit while the capacitor plays a minor role. The more inductive a circuit is, the less significant any capacitance is on the behavior of the circuit. For frequencies below the resonant frequency the reverse is true. (b) Right at the resonant frequency the inductive effects are exactly canceled by the capacitive effects. The impedance is equal to the resistance, and it is (almost) as if neither the capacitor or inductor are even in the circuit. E3710 The net y component is XC  XL . The net x component is R. The magnitude of the resultant is Z = R2 + (XC  XL )2 , while the phase angle is tan = (XC  XL ) . R (5910 rad/s)(88.3103 H)  1/(5910 rad/s)(937109 F) = 91.5 . tan(75 )
E3711 Yes. At resonance = 1/ (1.2 H)(1.3106 F) = 800 rad/s and Z = R. Then im = E/Z = (10 V)/(9.6 ) = 1.04 A, so [VL ]m = im XL = (1.08 A)(800 rad/s)(1.2 H) = 1000 V. 152
E3712 (a) Let O = XL  XC and A = R, then H 2 = A2 + O2 = Z 2 , so sin = (XL  XC )/Z and cos = R/Z. E3713 (a) The voltage across the generator is the generator emf, so when it is a maximum from Sample Problem 373, it is 36 V. This corresponds to t = /2. (b) The current through the circuit is given by i = im sin(t  ). We found in Sample Problem 373 that im = 0.196 A and = 29.4 = 0.513 rad. For a resistive load we apply Eq. 373, VR = im R sin(t  ) = (0.196 A)(160) sin((/2)  (0.513)) = 27.3 V. (c) For a capacitive load we apply Eq. 3712, VC = im XC sin(t   /2) = (0.196 A)(177) sin((0.513)) = 17.0 V. (d) For an inductive load we apply Eq. 377, VL = im XL sin(t  + /2) = (0.196 A)(87) sin(  (0.513)) = 8.4 V. (e) (27.3 V) + (17.0 V) + (8.4 V) = 35.9 V. E3714 If circuit 1 and 2 have the same resonant frequency then L1 C1 = L2 C2 . The series combination for the inductors is L = L1 + L2 , The series combination for the capacitors is 1/C = 1/C1 + 1/C2 , so C1 C2 L1 C1 C2 + L2 C2 C1 = = L1 C1 , C1 + C2 C1 + C2 which is the same as both circuit 1 and 2. LC = (L1 + L2 ) E3715 (a) Z = (125 V)/(3.20 A) = 39.1 . (b) Let O = XL  XC and A = R, then H 2 = A2 + O2 = Z 2 , so cos = R/Z. Using this relation, R = (39.1 ) cos(56.3 ) = 21.7 . (c) If the current leads the emf then the circuit is capacitive. E3716 (a) Integrating over a single cycle, 1 T
T
sin2 t dt
0
= =
1 T 1 (1  cos 2t) dt, T 0 2 1 1 T = . 2T 2 1 T = 0. = 153
T 0
(b) Integrating over a single cycle, 1 T
T
sin t cos t dt
0
1 sin 2tdt, 2
E3717
The resistance would be given by Eq. 3732, R= P av (0.10)(746 W) = = 177 . 2 irms (0.650 A)2
This would not be the same as the direct current resistance of the coils of a stopped motor, because there would be no inductive effects. E3718 Since irms = E rms /Z, then P av = i2 rms R = E3719 (a) Z = E 2 rms R . Z2
(160 )2 + (177 )2 = 239 ; then P av = 1 (36 V)2 (160 ) = 1.82 W. 2 (239 )2
(b) Z =
(160 )2 + (87 )2 = 182 ; then P av = 1 (36 V)2 (160 ) = 3.13 W. 2 (182 )2
E3720 (a) Z = (12.2 )2 + (2.30 )2 = 12.4 (b) P av = (120 V)2 (12.2 )/(12.4 )2 = 1140 W. (c) irms = (120 V)/(12.4 ) = 9.67 A. E3721 The rms value of any sinusoidal quantity is related to the maximum value by 2 v rms = vmax . Since this factor of 2 appears in all of the expressions, we can conclude that if the rms values are equal then so are the maximum values. This means that (VR )max = (VC )max = (VL )max or im R = im XC = im XL or, with one last simplification, R = XL = XC . Focus on the right hand side of the last equality. If XC = XL then we have a resonance condition, and the impedance (see Eq. 3720) is a minimum, and is equal to R. Then, according to Eq. 3721, im = Em , R
which has the immediate consequence that the rms voltage across the resistor is the same as the rms voltage across the generator. So everything is 100 V. E3722 (a) The antenna is "intune" when the impedance is a minimum, or = 1/ LC. So f = /2 = 1/2 (8.22106 H)(0.2701012 F) = 1.07108 Hz.
(b) irms = (9.13 V)/(74.7 ) = 1.22107 A. (c) XC = 1/2f C, so VC = iXC = (1.22107 A)/2(1.07108 Hz)(0.270 1012 F) = 6.72104 V.
154
E3723 Assuming no inductors or capacitors in the circuit, then the circuit effectively behaves as a DC circuit. The current through the circuit is i = E/(r + R). The power delivered to R is then P = iV = i2 R = E 2 R/(r + R)2 . Evaluate dP/dR and set it equal to zero to find the maximum. Then rR dP = E 2R , 0= dR (r + R)3 which has the solution r = R. E3724 (a) Since P av = im 2 R/2 = E m 2 R/2Z 2 , then P av is a maximum when Z is a minimum, and viseversa. Z is a minimum at resonance, when Z = R and f = 1/2 LC. When Z is a minimum C = 1/4 2 f 2 L = 1/4 2 (60 Hz)2 (60 mH) = 1.2107 F. (b) Z is a maximum when XC is a maximum, which occurs when C is very small, like zero. (c) When XC is a maximum P = 0. When P is a maximum Z = R so P = (30 V)2 /2(5.0 ) = 90 W. (d) The phase angle is zero for resonance; it is 90 for infinite XC or XL . (e) The power factor is zero for a system which has no power. The power factor is one for a system in resonance. E3725 (a) The resistance is R = 15.0 . The inductive reactance is XC = 1 1 = = 61.3 . 1 )(4.72F) C 2(550 s
The inductive reactance is given by XL = L = 2(550 s1 )(25.3 mH) = 87.4 . The impedance is then Z= Finally, the rms current is E rms (75.0 V) = = 2.49 A. Z (30.1 ) (b) The rms voltages between any two points is given by irms = (V )rms = irms Z, where Z is not the impedance of the circuit but instead the impedance between the two points in question. When only one device is between the two points the impedance is equal to the reactance (or resistance) of that device. We're not going to show all of the work here, but we will put together a nice table for you Points ab bc cd bd ac Impedance Expression Z=R Z = XC Z = XL Z = XL  XC  2 Z = R 2 + XC Impedance Value Z = 15.0 Z = 61.3 Z = 87.4 Z = 26.1 Z = 63.1 (V )rms , 37.4 V, 153 V, 218 V, 65 V, 157 V, (15.0 )2 + ((87.4 )  (61.3 )) = 30.1 .
2
Note that this last one was Vac , and not Vad , because it is more entertaining. You probably should use Vad for your homework. (c) The average power dissipated from a capacitor or inductor is zero; that of the resistor is PR = [(VR )rms ]2 /R = (37.4 V)2 /(15.0) = 93.3 W. 155
E3726 (a) The energy stored in the capacitor is a function of the charge on the capacitor; although the charge does vary with time it varies periodically and at the end of the cycle has returned to the original values. As such, the energy stored in the capacitor doesn't change from one period to the next. (b) The energy stored in the inductor is a function of the current in the inductor; although the current does vary with time it varies periodically and at the end of the cycle has returned to the original values. As such, the energy stored in the inductor doesn't change from one period to the next. (c) P = Ei = E m im sin(t) sin(t  ), so the energy generated in one cycle is
T T
U
=
0
P dt = E m im
0 T
sin(t) sin(t  )dt,
= E m im
0
sin(t) sin(t  )dt,
=
T E m im cos . 2
(d) P = im 2 R sin2 (t  ), so the energy dissipated in one cycle is
T T
U
=
0
P dt = im 2 R
0 T
sin2 (t  )dt,
= im 2 R
0
sin2 (t  )dt,
=
T 2 im R. 2
(e) Since cos = R/Z and E m /Z = im we can equate the answers for (c) and (d). E3727 Apply Eq. 3741, V s = V p E3728 (a) Apply Eq. 3741, V s = V p (b) is = (2.4 V)/(15 ) = 0.16 A; ip = is Ns (10) = (0.16 A) = 3.2103 A. Np (500) Ns (10) = (120 V) = 2.4 V. Np (500) Ns (780) = (150 V) = 1.8103 V. Np (65)
E3729 The autotransformer could have a primary connected between taps T1 and T2 (200 turns), T1 and T3 (1000 turns), and T2 and T3 (800 turns). The same possibilities are true for the secondary connections. Ignoring the onetoone connections there are 6 choices three are step up, and three are step down. The step up ratios are 1000/200 = 5, 800/200 = 4, and 1000/800 = 1.25. The step down ratios are the reciprocals of these three values.
156
E3730 = (1.69108 m)[1  (4.3103 /C )(14.6 C)] = 1.58108 m. The resistance of the two wires is L (1.58108 m)2(1.2103 m) R= = = 14.9 . A (0.9103 m)2 P = i2 R = (3.8 A)2 (14.9 ) = 220 W. E3731 The supply current is ip = (0.270 A)(74103 V/ 2)/(220 V) = 64.2 A. The potential drop across the supply lines is V = (64.2 A)(0.62 ) = 40 V. This is the amount by which the supply voltage must be increased. E3732 Use Eq. 3746: N p /N s = (1000 )/(10 ) = 10.
P371 (a) The emf is a maximum when t  /4 = /2, so t = 3/4 = 3/4(350 rad/s) = 6.73103 s. (b) The current is a maximum when t  3/4 = /2, so t = 5/4 = 5/4(350 rad/s) = 1.12102 s. (c) The current lags the emf, so the circuit contains an inductor. (d) XL = E m /im and XL = L, so L= Em (31.4 V) = = 0.144 H. im (0.622 A)(350 rad/s)
P372 (a) The emf is a maximum when t  /4 = /2, so t = 3/4 = 3/4(350 rad/s) = 6.73103 s. (b) The current is a maximum when t+/4 = /2, so t = /4 = /4(350 rad/s) = 2.24103 s. (c) The current leads the emf, so the circuit contains an capacitor. (d) XC = E m /im and XC = 1/C, so C= im (0.622 A) = = 5.66105 F. E m (31.4 V)(350 rad/s)
P373 (a) Since the maximum values for the voltages across the individual devices are proportional to the reactances (or resistances) for devices in series (the constant of proportionality is the maximum current), we have XL = 2R and XC = R. From Eq. 3718, XL  XC 2R  R tan = = = 1, R R or = 45 . (b) The impedance of the circuit, in terms of the resistive element, is Z = R2 + (XL  XC )2 = R2 + (2R  R)2 = 2 R. But E m = im Z, so Z = (34.4 V)/(0.320 A) = 108. Then we can use our previous work to finds that R = 76. 157
P374 When the switch is open the circuit is an LRC circuit. In position 1 the circuit is an RLC circuit, but the capacitance is equal to the two capacitors of C in parallel, or 2C. In position 2 the circuit is a simple LC circuit with no resistance. The impedance when the switch is in position 2 is Z2 = L  1/C. But Z2 = (170 V)/(2.82 A) = 60.3 . The phase angle when the switch is open is 0 = 20 . But tan 0 = Z2 L  1/C = , R R
so R = (60.3 )/ tan(20 ) = 166 . The phase angle when the switch is in position 1 is tan 1 = L  1/2C , R
so L  1/2C = (166 ) tan(10 ) = 29.2 . Equating the L part, (29.2 ) + 1/2C C Finally, L= (60.3) + 1/(377 rad/s)(1.48105 F) = 0.315 H. (377 rad/s) = = (60.3 ) + 1/C, 1/2(377 rad/s)[(60.3 ) + (29.2 )] = 1.48105 F.
P375 All three wires have emfs which vary sinusoidally in time; if we choose any two wires the phase difference will have an absolute value of 120 . We can then choose any two wires and expect (by symmetry) to get the same result. We choose 1 and 2. The potential difference is then V1  V2 = V m (sin t  sin(t  120 )) . We need to add these two sine functions to get just one. We use 1 1 sin  sin = 2 sin (  ) cos ( + ). 2 2 Then V1  V 2 1 1 2V m sin (120 ) cos (2t  120 ), 2 2 3 = 2V m ( ) cos(t  60 ), 2 = 3V m sin(t + 30 ). =
P376 (a) cos = cos(42 ) = 0.74. (b) The current leads. (c) The circuit is capacitive. (d) No. Resonance circuits have a power factor of one. (e) There must be at least a capacitor and a resistor. (f) P = (75 V)(1.2 A)(0.74)/2 = 33 W.
158
P377 (a) = 1/ LC = 1/ (0.988 H)(19.3106 F) = 229 rad/s. (b) im = (31.3 V)/(5.12 ) = 6.11 A. (c) The current amplitude will be halved when the impedance is doubled, or when Z = 2R. This occurs when 3R2 = (L  1/C)2 , or 3R2 2 = 4 L2  2 2 L/C + 1/C 2 . The solution to this quadratic is =
2
2L + 3CR2
9C 2 R4 + 12CR2 L , 2L2 C
so 1 = 224.6 rad/s and 2 = 233.5 rad/s. (d) / = (8.9 rad/s)/(229 rad/s) = 0.039. P378 (a) The current amplitude will be halved when the impedance is doubled, or when Z = 2R. This occurs when 3R2 = (L  1/C)2 , or 3R2 2 = 4 L2  2 2 L/C + 1/C 2 . The solution to this quadratic is =
2
2L + 3CR2
9C 2 R4 + 12CR2 L , 2L2 C
Note that = +   ; with a wee bit of algebra,
2 2 (+ +  ) = +   .
Also, + +  2. Hence, assuming that CR2 P379 P3710 P3711 Use Eq. 3746. (a) The resistance of this bulb is R= (V )2 (120 V)2 = = 14.4 . P (1000 W) 159 4L/3. 9C 2 R4 + 12CR2 L , 2 2L C 2 R 9C 2 R2 + 12LC , 2L R 9 2 C 2 R2 + 12 , 2L R 9CR2 /L + 12 , 2L 3R , L
The power is directly related to the brightness; if the bulb is to be varied in brightness by a factor of 5 then it would have a minimum power of 200 W. The rms current through the bulb at this power would be irms = P/R = (200 W)/(14.4 ) = 3.73 A. The impedance of the circuit must have been Z= The inductive reactance would then be XL = Z 2  R2 = (32.2 )2  (14.4 )2 = 28.8 . E rms (120 V) = = 32.2 . irms (3.73 A)
Finally, the inductance would be L = XL / = (28.8 )/(2(60.0 s1 )) = 7.64 H. (b) One could use a variable resistor, and since it would be in series with the lamp a value of 32.2  14.4 = 17.8 would work. But the resistor would get hot, while on average there is no power radiated from a pure inductor.
160
E381 The maximum value occurs where r = R; there Bmax = 1 0 0 R dE/dt. For r < R B is 2 half of Bmax when r = R/2. For r > R B is half of Bmax when r = 2R. Then the two values of r are 2.5 cm and 10.0 cm. E382 For a parallel plate capacitor E = / id =
0 0
and the flux is then E = A/
0
= q/ 0 . Then
dE dq d dV = = CV = C . dt dt dt dt
E383 Use the results of Exercise 2, and change the potential difference across the plates of the capacitor at a rate id (1.0 mA) dV = = = 1.0 kV/s. dt C (1.0F) Provide a constant current to the capacitor i= d dV dQ = CV = C = id . dt dt dt
E384 Since E is uniform between the plates E = EA, regardless of the size of the region of interest. Since j d = id /A, id 1 dE dE jd = = = 0 . 0 A A dt dt E385 (a) In this case id = i = 1.84 A. (b) Since E = q/ 0 A, dE/dt = i/ 0 A, or dE/dt = (1.84 A)/(8.851012 F/m)(1.22 m)2 = 1.401011 V/m. (c) id = 0 dE /dt = 0 adE/dt. a here refers to the area of the smaller square. Combine this with the results of part (b) and id = ia/A = (1.84 A)(0.61 m/1.22 m)2 = 0.46 A. (d) B ds = 0 id = (4107 H/m)(0.46 A) = 5.78107 T m.
E386 Substitute Eq. 388 into the results obtained in Sample Problem 381. Outside the capacitor E = R2 E, so 0 0 R2 dE 0 B= = id . 2r dt 2r Inside the capacitor the enclosed flux is E = r2 E; but we want instead to define id in terms of the total E inside the capacitor as was done above. Consequently, inside the conductor B= E387 have 0 r 2R2
0 R 2
dE
dt
=
0 r id . 2R2
Since the electric field is uniform in the area and perpendicular to the surface area we E = E dA = E dA = E dA = EA.
The displacement current is then id =
0A
dE dE = (8.851012 F/m)(1.9 m2 ) . dt dt 161
(a) In the first region the electric field decreases by 0.2 MV/m in 4s, so id = (8.851012 F/m)(1.9 m2 ) (0.2106 V/m) = 0.84 A. (4106 s)
(b) The electric field is constant so there is no change in the electric flux, and hence there is no displacement current. (c) In the last region the electric field decreases by 0.4 MV/m in 5s, so id = (8.851012 F/m)(1.9 m2 ) (0.4106 V/m) = 1.3 A. (5106 s)
E388 (a) Because of the circular symmetry B ds = 2rB, where r is the distance from the center of the circular plates. Not only that, but id = j d A = r2 j d . Equate these two expressions, and B = 0 rj d /2 = (4107 H/m)(0.053 m)(1.87101 A/m)/2 = 6.23107 T. (b) dE/dt = id / 0 A = j d /
0
= (1.87101 A/m)/(8.851012 F/m) = 2.111012 V/m.
E389 The magnitude of E is given by E= (162 V) sin 2(60/s)t; (4.8103 m)
Using the results from Sample Problem 381, Bm = = = 0 0 R dE 2 dt ,
t=0
(4107 H/m)(8.851012 F/m)(0.0321 m) (162 V) 2(60/s) , 2 (4.8103 m) 2.271012 T.
E3810 (a) Eq. 3313 from page 764 and Eq. 3334 from page 762. (b) Eq. 2711 from page 618 and the equation from Ex. 2725 on page 630. (c) The equations from Ex. 386 on page 876. (d) Eqs. 3416 and 3417 from page 785. E3811 (a) Consider the path abef a. The closed line integral consists of two parts: b e and e f a b. Then d E ds =  dt can be written as E ds +
be ef ab
E ds = 
d abef . dt
Now consider the path bcdeb. The closed line integral consists of two parts: b c d e and e b. Then d E ds =  dt can be written as E ds +
bcde eb
E ds =  162
d bcde . dt
These two expressions can be added together, and since E ds = 
eb be
E ds d (abef + bcde ) . dt
we get E ds +
ef ab bcde
E ds = 
The left hand side of this is just the line integral over the closed path ef adcde; the right hand side is the net change in flux through the two surfaces. Then we can simplify this expression as E ds =  d . dt
(b) Do everything above again, except substitute B for E. (c) If the equations were not self consistent we would arrive at different values of E and B depending on how we defined our surfaces. This multivalued result would be quite unphysical. E3812 (a) Consider the part on the left. It has a shared surface s, and the other surfaces l. Applying Eq. I, ql /
0
=
E dA =
s
E dA +
l
E dA.
Note that dA is directed to the right on the shared surface. Consider the part on the right. It has a shared surface s, and the other surfaces r. Applying Eq. I, qr /
0
=
E dA =
s
E dA +
r
E dA.
Note that dA is directed to the left on the shared surface. Adding these two expressions will result in a canceling out of the part E dA
s
since one is oriented opposite the other. We are left with qr + ql
0
=
r
E dA +
l
E dA =
E dA.
E3813 E3814 (a) Electric dipole is because the charges are separating like an electric dipole. Magnetic dipole because the current loop acts like a magnetic dipole. E3815 A series LC circuit will oscillate naturally at a frequency f= 1 = 2 2 LC
We will need to combine this with v = f , where v = c is the speed of EM waves. We want to know the inductance required to produce an EM wave of wavelength = 550109 m, so 2 (550 109 m)2 L= = = 5.01 1021 H. 4 2 c2 C 4 2 (3.00 108 m/s)2 (17 1012 F) This is a small inductance! 163
E3816 (a) B = E/c, and B must be pointing in the negative y direction in order that the wave be propagating in the positive x direction. Then Bx = Bz = 0, and By = Ez /c = (2.34104 V/m)/(3.00108 m/s) = (7.801013 T) sin k(x  ct). (b) = 2/k = 2/(9.72106 /m) = 6.46107 m. E3817 The electric and magnetic field of an electromagnetic wave are related by Eqs. 3815 and 3816, (321V/m) E B= = = 1.07 pT. c (3.00 108 m/s) E3818 Take the partial of Eq. 3814 with respect to x, E x x 2E x2 Take the partial of Eq. 3817 with respect to t,  B t x 2B  tx E , t t 2 E = 0 0 2 . t = 0
0
B , x t 2B =  . xt = 
Equate, and let 0
0
= 1/c2 , then
2E 1 2E = 2 2. x2 c t Repeat, except now take the partial of Eq. 3814 with respect to t, and then take the partial of Eq. 3817 with respect to x. E3819 (a) Since sin(kx  t) is of the form f (kx t), then we only need do part (b). (b) The constant E m drops out of the wave equation, so we need only concern ourselves with f (kx t). Letting g = kx t, 2f t2 2 g t g t = c2 2f , x2 2 f g = c2 2 g x g = c , x = ck.
2f g 2
2
,
E3820 Use the right hand rule. E3821 U = P t = (1001012 W)(1.0109 s) = 1.0105 J. E3822 E = Bc = (28109 T)(3.0108 m/s) = 8.4 V/m. It is in the positive x direction.
164
E3823 Intensity is given by Eq. 3828, which is simply an expression of power divided by surface area. To find the intensity of the TV signal at Centauri we need to find the distance in meters; r = (4.30 lightyears)(3.00108 m/s)(3.15107 s/year) = 4.06 1016 m. The intensity of the signal when it has arrived at out nearest neighbor is then I= (960 kW) P 2 = = 4.63 1029 W/m 4r2 4(4.06 1016 m)2
E3824 (a) From Eq. 3822, S = cB 2 /0 . B = B m sin t. The time average is defined as 1 T
T
S dt =
0
cB m 2 0 T
T
cos2 t dt =
0
cB m 2 . 20
(b) S av = (3.0108 m/s)(1.0104 T)2 /2(4107 H/m) = 1.2106 W/m2 . E3825 I = P/4r2 , so r= E3826 uE =
0E 2
P/4I =
2 0 (cB) /2
(1.0103 W)/4(130 W/m2 ) = 0.78 m.
/2 =
= B 2 /20 = uB .
E3827 (a) Intensity is related to distance by Eq. 3828. If r1 is the original distance from the street lamp and I1 the intensity at that distance, then I1 = P 2. 4r1
There is a similar expression for the closer distance r2 = r1 162 m and the intensity at that distance I2 = 1.50I1 . We can combine the two expression for intensity, I2 P 2 4r2
2 r1
=
1.50I1 , P = 1.50 2, 4r1
r1
1.50r2 , 2 = 1.50 (r1  162 m). =
The last line is easy enough to solve and we find r1 = 883 m. (b) No, we can't find the power output from the lamp, because we were never provided with an absolute intensity reference. E3828 (a) E m = Em = 20 cI, so
2(4107 H/m)(3.00108 m/s)(1.38103 W/m2 ) = 1.02103 V/m.
(b) B m = E m /c = (1.02103 V/m)/(3.00108 m/s) = 3.40106 T. E3829 (a) B m = E m /c = (1.96 V/m)/(3.00108 m/s) = 6.53109 T. (b) I = E m 2 /20 c = (1.96 V)2 /2(4107 H/m)(3.00108 m/s) = 5.10103 W/m2 . (c) P = 4r2 I = 4(11.2 m)2 (5.10103 W/m2 ) = 8.04 W. 165
E3830 (a) The intensity is I= (11012 W) P = = 1.961027 W/m2 . A 4(6.37106 m)2
The power received by the Arecibo antenna is P = IA = (1.961027 W/m2 )(305 m)2 /4 = 1.41022 W. (b) The power of the transmitter at the center of the galaxy would be P = IA = (1.961027 W)(2.3104 ly)2 (9.461015 m/ly)2 = 2.91014 W. E3831 (a) The electric field amplitude is related to the intensity by Eq. 3826, I= or Em = 20 cI = 2(4107 H/m)(3.00108 m/s)(7.83W/m2 ) = 7.68102 V/m. (b) The magnetic field amplitude is given by Bm = Em (7.68 102 V/m) = = 2.56 1010 T c (3.00 108 m/s) E2 m , 20 c
(c) The power radiated by the transmitter can be found from Eq. 3828, P = 4r2 I = 4(11.3 km)2 (7.83W/m2 ) = 12.6 kW. E3832 (a) The power incident on (and then reflected by) the target craft is P1 = I1 A = P0 A/2r2 . The intensity of the reflected beam is I2 = P1 /2r2 = P0 A/4 2 r4 . Then I2 = (183103 W)(0.222 m2 )/4 2 (88.2103 m)4 = 1.701017 W/m2 . (b) Use Eq. 3826: Em = (c) B rms 20 cI = 2(4107 H/m)(3.00108 m/s)(1.701017 W/m2 ) = 1.13107 V/m. = E m / 2c = (1.13107 V/m)/ 2(3.00108 m/s) = 2.661016 T.
E3833 Radiation pressure for absorption is given by Eq. 3834, but we need to find the energy absorbed before we can apply that. We are given an intensity, a surface area, and a time, so U = (1.1103 W/m2 )(1.3 m2 )(9.0103 s) = 1.3107 J. The momentum delivered is p = (U )/c = (1.3107 J)/(3.00108 m/s) = 4.3102 kg m/s. E3834 (a) F/A = I/c = (1.38103 W/m2 )/(3.00108 m/s) = 4.60106 Pa. (b) (4.60106 Pa)/(101105 Pa) = 4.551011 . E3835 F/A = 2P/Ac = 2(1.5109 W)/(1.3106 m2 )(3.0108 m/s) = 7.7106 Pa. 166
E3836 F/A = P/4r2 c, so F/A = (500 W)/4(1.50 m)2 (3.00108 m/s) = 5.89108 Pa. E3837 (a) F = IA/c, so F = (1.38103 W/m2 )(6.37106 m)2 = 5.86108 N. (3.00108 m/s)
E3838 (a) Assuming MKSA, the units are m C V sN Ns mFV N = = 2 . s m m Am s Vm m Cm m s (b) Assuming MKSA, the units are A2 V N A2 J N 1 J J = = = 2 . N m Am N Cm Am sm m m s E3839 We can treat the object as having two surfaces, one completely reflecting and the other completely absorbing. If the entire surface has an area A then the absorbing part has an area f A while the reflecting part has area (1  f )A. The average force is then the sum of the force on each part, I 2I F av = f A + (1  f )A, c c which can be written in terms of pressure as F av I = (2  f ). A c E3840 We can treat the object as having two surfaces, one completely reflecting and the other completely absorbing. If the entire surface has an area A then the absorbing part has an area f A while the reflecting part has area (1  f )A. The average force is then the sum of the force on each part, I 2I F av = f A + (1  f )A, c c which can be written in terms of pressure as F av I = (2  f ). A c The intensity I is that of the incident beam; the reflected beam will have an intensity (1  f )I. Each beam will contribute to the energy density I/c and (1  f )I/c, respectively. Add these two energy densities to get the net energy density outside the surface. The result is (2  f )I/c, which is the left hand side of the pressure relation above. E3841 The bullet density is = N m/V . Let V = Ah; the kinetic energy density is K/V = 1 2 2 N mv /Ah. h/v, however, is the time taken for N balls to strike the surface, so that P = F N mv N mv 2 2K = = = . A At Ah V
167
E3842 F = IA/c; P = IA; a = F/m; and v = at. Combine: v = P t/mc = (10103 W)(86400 s)/(1500 kg)(3108 m/s) = 1.9103 m/s. E3843 The force of radiation on the bottom of the cylinder is F = 2IA/c. The force of gravity on the cylinder is W = mg = HAg. Equating, 2I/c = Hg. The intensity of the beam is given by I = 4P/d2 . Solving for H, H= 8(4.6 W) 8P = 4.9107 m. = 2 8 m/s)(1200 kg/m3 )(9.8 m/s2 )(2.6103 m)2 cgd (3.010
E3844 F = 2IA/c. The value for I is in Ex. 3837, among other places. Then F = (1.38103 W/m2 )(3.1106 m2 )/(3.00108 m/s) = 29 N. P381 For the two outer circles use Eq. 3313. For the inner circle use E = V /d, Q = CV , C = 0 A/d, and i = dQ/dt. Then i= dQ 0 A dV = = dt d dt
0A
dE . dt
The change in flux is dE /dt = A dE/dt. Then B dl = 0 so B = 0 i/2r. P382 (a) id = i. Assuming V = (174103 V) sin t, then q = CV and i = dq/dt = Cd(V )/dt. Combine, and use = 2(50.0/s), id = (1001012 F)(174103 V)2(50.0/s) = 5.47103 A. P383 (a) i = id = 7.63A. (b) dE /dt = id / 0 = (7.63A)/(8.851012 F/m) = 8.62105 V/m. (c) i = dq/dt = Cd(V )/dt; C = 0 A/d; [d(V )/dt]m = E m . Combine, and d=
0A 0
dE = 0 i, dt
C
=
0 AE m
i
=
(8.851012 F/m)(0.182 m)2 (225 V)(128 rad/s) = 3.48103 m. (7.63A)
P384 (a) q = i dt = t dt = t2 /2. (b) E = / 0 = q/ 0 A = t2 /2R2 0 . (d) 2rB = 0 0 r2 dE/dt, so B = 0 r(dE/dt)/2 = 0 rt/2R2 . (e) Check Exercise 3810! P385 ^ (a) E = E^ and B = B k. Then S = E B/0 , or j S = EB/mu0 ^ i. Energy only passes through the yz faces; it goes in one face and out the other. The rate is P = SA = EBa2 /mu0 . (b) The net change is zero. 168
P386
(a) For a sinusoidal time dependence dE/dtm = E m = 2f E m . Then dE/dtm = 2(2.4109 /s)(13103 V/m) = 1.961014 V/m s.
(b) Using the result of part (b) of Sample Problem 381, B= 1 1 (4107 H/m)(8.91012 F/m)(2.4102 m) (1.961014 V/m s) = 1.3105 T. 2 2
P387 Look back to Chapter 14 for a discussion on the elliptic orbit. On page 312 it is pointed out that the closest distance to the sun is Rp = a(1  e) while the farthest distance is Ra = a(1 + e), where a is the semimajor axis and e the eccentricity. The fractional variation in intensity is I I = = = Ip  Ia , Ia Ip  1, Ia Ra 2  1, Rp 2 (1 + e)2  1. (1  e)2
We need to expand this expression for small e using (1 + e)2 1 + 2e, and (1  e)2 1 + 2e, and finally (1 + 2e)2 1 + 4e. Combining, I (1 + 2e)2  1 4e. I P388 The beam radius grows as r = (0.440 rad)R, where R is the distance from the origin. The beam intensity is I= P (3850 W) = = 4.3102 W. 2 r (0.440 rad)2 (3.82108 m)2
P389
Eq. 3814 requires E x E m k cos kx sin t Emk B , t = B m cos kx sin t, = B m . = 
Eq. 3817 requires E t 0 0 E m sin kx cos t 0 0 E m 0
0
B , x = B m k sin kx cos t, = B m k. = 
Dividing one expression by the other, 0 0 k 2 = 2 , 169
or .
1 =c= k 0
0
Not only that, but E m = cB m . You've seen an expression similar to this before, and you'll see expressions similar to it again. (b) We'll assume that Eq. 3821 is applicable here. Then S = = 1 EmBm = sin kx sin t cos kx cos t, 0 0 E2 m sin 2kx sin 2t 40 c
is the magnitude of the instantaneous Poynting vector. (c) The time averaged power flow across any surface is the value of 1 T
T
S dA dt,
0
where T is the period of the oscillation. We'll just gloss over any concerns about direction, and assume that the S will be constant in direction so that we will, at most, need to concern ourselves about a constant factor cos . We can then deal with a scalar, instead of vector, integral, and we can integrate it in any order we want. We want to do the t integration first, because an integral over sin t for a period T = 2/ is zero. Then we are done! (d) There is no energy flow; the energy remains inside the container. P3810 (a) The electric field is parallel to the wire and given by E = V /d = iR/d = (25.0 A)(1.00 /300 m) = 8.33102 V/m (b) The magnetic field is in rings around the wire. Using Eq. 3313, B= (c) S = EB/0 , so S = (8.33102 V/m)(4.03103 T)/(4107 H/m) = 267 W/m2 . P3811 (a) We've already calculated B previously. It is B= 0 i E where i = . 2r R 0 i (4107 H/m)(25 A) = = 4.03103 T. 2r 2(1.24103 m)
The electric field of a long straight wire has the form E = k/r, where k is some constant. But
b
V = 
E ds = 
a
E dr = k ln(b/a).
In this problem the inner conductor is at the higher potential, so k= V E = , ln(b/a) ln(b/a)
170
E . r ln(b/a) This is also a vector field, and if E is positive the electric field points radially out from the central conductor. (b) The Poynting vector is 1 S= E B; 0 E= E is radial while B is circular, so they are perpendicular. Assuming that E is positive the direction of S is away from the battery. Switching the sign of E (connecting the battery in reverse) will flip the direction of both E and B, so S will pick up two negative signs and therefore still point away from the battery. The magnitude is E2 EB S= = 0 2R ln(b/a)r2 (c) We want to evaluate a surface integral in polar coordinates and so dA = (dr)(rd). We have already established that S is pointing away from the battery parallel to the central axis. Then we can integrate P = =
a b 0
and then the electric field is
S dA =
b 2
S dA,
E2 d r dr, 2R ln(b/a)r2
=
a
E2 dr, R ln(b/a)r
= (d) Read part (b) above.
E2 . R
P3812 (a) B is oriented as rings around the cylinder. If the thumb is in the direction of current then the fingers of the right hand grip ion the direction of the magnetic field lines. E is directed parallel to the wire in the direction of the current. S is found from the cross product of these two, and must be pointing radially inward. (b) The magnetic field on the surface is given by Eq. 3313: B = 0 i/2a. The electric field on the surface is given by E = V /l = iR/l Then S has magnitude i iR i2 R = . 2a l 2al S dA is only evaluated on the surface of the cylinder, not the end caps. S is everywhere parallel to dA, so the dot product reduces to S dA; S is uniform, so it can be brought out of the integral; dA = 2al on the surface. Hence, S = EB/0 = S dA = i2 R, as it should. 171
P3813 (a) f = vlambda = (3.00108 m/s)/(3.18 m) = 9.43107 Hz. (b) Bmust be directed along the z axis. The magnitude is B = E/c = (288 V/m)/(3.00108 m/s) = 9.6107 T. (c) k = 2/ = 2/(3.18 m) = 1.98/m while = 2f , so = 2(9.43107 Hz) = 5.93108 rad/s. (d) I = E m B m /20 , so I= (288 V)(9.6107 T) = 110 W. 2(4107 H/m)
(e) P = I/c = (110 W)/(3.00108 m/s) = 3.67107 Pa. P3814 (a) B is oriented as rings around the cylinder. If the thumb is in the direction of current then the fingers of the right hand grip ion the direction of the magnetic field lines. E is directed parallel to the wire in the direction of the current. S is found from the cross product of these two, and must be pointing radially inward. (b) The magnitude of the electric field is E= V Q Q it = = = . d Cd 0A 0A
The magnitude of the magnetic field on the outside of the plates is given by Sample Problem 381, B= S has magnitude S= Integrating, S dA =
0R
0 0 R dE 0 0 iR 0 0 R = = E. 2 dt 2 0A 2t EB 0R 2 = E . 0 2t E 2 2Rd = Ad
0E 2
2t
t
.
But E is linear in t, so d(E 2 )/dt = 2E 2 /t; and then S dA = Ad d dt 1 2 . 0E 2
P3815 (a) I = P/A = (5.00103 W)/(1.05)2 (633109 m)2 = 3.6109 W/m2 . (b) p = I/c = (3.6109 W/m2 )/(3.00108 m/s) = 12 Pa (c) F = pA = P/c = (5.00103 W)/(3.00108 m/s) = 1.671011 N. (d) a = F/m = F/V , so a= (1.671011 N) = 2.9103 m/s2 . 4(4880 kg/m3 )(1.05)3 (633109 )3 /3
172
P3816
The force from the sun is F = GM m/r2 . The force from radiation pressure is F = 2P A 2IA = . c 4r2 c 4GM m , 2P/c
Equating, A= so A=
4(6.671011 N m2 /kg2 )(1.991030 kg)(1650 kg) = 1.06106 m2 . 2(3.91026 W)/(3.0108 m/s)
That's about one square kilometer.
173
E391 Both scales are logarithmic; choose any data point from the right hand side such as c = f (1 Hz)(3108 m) = 3108 m/s, and another from the left hand side such as c = f (11021 Hz)(31013 m) = 3108 m/s. E392 (a) f = v/ = (3.0108 m/s)/(1.0104 )(6.37106 m) = 4.7103 Hz. If we assume that this is the data transmission rate in bits per second (a generous assumption), then it would take 140 days to download a webpage which would take only 1 second on a 56K modem! (b) T = 1/f = 212 s = 3.5 min. E393 (a) Apply v = f . Then f = (3.0108 m/s)/(0.0671015 m) = 4.51024 Hz. (b) = (3.0108 m/s)/(30 Hz) = 1.0107 m. E394 Don't simply take reciprocal of linewidth! f = c/, so f = (c/2 ). Ignore the negative, and f = (3.00108 m/s)(0.010109 m)/(632.8109 m)2 = 7.5109 Hz. E395 (a) We refer to Fig. 396 to answer this question. The limits are approximately 520 nm and 620 nm. (b) The wavelength for which the eye is most sensitive is 550 nm. This corresponds to to a frequency of f = c/ = (3.00 108 m/s)/(550 109 m) = 5.45 1014 Hz. This frequency corresponds to a period of T = 1/f = 1.83 1015 s. E396 f = c/. The number of complete pulses is f t, or f t = ct/ = (3.00108 m/s)(4301012 s)/(520109 m) = 2.48105 . E397 (a) 2(4.34 y) = 8.68 y. (b) 2(2.2106 y) = 4.4106 y. E398 (a) t = (150103 m)/(3108 m/s) = 5104 s. (b) The distance traveled by the light is (1.51011 m) + 2(3.8108 m), so t = (1.511011 m)/(3108 m/s) = 503 s. (c) t = 2(1.31012 m)/(3108 m/s) = 8670 s. (d) 1054  6500 5400 BC. E399 This is a question of how much time it takes light to travel 4 cm, because the light traveled from the Earth to the moon, bounced off of the reflector, and then traveled back. The time to travel 4 cm is t = (0.04 m)/(3 108 m/s) = 0.13 ns. Note that I interpreted the question differently than the answer in the back of the book.
174
E3910 Consider any incoming ray. The path of the ray can be projected onto the xy plane, the xz plane, or the yz plane. If the projected rays is exactly reflected in all three cases then the three dimensional incoming ray will be reflected exactly reversed. But the problem is symmetric, so it is sufficient to show that any plane works. Now the problem has been reduced to Sample Problem 392, so we are done. E3911 We will choose the mirror to lie in the xy plane at z = 0. There is no loss of generality in doing so; we had to define our coordinate system somehow. The choice is convenient in that any normal is then parallel to the z axis. Furthermore, we can arbitrarily define the incident ray to originate at (0, 0, z1 ). Lastly, we can rotate the coordinate system about the z axis so that the reflected ray passes through the point (0, y3 , z3 ). The point of reflection for this ray is somewhere on the surface of the mirror, say (x2 , y2 , 0). This distance traveled from the point 1 to the reflection point 2 is d12 = (0  x2 )2 + (0  y2 )2 + (z1  0)2 =
2 2 x2 + y2 + z1 2
and the distance traveled from the reflection point 2 to the final point 3 is d23 = (x2  0)2 + (y2  y3 )2 + (0  z3 )2 =
2 x2 + (y2  y3 )2 + z3 . 2
The only point which is free to move is the reflection point, (x2 , y2 , 0), and that point can only move in the xy plane. Fermat's principle states that the reflection point will be such to minimize the total distance, d12 + d23 =
2 2 x2 + y2 + z1 + 2 2 x2 + (y2  y3 )2 + z3 . 2
We do this minimization by taking the partial derivative with respect to both x2 and y2 . But we can do part by inspection alone. Any nonzero value of x2 can only add to the total distance, regardless of the value of any of the other quantities. Consequently, x2 = 0 is one of the conditions for minimization. We are done! Although you are invited to finish the minimization process, once we know that x2 = 0 we have that point 1, point 2, and point 3 all lie in the yz plane. The normal is parallel to the z axis, so it also lies in the yz plane. Everything is then in the yz plane. E3912 Refer to Page 442 of Volume 1. E3913 (a) 1 = 38 . (b) (1.58) sin(38 ) = (1.22) sin 2 . Then 2 = arcsin(0.797) = 52.9 . E3914 ng = nv sin 1 / sin 2 = (1.00) sin(32.5 )/ sin(21.0 ) = 1.50. E3915 n = c/v = (3.00108 m/s)/(1.92108 m/s) = 1.56. E3916 v = c/n = (3.00108 m/s)/(1.46) = 2.05108 m/s. E3917 The speed of light in a substance with index of refraction n is given by v = c/n. An electron will then emit Cerenkov radiation in this particular liquid if the speed exceeds v = c/n = (3.00 108 m/s)/(1.54) = 1.95108 m/s.
175
E3918 Since t = d/v = nd/c, t = n d/c. Then t = (1.00029  1.00000)(1.61103 m)/(3.00108 m/s) = 1.56109 s. E3919 The angle of the refracted ray is 2 = 90 , the angle of the incident ray can be found by trigonometry, (1.14 m) tan 1 = = 1.34, (0.85 m) or 1 = 53.3 . We can use these two angles, along with the index of refraction of air, to find that the index of refraction of the liquid from Eq. 394, n1 = n2 (sin 90 ) sin 2 = 1.25. = (1.00) sin 1 (sin 53.3 )
There are no units attached to this quantity. E3920 For an equilateral prism = 60 . Then n= E3921 E3922 t = d/v; but L/d = cos 2 = t= nL c 1  sin 2
2
sin[ + ]/2 sin[(37 ) + (60 )]/2 = = 1.5. sin[/2] sin[(60 )/2]
1  sin2 2 and v = c/n. Combining, = (1.63)2 (0.547 m) (3108 m/s) (1.632 )  sin (24 )
2
= c
n2 L n2  sin 1
2
= 3.07109 s.
E3923 The ray of light from the top of the smokestack to the life ring is 1 , where tan 1 = L/h with h the height and L the distance of the smokestack. Snell's law gives n1 sin 1 = n2 sin 2 , so 1 = arcsin[(1.33) sin(27 )/(1.00)] = 37.1 . Then L = h tan 1 = (98 m) tan(37.1 ) = 74 m. E3924 The length of the shadow on the surface of the water is x1 = (0.64 m)/ tan(55 ) = 0.448 m. The ray of light which forms the "end" of the shadow has an angle of incidence of 35 , so the ray travels into the water at an angle of 2 = arcsin The ray travels an additional distance x2 = (2.00 m  0.64 m)/ tan(90  25.5 ) = 0.649 m The total length of the shadow is (0.448 m) + (0.649 m) = 1.10 m. 176 (1.00) sin(35 ) (1.33) = 25.5 .
E3925 We'll rely heavily on the figure for our arguments. Let x be the distance between the points on the surface where the vertical ray crosses and the bent ray crosses.
x d app 1
2
d
In this exercise we will take advantage of the fact that, for small angles , sin tan In this approximation Snell's law takes on the particularly simple form n1 1 = n2 2 The two angles here are conveniently found from the figure, 1 tan 1 = and 2 tan 2 = x , d x dapp .
Inserting these two angles into the simplified Snell's law, as well as substituting n1 = n and n2 = 1.0, n1 1 x n d dapp = n2 2 , x = , dapp d = . n
E3926 (a) You need to address the issue of total internal reflection to answer this question. (b) Rearrange sin[ + ]/2 n= sin[/2] / and = ( + )/2 to get = arcsin (n sin[/2]) = arcsin ((1.60) sin[(60 )/2]) = 53.1 . E3927 Use the results of Ex. 3935. The apparent thickness of the carbon tetrachloride layer, as viewed by an observer in the water, is dc,w = nw dc /nc = (1.33)(41 mm)/(1.46) = 37.5 mm. The total "thickness" from the water perspective is then (37.5 mm) + (20 mm) = 57.5 mm. The apparent thickness of the entire system as view from the air is then dapp = (57.5 mm)/(1.33) = 43.2 mm. 177
E3928 (a) Use the results of Ex. 3935. dapp = (2.16 m)/(1.33) = 1.62 m. (b) Need a diagram here! E3929 (a) n = /n = (612 nm)/(1.51) = 405 nm. (b) L = nLn = (1.51)(1.57 pm) = 2.37 pm. There is actually a typo: the "p" in "pm" was supposed to be a . This makes a huge difference for part (c)! E3930 (a) f = c/ = (3.00108 m/s)/(589 nm) = 5.091014 Hz. (b) n = /n = (589 nm)/(1.53) = 385 nm. (c) v = f = (5.091014 Hz)(385 nm) = 1.96108 m/s. E3931 (a) The second derivative of L= is a2 + x2 + b2 + (d  x)2
a2 (b2 + (d  2)2 )3/2 + b2 (a2 + x2 )3/2 . (b2 + (d  2)2 )3/2 (a2 + x2 )3/2
This is always a positive number, so dL/dx = 0 is a minimum. (a) The second derivative of L = n1 is a2 + x2 + n2 b2 + (d  x)2
n1 a2 (b2 + (d  2)2 )3/2 + n2 b2 (a2 + x2 )3/2 . (b2 + (d  2)2 )3/2 (a2 + x2 )3/2
This is always a positive number, so dL/dx = 0 is a minimum. E3932 (a) The angle of incidence on the face ac will be 90  . Total internal reflection occurs when sin(90  ) > 1/n, or < 90  arcsin[1/(1.52)] = 48.9 . (b) Total internal reflection occurs when sin(90  ) > nw /n, or < 90  arcsin[(1.33)/(1.52)] = 29.0 . E3933 (a) The critical angle is given by Eq. 3917, c = sin1 n2 (1.586) = sin1 = 72.07 . n1 (1.667)
(b) Critical angles only exist when "attempting" to travel from a medium of higher index of refraction to a medium of lower index of refraction; in this case from A to B. E3934 If the fire is at the water's edge then the light travels along the surface, entering the water near the fish with an angle of incidence of effectively 90 . Then the angle of refraction in the water is numerically equivalent to a critical angle, so the fish needs to look up at an angle of = arcsin(1/1.33) = 49 with the vertical. That's the same as 41 with the horizontal.
178
E3935 Light can only emerge from the water if it has an angle of incidence less than the critical angle, or < c = arcsin 1/n = arcsin 1/(1.33) = 48.8 . The radius of the circle of light is given by r/d = tan c , where d is the depth. The diameter is twice this radius, or 2(0.82 m) tan(48.8 ) = 1.87 m. E3936 The refracted angle is given by n sin 1 = sin(39 ). This ray strikes the left surface with an angle of incidence of 90  1 . Total internal reflection occurs when sin(90  1 ) = 1/n; but sin(90  1 ) = cos 1 , so we can combine and get tan = sin(39 ) with solution 1 = 32.2 . The index of refraction of the glass is then n = sin(39 )/ sin(32.2) = 1.18. E3937 The light strikes the quartzair interface from the inside; it is originally "white", so if the reflected ray is to appear "bluish" (reddish) then the refracted ray should have been "reddish" (bluish). Since part of the light undergoes total internal reflection while the other part does not, then the angle of incidence must be approximately equal to the critical angle. (a) Look at Fig. 3911, the index of refraction of fused quartz is given as a function of the wavelength. As the wavelength increases the index of refraction decreases. The critical angle is a function of the index of refraction; for a substance in air the critical angle is given by sin c = 1/n. As n decreases 1/n increases so c increases. For fused quartz, then, as wavelength increases c also increases. In short, red light has a larger critical angle than blue light. If the angle of incidence is midway between the critical angle of red and the critical angle of blue, then the blue component of the light will experience total internal reflection while the red component will pass through as a refracted ray. So yes, the light can be made to appear bluish. (b) No, the light can't be made to appear reddish. See above. (c) Choose an angle of incidence between the two critical angles as described in part (a). Using a value of n = 1.46 from Fig. 3911, c = sin1 (1/1.46) = 43.2 . Getting the effect to work will require considerable sensitivity. E3938 (a) There needs to be an opaque spot in the center of each face so that no refracted ray emerges. The radius of the spot will be large enough to cover rays which meet the surface at less than the critical angle. This means tan c = r/d, where d is the distance from the surface to the spot, or 6.3 mm. Since c = arcsin 1/(1.52) = 41.1 , then r = (6.3 mm) tan(41.1 ) = 5.50 mm. (b) The circles have an area of a = (5.50 mm)2 = 95.0 mm2 . Each side has an area of (12.6 mm)2 ; the fraction covered is then (95.0 mm2 )/(12.6 mm)2 = 0.598. E3939 For u c the relativistic Doppler shift simplifies to f = f0 u/c = u/0 , so u = 0 f = (0.211 m)f. 179
E3940 c = f , so 0 = f + f . Then / = f /f . Furthermore, f0  f , from Eq. 3921, is f0 u/c for small enough u. Then f  f0 u = = . f0 c E3941 The Doppler theory for light gives f = f0 1  u/c 1 u2 /c2 = f0 1  (0.2) 1  (0.2)2 = 0.82 f0 .
The frequency is shifted down to about 80%, which means the wavelength is shifted up by an additional 25%. Blue light (480 nm) would appear yellow/orange (585 nm). E3942 Use Eq. 3920: f = f0 1  u/c 1 u2 /c2 = (100 Mhz) 1  (0.892) 1  (0.892)2 = 23.9 MHz.
E3943 (a) If the wavelength is three times longer then the frequency is onethird, so for the classical Doppler shift f0 /3 = f0 (1  u/c), or u = 2c. (b) For the relativistic shift, f0 /3 = f0 1  u/c 1  u2 /c2 ,
1  u2 /c2 = 3(1  u/c), c2  u2 = 9(c  u)2 , 0 = 10u2  18uc + 8c2 . The solution is u = 4c/5. E3944 (a) f0 /f = /0 . This shift is small, so we apply the approximation: u=c 0 1 = (3108 m/s) (462 nm) 1 (434 nm) = 1.9107 m/s.
(b) A red shift corresponds to objects moving away from us. E3945 The sun rotates once every 26 days at the equator, while the radius is 7.0108 m. The speed of a point on the equator is then v= 2R 2(7.0108 m) = = 2.0103 m/s. T (2.2106 s)
This corresponds to a velocity parameter of = u/c = (2.0103 m/s)/(3.0108 m/s) = 6.7106 . This is a case of small numbers, so we'll use the formula that you derived in Exercise 3940: = = (553 nm)(6.7106 ) = 3.7103 nm. 180
E3946 Use Eq. 3923 written as (1  u/c)2 = 2 (1 + u/c), 0 which can be rearranged as u/c = 2  2 (540 nm)2  (620 nm)2 0 = = 0.137. 2 + 2 (540 nm)2 + (620 nm)2 0
The negative sign means that you should be going toward the red light. E3947 (a) f1 = cf /(c + v) and f2 = cf /(c  v). f = (f2  f )  (f  f1 ) = f2 + f1  2f, so f f = = = = c c +  2, c+v cv 2v 2 , c2  v 2 2(8.65105 m/s)2 , (3.00108 m/s)2  (8.65105 m/s)2 1.66105 .
(b) f1 = f (c  u)/sqrtc2  u2 and f2 = f (c + u)/ c2  u2 . f = (f2  f )  (f  f1 ) = f2 + f1  2f, so f f = = = c2 2c  2,  u2 2(3.00108 m/s)
(3.00108 m/s)2  (8.65105 m/s)2 8.3106 .
 2,
E3948 (a) No relative motion, so every 6 minutes. (b) The Doppler effect at this speed is 1  u/c 1 u2 /c2 = 1  (0.6) 1  (0.6)2 = 0.5;
this means the frequency is one half, so the period is doubled to 12 minutes. (c) If C send the signal at the instant the signal from A passes, then the two signals travel together to C, so C would get B's signals at the same rate that it gets A's signals: every six minutes. E3949 E3950 The transverse Doppler effect is = 0 / 1  u2 /c2 . Then = (589.00 nm)/ 1  (0.122)2 = 593.43 nm. The shift is (593.43 nm)  (589.00 nm) = 4.43 nm. 181
E3951
The frequency observed by the detector from the first source is (Eq. 3931) f = f1 1  (0.717)2 = 0.697f1 .
The frequency observed by the detector from the second source is (Eq. 3930) f = f2 1  (0.717)2 0.697f2 = . 1 + (0.717) cos 1 + (0.717) cos 0.697f2 , 1 + 0.717 cos = f2 /f1 , = (f2 /f1  1) /0.717, = 101.1 . =
We need to equate these and solve for . Then 0.697f1 1 + 0.717 cos cos
Subtract from 180 to find the angle with the line of sight. E3952 P391 Consider the triangle in Fig. 3945. The true position corresponds to the speed of light, the opposite side corresponds to the velocity of earth in the orbit. Then = arctan(29.8103 m/s)/(3.00108 m/s) = 20.5 . P392 is The distance to Jupiter from point x is dx = rj  re . The distance to Jupiter from point y d2 =
2 2 re + rj .
The difference in distance is related to the time according to (d2  d1 )/t = c, so (778109 m)2 + (150109 m)2  (778109 m) + (150109 m) = 2.7108 m/s. (600 s)
P393 sin(30 )/(4.0 m/s) = sin /(3.0 m/s). Then = 22 . Water waves travel more slowly in shallower water, which means they always bend toward the normal as they approach land. P394 (a) If the ray is normal to the water's surface then it passes into the water undeflected. Once in the water the problem is identical to Sample Problem 392. The reflected ray in the water is parallel to the incident ray in the water, so it also strikes the water normal, and is transmitted normal. (b) Assume the ray strikes the water at an angle 1 . It then passes into the water at an angle 2 , where nw sin 2 = na sin 1 . Once the ray is in the water then the problem is identical to Sample Problem 392. The reflected ray in the water is parallel to the incident ray in the water, so it also strikes the water at an angle 2 . When the ray travels back into the air it travels with an angle 3 , where nw sin 2 = na sin 3 . Comparing the two equations yields 1 = 3 , so the outgoing ray in the air is parallel to the incoming ray. 182
P395
(a) As was done in Ex. 3925 above we use the small angle approximation of sin tan
The incident angle is ; if the light were to go in a straight line we would expect it to strike a distance y1 beneath the normal on the right hand side. The various distances are related to the angle by tan y1 /t. The light, however, does not go in a straight line, it is refracted according to (the small angle approximation to) Snell's law, n1 1 = n2 2 , which we will simplify further by letting 1 = , n2 = n, and n1 = 1, = n2 . The point where the refracted ray does strike is related to the angle by 2 tan 2 = y2 /t. Combining the three expressions, y1 = ny2 . The difference, y1  y2 is the vertical distance between the displaced ray and the original ray as measured on the plate glass. A little algebra yields y1  y2 = y1  y1 /n, = y1 (1  1/n) , n1 = t . n
The perpendicular distance x is related to this difference by cos = x/(y1  y2 ). In the small angle approximation cos 1  2 /2. If is sufficiently small we can ignore the square term, and x y2  y1 . (b) Remember to use radians and not degrees whenever the small angle approximation is applied. Then (1.52)  1 x = (1.0 cm)(0.175 rad) = 0.060 cm. (1.52) P396 (a) At the top layer, n1 sin 1 = sin ; at the next layer, n2 sin 2 = n1 sin 1 ; at the next layer, n3 sin 3 = n2 sin 2 . Combining all three expressions, n3 sin 3 = sin . (b) 3 = arcsin[sin(50 )/(1.00029)] = 49.98 . Then shift is (50 )  (49.98 ) = 0.02 . P397 The "big idea" of Problem 6 is that when light travels through layers the angle that it makes in any layer depends only on the incident angle, the index of refraction where that incident angle occurs, and the index of refraction at the current point. That means that light which leaves the surface of the runway at 90 to the normal will make an angle n0 sin 90 = n0 (1 + ay) sin 183
at some height y above the runway. It is mildly entertaining to note that the value of n0 is unimportant, only the value of a! The expression 1 sin = 1  ay 1 + ay can be used to find the angle made by the curved path against the normal as a function of y. The slope of the curve at any point is given by dy cos = tan(90  ) = cot = . dx sin Now we need to know cos . It is cos = Combining 1  sin2 2ay dy , dx 1  ay 2ay.
and now we integrate. We will ignore the ay term in the denominator because it will always be small compared to 1. Then
d h
dx =
0 0
dy , 2ay 2(1.7 m) = 1500 m. (1.5106 m1 )
d
=
2h = a
P398 The energy of a particle is given by E 2 = p2 c2 + m2 c4 . This energy is related to the mass by E = mc2 . is related to the speed by = 1/ 1  u2 /c2 . Rearranging, u c = 1 1 = 2 1 m2 c2 , + m2 c2
p2
= Since n = c/u we can write this as n= For the pion, n= For the muon, n=
p2 . p2 + m2 c2
1+
m2 c2 = p2
1+
mc2 pc
2
.
1+
(135 MeV) (145 MeV) (106 MeV) (145 MeV)
2
= 1.37.
2
1+
= 1.24.
184
P399 (a) Before adding the drop of liquid project the light ray along the angle so that = 0. Increase slowly until total internal reflection occurs at angle 1 . Then ng sin 1 = 1 is the equation which can be solved to find ng . Now put the liquid on the glass and repeat the above process until total internal reflection occurs at angle 2 . Then ng sin 2 = nl . Note that ng < ng for this method to work. (b) This is not terribly practical. P3910 Let the internal angle at Q be Q . Then n sin Q = 1, because it is a critical angle. Let the internal angle at P be P . Then P + Q = 90 . Combine this with the other formula and 1 = n sin(90  P ) = n cos Q = n Not only that, but sin 1 = n sin P , or 1=n which can be solved for n to yield n= 1 + sin2 1 . 2. 1  (sin 1 )2 /n2 , 1  sin2 P .
(b) The largest value of the sine function is one, so nmax =
P3911 (a) The fraction of light energy which escapes from the water is dependent on the critical angle. Light radiates in all directions from the source, but only that which strikes the surface at an angle less than the critical angle will escape. This critical angle is sin c = 1/n. We want to find the solid angle of the light which escapes; this is found by integrating
2 c
=
0 0
sin d d.
This is not a hard integral to do. The result is = 2(1  cos c ). There are 4 steradians in a spherical surface, so the fraction which escapes is f= 1 1 (1  cos c ) = (1  2 2 1  sin2 c ).
The last substitution is easy enough. We never needed to know the depth h. (b) f = 1 (1  1  (1/(1.3))2 ) = 0.18. 2
185
P3912 to
(a) The beam of light strikes the face of the fiber at an angle and is refracted according n1 sin 1 = sin .
The beam then travels inside the fiber until it hits the cladding interface; it does so at an angle of 90  1 to the normal. It will be reflected if it exceeds the critical angle of n1 sin c = n2 , or if sin(90  1 ) n2 /n1 , which can be written as cos 1 n2 /n1 . but if this is the cosine, then we can use sin2 + cos2 = 1 to find the sine, and sin 1 Combine this with the first equation and arcsin (b) = arcsin (1.58)2  (1.53)2 = 23.2 . n2  n2 . 1 2 1  n2 /n2 . 2 1
P3913 Consider the two possible extremes: a ray of light can propagate in a straight line directly down the axis of the fiber, or it can reflect off of the sides with the minimum possible angle of incidence. Start with the harder option. The minimum angle of incidence that will still involve reflection is the critical angle, so sin c = n2 . n1
This light ray has farther to travel than the ray down the fiber axis because it is traveling at an angle. The distance traveled by this ray is L = L/ sin c = L n1 , n2
The time taken for this bouncing ray to travel a length L down the fiber is then t = L L n1 L n2 1 = = . v c c n2
Now for the easier ray. It travels straight down the fiber in a time t= The difference is t  t = t = L c L n1 . c = Ln1 (n1  n2 ). cn2
n2 1  n1 n2
(b) For the numbers in Problem 12 we have t = (350103 m)(1.58) ((1.58)  (1.53)) = 6.02105 s. (3.00108 m/s)(1.53) 186
P3914 P3915 We can assume the airplane speed is small compared to the speed of light, and use Eq. 3921. f = 990 Hz; so f  = f0 u/c = u/0 , hence u = (990/s)(0.12 m) = 119 m/s. The actual answer for the speed of the airplane is half this because there were two Doppler shifts: once when the microwaves struck the plane, and one when the reflected beam was received by the station. Hence, the plane approaches with a speed of 59.4 m/s.
187
E401 (b) Since i = o, vi = di/dt = do/dt = vo . (a) In order to change from the frame of reference of the mirror to your own frame of reference you need to subtract vo from all velocities. Then your velocity is vo  v0 = 0, the mirror is moving with velocity 0  vo = vo and your image is moving with velocity vo  vo = 2vo . E402 You are 30 cm from the mirror, the image is 10 cm behind the mirror. You need to focus 40 cm away. E403 If the mirror rotates through an angle then the angle of incidence will increase by an angle , and so will the angle of reflection. But that means that the angle between the incident angle and the reflected angle has increased by twice. E404 Sketch a line from Sarah through the right edge of the mirror and then beyond. Sarah can see any image which is located between that line and the mirror. By similar triangles, the image of Bernie will be d/2 = (3.0 m)/2 = 1/5 m from the mirror when it becomes visible. Since i = o, Bernie will also be 1.5 m from the mirror. E405 The images are fainter than the object. Several sample rays are shown.
E406 The image is displaced. The eye would need to look up to see it. E407 The apparent depth of the swimming pool is given by the work done for Exercise 3925, dapp = d/n The water then "appears" to be only 186 cm/1.33 = 140 cm deep. The apparent distance between the light and the mirror is then 250 cm + 140 cm = 390 cm; consequently the image of the light is 390 cm beneath the surface of the mirror. E408 Three. There is a single direct image in each mirror and one more image of an image in one of the mirrors.
188
E409 We want to know over what surface area of the mirror are rays of light reflected from the object into the eye. By similar triangles the diameter of the pupil and the diameter of the part of the mirror (d) which reflects light into the eye are related by (5.0 mm) d = , (10 cm) (24 cm) + (10 cm) which has solution d = 1.47 mm The area of the circle on the mirror is A = (1.47 mm)2 /4 = 1.7 mm2 . E4010 (a) Seven; (b) Five; and (c) Two. This is a problem of symmetry. E4011 Seven. Three images are the ones from Exercise 8. But each image has an image in the ceiling mirror. That would make a total of six, except that you also have an image in the ceiling mirror (look up, eh?). So the total is seven! E4012 A point focus is not formed. The envelope of rays is called the caustic. You can see a similar effect when you allow light to reflect off of a spoon onto a table.
E4013 The image is magnified by a factor of 2.7, so the image distance is 2.7 times farther from the mirror than the object. An important question to ask is whether or not the image is real or virtual. If it is a virtual image it is behind the mirror and someone looking at the mirror could see it. If it were a real image it would be in front of the mirror, and the man, who serves as the object and is therefore closer to the mirror than the image, would not be able to see it. So we shall assume that the image is virtual. The image distance is then a negative number. The focal length is half of the radius of curvature, so we want to solve Eq. 406, with f = 17.5 cm and i = 2.7o 1 1 1 0.63 = + = , (17.5 cm) o 2.7o o which has solution o = 11 cm. E4014 The image will be located at a point given by 1 1 1 1 1 1 =  =  = . i f o (10 cm) (15 cm) (30 cm) The vertical scale is three times the horizontal scale in the figure below.
189
E4015 This problem requires repeated application of 1/f = 1/o + 1/i, r = 2f , m = i/o, or the properties of plane, convex, or concave mirrors. All dimensioned variables below (f, r, i, o) are measured in centimeters. (a) Concave mirrors have positive focal lengths, so f = +20; r = 2f = +40; 1/i = 1/f  1/o = 1/(20)  1/(10) = 1/(20); m = i/o = (20)/(10) = 2; the image is virtual and upright. (b) m = +1 for plane mirrors only; r = for flat surface; f = /2 = ; i = o = 10; the image is virtual and upright. (c) If f is positive the mirror is concave; r = 2f = +40; 1/i = 1/f  1/o = 1/(20)  1/(30) = 1/(60); m = i/o = (60)/(30) = 2; the image is real and inverted. (d) If m is negative then the image is real and inverted; only Concave mirrors produce real images (from real objects); i = mo = (0.5)(60) = 30; 1/f = 1/o + 1/i = 1/(30) + 1/(60) = 1/(20); r = 2f = +40. (e) If r is negative the mirror is convex; f = r/2 = (40)/2 = 20; 1/o = 1/f  1/i = 1/(20)  1/(10) = 1/(20); m = (10)/(20) = 0.5; the image is virtual and upright. (f) If m is positive the image is virtual and upright; if m is less than one the image is reduced, but only convex mirrors produce reduced virtual images (from real objects); f = 20 for convex mirrors; r = 2f = 40; let i = mo = o/10, then 1/f = 1/o + 1/i = 1/o  10/o = 9/o, so o = 9f = 9(20) = 180; i = o/10 = (180)/10 = 18. (g) r is negative for convex mirrors, so r = 40; f = r/2 = 20; convex mirrors produce only virtual upright images (from real objects); so i is negative; and 1/o = 1/f  1/i = 1/(20)  1/(4) = 1/(5); m = i/o = (4)/(5) = 0.8. (h) Inverted images are real; only concave mirrors produce real images (from real objects); inverted images have negative m; i = mo = (0.5)(24) = 12; 1/f = 1/o + 1/i = 1/(24) + 1/(12) = 1/(8); r = 2f = 16. 190
E4016 Use the angle definitions provided by Eq. 408. From triangle OaI we have + = 2, while from triangle IaC we have + = . Combining to eliminate we get  = 2. Substitute Eq. 408 and eliminate s, 2 1 1  = , o i r or 1 1 2 + = , o i r which is the same as Eq. 404 if i i and r r.
E4017 (a) Consider the point A. Light from this point travels along the line ABC and will be parallel to the horizontal center line from the center of the cylinder. Since the tangent to a circle defines the outer limit of the intersection with a line, this line must describe the apparent size. (b) The angle of incidence of ray AB is given by sin 1 = r/R. The angle of refraction of ray BC is given by sin 2 = r /R. Snell's law, and a little algebra, yields n1 sin 1 r n1 R nr = n2 sin 2 , r = n2 , R = r .
In the last line we used the fact that n2 = 1, because it is in the air, and n1 = n, the index of refraction of the glass. E4018 This problem requires repeated application of (n2  n1 )/r = n1 /o + n2 /i. All dimensioned variables below (r, i, o) are measured in centimeters. (a) (1.5)  (1.0) (1.0)  = 0.08333, (30) (10) so i = (1.5)/(0.08333) = 18, and the image is virtual. (b) (1.0) (1.5) + = 0.015385, (10) (13) so r = (1.5  1.0)/(0.015385) = 32.5, and the image is virtual. (c) (1.5)  (1.0) (1.5)  = 0.014167, (30) (600) 191
so o = (1.0)/(0.014167) = 71. The image was real since i > 0. (d) Rearrange the formula to solve for n2 , then n2 Substituting the numbers, n2 1 1  (20) (20) = (1.0) 1 1 + (20) (20) , 1  1i r = n1 1 1 + r o .
which has any solution for n2 ! Since i < 0 the image is virtual. (e) (1.5) (1.0) + = 0.016667, (10) (6) so r = (1.0  1.5)/(0.016667) = 30, and the image is virtual. (f) (1.0) (1.0)  (1.5)  = 0.15, (30) (7.5) so o = (1.5)/(0.15) = 10. The image was virtual since i < 0. (g) (1.0)  (1.5) (1.5)  = 3.81102 , (30) (70) so i = (1.0)/(3.81102 ) = 26, and the image is virtual. (h) Solving Eq. 4010 for n2 yields n2 = n1 so n2 = (1.5) and the image is real. E4019 (b) If the beam is small we can use Eq. 4010. Parallel incoming rays correspond to an object at infinity. Solving for n2 yields n2 = n1 so if o and i = 2r, then n2 = (1.0) (c) There is no solution if i = r! E4020 The image will be located at a point given by 1 1 1 1 1 1 =  =  = . i f o (10 cm) (6 cm) (15 cm) 1/ + 1/r = 2.0 1/r  1/2r 1/o + 1/r , 1/r  1/i 1/o + 1/r , 1/r  1/i
1/(100) + 1/(30) = 1.0 1/(30)  1/(600)
192
E4021
The image location can be found from Eq. 4015, 1 1 1 1 1 1 =  =  = , i f o (30 cm) (20 cm) 12 cm
so the image is located 12 cm from the thin lens, on the same side as the object. E4022 For a double convex lens r1 > 0 and r2 < 0 (see Fig. 4021 and the accompanying text). Then the problem states that r2 = r1 /2. The lens maker's equation can be applied to get 1 = (n  1) f 1 1  r1 r2 = 3(n  1) , r1
so r1 = 3(n  1)f = 3(1.5  1)(60 mm) = 90 mm, and r2 = 45 mm. E4023 The object distance is essentially o = , so 1/f = 1/o + 1/i implies f = i, and the image forms at the focal point. In reality, however, the object distance is not infinite, so the magnification is given by m = i/o f /o, where o is the Earth/Sun distance. The size of the image is then hi = ho f /o = 2(6.96108 m)(0.27 m)/(1.501011 m) = 2.5 mm. The factor of two is because the sun's radius is given, and we need the diameter! E4024 (a) The flat side has r2 = , so 1/f = (n  1)/r, where r is the curved side. Then f = (0.20 m)/(1.5  1) = 0.40 m. (b) 1/i = 1/f  1/o = 1/(0.40 m)  1/(0.40 m) = 0. Then i is . E4025 (a) 1/f = (1.5  1)[1/(0.4 m)  1/(0.4 m)] = 1/(0.40 m). (b) 1/f = (1.5  1)[1/()  1/(0.4 m)] = 1/(0.80 m). (c) 1/f = (1.5  1)[1/(0.4 m)  1/(0.6 m)] = 1/(2.40 m). (d) 1/f = (1.5  1)[1/(0.4 m)  1/(0.4 m)] = 1/(0.40 m). (e) 1/f = (1.5  1)[1/()  1/(0.8 m)] = 1/(0.80 m). (f) 1/f = (1.5  1)[1/(0.6 m)  1/(0.4 m)] = 1/(2.40 m). E4026 (a) 1/f = (n  1)[1/(r)  1/r], so 1/f = 2(1  n)/r. 1/i = 1/f  1/o so if o = r, then 1/i = 2(1  n)/r  1/r = (1  2n)/r, so i = r/(1  2n). For n > 0.5 the image is virtual. (b) For n > 0.5 the image is virtual; the magnification is m = i/o = r/(1  2n)/r = 1/(2n  1). E4027 According to the definitions, o = f + x and i = f + x . Starting with Eq. 4015, 1 1 + o i i+o oi 2f + x + x (f + x)(f + x ) 2f 2 + f x + f x f2 = = = 1 , f 1 , f 1 , f
= f 2 + f x + f x + xx , = xx . 193
E4028 (a) You can't determine r1 , r2 , or n. i is found from 1 1 1 1 =  = , i +10 +20 +20 the image is real and inverted. m = (20)/(20) = 1. (b) You can't determine r1 , r2 , or n. The lens is converging since f is positive. i is found from 1 1 1 1 =  = , i +10 +5 10 the image is virtual and upright. m = (10)/(+5) = 2. (c) You can't determine r1 , r2 , or n. Since m is positive and greater than one the lens is converging. Then f is positive. i is found from 1 1 1 1 =  = , i +10 +5 10 the image is virtual and upright. m = (10)/(+5) = 2. (d) You can't determine r1 , r2 , or n. Since m is positive and less than one the lens is diverging. Then f is negative. i is found from 1 1 1 1 =  = , i 10 +5 3.3 the image is virtual and upright. m = (3.3)/(+5) = 0.66. (e) f is found from 1 1 1 1 = (1.5  1)  = . f +30 30 +30 The lens is converging. i is found from 1 1 1 1 =  = , i +30 +10 15 the image is virtual and upright. m = (15)/(+10) = 1.5. (f) f is found from 1 1 1 1 = (1.5  1)  = . f 30 +30 30 The lens is diverging. i is found from 1 1 1 1 =  = , i 30 +10 7.5 the image is virtual and upright. m = (7.5)/(+10) = 0.75. (g) f is found from 1 1 1 1 = (1.5  1)  = . f 30 60 120 The lens is diverging. i is found from 1 1 1 1 =  = , i 120 +10 9.2 the image is virtual and upright. m = (9.2)/(+10) = 0.92. (h) You can't determine r1 , r2 , or n. Upright images have positive magnification. i is found from i = (0.5)(10) = 5; 194
f is found from 1 1 1 1 = + = , f +10 5 10 so the lens is diverging. (h) You can't determine r1 , r2 , or n. Real images have negative magnification. i is found from i = (0.5)(10) = 5; f is found from 1 1 1 1 = + = , f +10 5 +3.33 so the lens is converging. E4029 o + i = 0.44 m = L, so 1 1 1 1 1 L = + = + = , f o i o Lo o(L  o) which can also be written as o2  oL + f L = 0. This has solution o= L (0.44 m) L2  4f L = 2 (0.44 m)  4(0.11 m)(0.44 m) = 0.22 m. 2
There is only one solution to this problem, but sometimes there are two, and other times there are none! E4030 (a) Real images (from real objects) are only produced by converging lenses. (b) Since hi = h0 /2, then i = o/2. But d = i+o = o+o/2 = 3o/2, so o = 2(0.40 m)/3 = 0.267 m, and i = 0.133 m. (c) 1/f = 1/o + 1/i = 1/(0.267 m) + 1/(0.133 m) = 1/(0.0889 m). E4031 Step through the exercise one lens at a time. The object is 40 cm to the left of a converging lens with a focal length of +20 cm. The image from this first lens will be located by solving 1 1 1 1 1 1 =  =  = , i f o (20 cm) (40 cm) 40 cm so i = 40 cm. Since i is positive it is a real image, and it is located to the right of the converging lens. This image becomes the object for the diverging lens. The image from the converging lens is located 40 cm  10 cm from the diverging lens, but it is located on the wrong side: the diverging lens is "in the way" so the rays which would form the image hit the diverging lens before they have a chance to form the image. That means that the real image from the converging lens is a virtual object in the diverging lens, so that the object distance for the diverging lens is o = 30 cm. The image formed by the diverging lens is located by solving 1 1 1 1 1 1 =  =  = , i f o (15 cm) (30 cm) 30 cm or i = 30 cm. This would mean the image formed by the diverging lens would be a virtual image, and would be located to the left of the diverging lens. The image is virtual, so it is upright. The magnification from the first lens is m1 = i/o = (40 cm)/(40 cm)) = 1; 195
the magnification from the second lens is m2 = i/o = (30 cm)/(30 cm)) = 1; which implies an overall magnification of m1 m2 = 1. E4032 (a) The parallel rays of light which strike the lens of focal length f will converge on the focal point. This point will act like an object for the second lens. If the second lens is located a distance L from the first then the object distance for the second lens will be L  f . Note that this will be a negative value for L < f , which means the object is virtual. The image will form at a point 1/i = 1/(f )  1/(L  f ) = L/f (f  L). Note that i will be positive if L < f , so the rays really do converge on a point. (b) The same equation applies, except switch the sign of f . Then 1/i = 1/(f )  1/(L  f ) = L/f (L  f ). This is negative for L < f , so there is no real image, and no converging of the light rays. (c) If L = 0 then i = , which means the rays coming from the second lens are parallel. E4033 The image from the converging lens is found from 1 1 1 1 =  = i1 (0.58 m) (1.12 m) 1.20 m so i1 = 1.20 m, and the image is real and inverted. This real image is 1.97 m  1.20 m = 0.77 m in front of the plane mirror. It acts as an object for the mirror. The mirror produces a virtual image 0.77 m behind the plane mirror. This image is upright relative to the object which formed it, which was inverted relative to the original object. This second image is 1.97 m + 0.77 m = 2.74 m away from the lens. This second image acts as an object for the lens, the image of which is found from 1 1 1 1 =  = i3 (0.58 m) (2.74 m) 0.736 m so i3 = 0.736 m, and the image is real and inverted relative to the object which formed it, which was inverted relative to the original object. So this image is actually upright. E4034 (a) The first lens forms a real image at a location given by 1/i = 1/f  1/o = 1/(0.1 m)  1/(0.2 m) = 1/(0.2 m). The image and object distance are the same, so the image has a magnification of 1. This image is 0.3 m  0.2 m = 0.1 m from the second lens. The second lens forms an image at a location given by 1/i = 1/f  1/o = 1/(0.125 m)  1/(0.1 m) = 1/(0.5 m). Note that this puts the final image at the location of the original object! The image is magnified by a factor of (0.5 m)/(0.1 m) = 5. (c) The image is virtual, but inverted.
196
E4035 If the two lenses "pass" the same amount of light then the solid angle subtended by each lens as seen from the respective focal points must be the same. If we assume the lenses have the same round shape then we can write this as do /f o = de /f e . Then de fo = = m , do fe or de = (72 mm)/36 = 2 mm. E4036 (a) f = (0.25 m)/(200) 1.3 mm. Then 1/f = (n  1)(2/r) can be used to find r; r = 2(n  1)f = 2(1.5  1)(1.3 mm) = 1.3 mm. (b) The diameter would be twice the radius. In effect, these were tiny glass balls. E4037 (a) In Fig. 4046(a) the image is at the focal point. This means that in Fig. 4046(b) i = f = 2.5 cm, even though f = f . Solving, 1 1 1 1 = + = . f (36 cm) (2.5 cm) 2.34 cm (b) The effective radii of curvature must have decreased. E4038 (a) s = (25 cm)  (4.2 cm)  (7.7 cm) = 13.1 cm. (b) i = (25 cm)  (7.7 cm) = 17.3 cm. Then 1 1 1 1 =  = o (4.2 cm) (17.3 cm) 5.54 cm. The object should be placed 5.5  4.2 = 1.34 cm beyond F1 . (c) m = (17.3)/(5.5) = 3.1. (d) m = (25 cm)/(7.7 cm) = 3.2. (e) M = mm = 10. E4039 Microscope magnification is given by Eq. 4033. We need to first find the focal length of the objective lens before we can use this formula. We are told in the text, however, that the microscope is constructed so the at the object is placed just beyond the focal point of the objective lens, then f ob 12.0 mm. Similarly, the intermediate image is formed at the focal point of the eyepiece, so f ey 48.0 mm. The magnification is then m= s(250 mm) (285 mm)(250 mm) = = 124. f ob f ey (12.0 mm)(48.0 mm)
A more accurate answer can be found by calculating the real focal length of the objective lens, which is 11.4 mm, but since there is a huge uncertainty in the near point of the eye, I see no point in trying to be more accurate than this. P401 The old intensity is Io = P/4d2 , where P is the power of the point source. With the mirror in place there is an additional amount of light which needs to travel a total distance of 3d in order to get to the screen, so it contributes an additional P/4(3d)2 to the intensity. The new intensity is then In = P/4d2 + P/4(3d)2 = (10/9)P/4d2 = (10/9)Io .
197
P402
(a) vi = di/dt; but i = f o/(o  f ) and f = r/2 so vi = d dt ro 2o  r = r 2o  r
2
do = dt
r 2o  r
2
vo .
(b) Put in the numbers! vi =  (15 cm) 2(75 cm)  (15 cm)
2
(5.0 cm/s) = 6.2102 cm/s.
(c) Put in the numbers! vi =  (d) Put in the numbers! vi =  (15 cm) 2(0.15 cm)  (15 cm)
2
(15 cm) 2(7.7 cm)  (15 cm)
2
(5.0 cm/s) = 70 m/s
(5.0 cm/s) = 5.2 cm/s.
P403 (b) There are two ends to the object of length L, one of these ends is a distance o1 from the mirror, and the other is a distance o2 from the mirror. The images of the two ends will be located at i1 and i2 . Since we are told that the object has a short length L we will assume that a differential approach to the problem is in order. Then L = o = o1  o2 and L = i = i1  i2 , Finding the ratio of L /L is then reduced to L i di = . L o do We can take the derivative of Eq. 4015 with respect to changes in o and i, di do + 2 = 0, i2 o or L di i2 =  2 = m2 , L do o
where m is the lateral magnification. (a) Since i is given by 1 1 1 of =  = , i f o of the fraction i/o can also be written i of f = = . o o(o  f ) of Then L i2 = o2 f of
2
198
P404 The left surface produces an image which is found from n/i = (n  1)/R  1/o, but since the incoming rays are parallel we take o = and the expression simplifies to i = nR/(n  1). This image is located a distance o = 2R  i = (n  2)R/(n  1) from the right surface, and the image produced by this surface can be found from 1/i = (1  n)/(R)  n/o = (n  1)/R  n(n  1)/(n  2)R = 2(1  n)/(n  2)R. Then i = (n  2)R/2(n  1). P405 The "1" in Eq. 4018 is actually nair ; the assumption is that the thin lens is in the air. If that isn't so, then we need to replace "1" with n , so Eq. 4018 becomes n nn n  = . o i  r1 A similar correction happens to Eq. 4021: n n nn + = . i  i r2 Adding these two equations, n n + = (n  n ) o i This yields a focal length given by 1 nn = f n P406 Start with Eq. 404 1 1 + o i f  f  + o i 1 1 + y y = = 1 , f f  , f 1 1  r1 r2 . 1 1  r1 r2 .
= 1,
where + is when f is positive and  is when f is negative.
The plot on the right is for +, that on the left for . Real image and objects occur when y or y is positive. 199
P407 (a) The image (which will appear on the screen) and object are a distance D = o + i apart. We can use this information to eliminate one variable from Eq. 4015, 1 1 + o i 1 1 + o Do D o(D  o) o2  oD + f D = = = = 1 , f 1 , f 1 , f 0.
This last expression is a quadratic, and we would expect to get two solutions for o. These solutions will be of the form "something" plus/minus "something else"; the distance between the two locations for o will evidently be twice the "something else", which is then d = o+  o = (D)2  4(f D) = D(D  4f ).
(b) The ratio of the image sizes is m+ /m , or i+ o /i o+ . Now it seems we must find the actual values of o+ and o . From the quadratic in part (a) we have o = so the ratio is D D(D  4f ) Dd = , 2 2 Dd D+d .
o = o+
But i = o+ , and viceversa, so the ratio of the image sizes is this quantity squared. P408 1/i = 1/f  1/o implies i = f o/(o  f ). i is only real if o f . The distance between the image and object is of o2 y =i+o= +o= . of of This quantity is a minimum when dy/do = 0, which occurs when o = 2f . Then i = 2f , and y = 4f . P409 (a) The angular size of each lens is the same when viewed from the shared focal point. This means W1 /f1 = W2 /f2 , or W2 = (f2 /f1 )W1 . (b) Pass the light through the diverging lens first; choose the separation of the lenses so that the focal point of the converging lens is at the same location as the focal point of the diverging lens which is on the opposite side of the diverging lens. (c) Since I 1/A, where A is the area of the beam, we have I 1/W 2 . Consequently, I2 /I1 = (W1 /W2 )2 = (f1 /f2 )2 P4010 The location of the image in the mirror is given by 1 1 1 =  . i f a+b
200
The location of the image in the plate is given by i = a, which is located at b  a relative to the mirror. Equating, 1 1 + ba b+a 2b 2  a2 b b2  a2 = = = = 1 , f 1 , f 2bf, b2  2bf , (7.5 cm)2  2(7.5 cm)(28.2 cm) = 21.9 cm.
a =
P4011 We'll solve the problem by finding out what happens if you put an object in front of the combination of lenses. Let the object distance be o1 . The first lens will create an image at i1 , where 1 1 1 =  i1 f1 o1 This image will act as an object for the second lens. If the first image is real (i1 positive) then the image will be on the "wrong" side of the second lens, and as such the real image will act like a virtual object. In short, o2 = i1 will give the correct sign to the object distance when the image from the first lens acts like an object for the second lens. The image formed by the second lens will then be at 1 i2 = = = In this case it appears as if the combination 1 1 + f2 f1 is equivalent to the reciprocal of a focal length. We will go ahead and make this connection, and 1 1 1 f1 + f2 = + = . f f2 f1 f1 f2 The rest is straightforward enough. P4012 (a) The image formed by the first lens can be found from 1 1 1 1 =  = . i1 f1 2f1 2f1 This is a distance o2 = 2(f1 + f2 ) = 2f2 from the mirror. The image formed by the mirror is at an image distance given by 1 1 1 1 =  = . i2 f2 2f2 2f2 Which is at the same point as i1 !. This means it will act as an object o3 in the lens, and, reversing the first step, produce a final image at O, the location of the original object. There are then three images formed; each is real, same size, and inverted. Three inversions nets an inverted image. The final image at O is therefore inverted. 201 1 1  , f2 o2 1 1 + , f2 i2 1 1 1 +  . f2 f1 o1
P4013
(a) Place an object at o. The image will be at a point i given by 1 1 1 =  , i f o
or i = f o/(o  f ). (b) The lens must be shifted a distance i  i, or i i= (c) The range of motion is i = (0.05 m)(1.2 m)  1 = 5.2 cm. (1.2 m)  (0.05 m) fo  1. of
P4014 (a) Because magnification is proportional to 1/f . (b) Using the results of Problem 4011, 1 1 1 = + , f f2 f1 so P = P1 + P2 . P4015 We want the maximum linear motion of the train to move no more than 0.75 mm on the film; this means we want to find the size of an object on the train that will form a 0.75 mm image. The object distance is much larger than the focal length, so the image distance is approximately equal to the focal length. The magnification is then m = i/o = (3.6 cm)/(44.5 m) = 0.00081. The size of an object on the train that would produce a 0.75 mm image on the film is then 0.75 mm/0.00081 = 0.93 m. How much time does it take the train to move that far? t= (0.93 m) = 25 ms. (135 km/hr)(1/3600 hr/s)
P4016 (a) The derivation leading to Eq. 4034 depends only on the fact that two converging optical devices are used. Replacing the objective lens with an objective mirror doesn't change anything except the ray diagram. (b) The image will be located very close to the focal point, so m f /o, and hi = (1.0 m) (16.8 m) = 8.4103 m (2000 m)
(c) f e = (5 m)/(200) = 0.025 m. Note that we were given the radius of curvature, not the focal length, of the mirror!
202
E411
In this problem we look for the location of the thirdorder bright fringe, so = sin1 m (3)(554 109 m) = sin1 = 12.5 = 0.22 rad. d (7.7 106 m)
E412 d1 sin = gives the first maximum; d2 sin = 2 puts the second maximum at the location of the first. Divide the second expression by the first and d2 = 2d1 . This is a 100% increase in d. E413 y = D/d = (512109 m)(5.4 m)/(1.2103 m) = 2.3103 m. E414 d = / sin = (592109 m)/ sin(1.00 ) = 3.39105 m. E415 Since the angles are very small, we can assume sin for angles measured in radians. If the interference fringes are 0.23 apart, then the angular position of the first bright fringe is 0.23 away from the central maximum. Eq. 411, written with the small angle approximation in mind, is d = for this first (m = 1) bright fringe. The goal is to find the wavelength which increases by 10%. To do this we must increase the right hand side of the equation by 10%, which means increasing by 10%. The new wavelength will be = 1.1 = 1.1(589 nm) = 650 nm E416 Immersing the apparatus in water will shorten the wavelengths to /n. Start with d sin 0 = ; and then find from d sin = /n. Combining the two expressions, = arcsin[sin 0 /n] = arcsin[sin(0.20 )/(1.33)] = 0.15 . E417 The thirdorder fringe for a wavelength will be located at y = 3D/d, where y is measured from the central maximum. Then y is y1  y2 = 3(1  2 )D/d = 3(612109 m  480109 m)(1.36 m)/(5.22103 m) = 1.03104 m. E418 = arctan(y/D); = d sin = (0.120 m) sin[arctan(0.180 m/2.0 m)] = 1.08102 m. Then f = v/ = (0.25 m/s)/(1.08102 m) = 23 Hz. E419 A variation of Eq. 413 is in order: ym = m+ 1 2 D d
We are given the distance (on the screen) between the first minima (m = 0) and the tenth minima (m = 9). Then (50 cm) 18 mm = y9  y0 = 9 , (0.15 mm) or = 6104 mm = 600 nm. E4110 The "maximum" maxima is given by the integer part of m = d sin(90 )/ = (2.0 m)/(0.50 m) = 4. Since there is no integer part, the "maximum" maxima occurs at 90 . These are point sources radiating in both directions, so there are two central maxima, and four maxima each with m = 1, m = 2, and m = 3. But the m = 4 values overlap at 90 , so there are only two. The total is 16. 203
E4111
This figure should explain it well enough.
E4112 y = D/d = (589109 m)(1.13 m)/(0.18103 m) = 3.70103 m. E4113 Consider Fig. 415, and solve it exactly for the information given. For the tenth bright fringe r1 = 10 + r2 . There are two important triangles:
2 r2 = D2 + (y  d/2)2
and
2 r1 = D2 + (y + d/2)2
Solving to eliminate r2 , D2 + (y + d/2)2 = This has solution y = 5 The solution predicted by Eq. 411 is y = or y = 5 The fractional error is y /y  1, or 4D2  1, + d2  1002 d2 4D2 .  1002 10 d D2 + y 2 , 4D2 + d2  1002 . d2  1002 D2 + (y  d/2)2 + 10.
4D2 or
4(40 mm)2  1 = 3.1104 . 4(40 mm)2 + (2 mm)2  100(589106 mm)2 E4114 (a) x = c/t = (3.00108 m/s)/(1108 s) = 3 m. (b) No.
204
E4115 Leading by 90 is the same as leading by a quarter wavelength, since there are 360 in a circle. The distance from A to the detector is 100 m longer than the distance from B to the detector. Since the wavelength is 400 m, 100 m corresponds to a quarter wavelength. So a wave peak starts out from source A and travels to the detector. When it has traveled a quarter wavelength a wave peak leaves source B. But when the wave peak from A has traveled a quarter wavelength it is now located at the same distance from the detector as source B, which means the two wave peaks arrive at the detector at the same time. They are in phase. E4116 The first dark fringe involves waves radians out of phase. Each dark fringe after that involves an additional 2 radians of phase difference. So the mth dark fringe has a phase difference of (2m + 1) radians. E4117 I = 4I0 cos2
2d
sin , so for this problem we want to plot 2(0.60 mm) sin (600109 m) = cos2 (6280 sin ) .
I/I0 = cos2
E4118 The resultant quantity will be of the form A sin(t + ). Solve the problem by looking at t = 0; then y1 = 0, but x1 = 10, and y2 = 8 sin 30 = 4 and x2 = 8 cos 30 = 6.93. Then the resultant is of length A = (4)2 + (10 + 6.93)2 = 17.4, and has an angle given by = arctan(4/16.93) = 13.3 . E4119 (a) We want to know the path length difference of the two sources to the detector. Assume the detector is at x and the second source is at y = d. The distance S1 D is x; the distance S2 D is x2 + d2 . The difference is x2 + d2  x. If this difference is an integral number of wavelengths then we have a maximum; if instead it is a half integral number of wavelengths we have a minimum. For part (a) we are looking for the maxima, so we set the path length difference equal to m and solve for xm . x2 + d2  xm m x2 + d2 m x2 + d2 m xm = m, = (m + xm )2 , = m2 2 + 2mxm + x2 , m d 2  m2 2 = 2m
The first question we need to ask is what happens when m = 0. The right hand side becomes indeterminate, so we need to go back to the first line in the above derivation. If m = 0 then d2 = 0; since this is not true in this problem, there is no m = 0 solution. In fact, we may have even more troubles. xm needs to be a positive value, so the maximum allowed value for m will be given by m2 2 < d2 , m < d/ = (4.17 m)/(1.06 m) = 3.93; but since m is an integer, m = 3 is the maximum value.
205
The first three maxima occur at m = 3, m = 2, and m = 1. These maxima are located at x3 x2 x1 = = = (4.17 m)2  (3)2 (1.06 m)2 = 1.14 m, 2(3)(1.06 m) (4.17 m)2  (2)2 (1.06 m)2 = 3.04 m, 2(2)(1.06 m) (4.17 m)2  (1)2 (1.06 m)2 = 7.67 m. 2(1)(1.06 m)
Interestingly enough, as m decreases the maxima get farther away! (b) The closest maxima to the origin occurs at x = 6.94 cm. What then is x = 0? It is a local minimum, but the intensity isn't zero. It corresponds to a point where the path length difference is 3.93 wavelengths. It should be half an integer to be a complete minimum. E4120 The resultant can be written in the form A sin(t + ). Consider t = 0. The three components can be written as y1 y2 y3 y and x1 x2 x3 x Then A = = 10 cos 0 = 10, = 14 cos 26 = 12.6, = 4.7 cos(41 ) = 3.55, = 10 + 12.6 + 3.55 = 26.2. = = = = 10 sin 0 = 0, 14 sin 26 = 6.14, 4.7 sin(41 ) = 3.08, 0 + 6.14  3.08 = 3.06.
(3.06)2 + (26.2)2 = 26.4 and = arctan(3.06/26.2) = 6.66 .
E4121 The order of the indices of refraction is the same as in Sample Problem 414, so d = /4n = (620 nm)/4(1.25) = 124 nm. E4122 Follow the example in Sample Problem 413. = 2dn 2(410 nm)(1.50) 1230 nm = = . m  1/2 m  1/2 m  1/2
The result is only in the visible range when m = 3, so = 492 nm. E4123 (a) Light from above the oil slick can be reflected back up from the top of the oil layer or from the bottom of the oil layer. For both reflections the light is reflecting off a substance with a higher index of refraction so both reflected rays pick up a phase change of . Since both waves have this phase the equation for a maxima is 1 1 2d + n + n = mn . 2 2 Remember that n = /n, where n is the index of refraction of the thin film. Then 2nd = (m  1) is the condition for a maxima. We know n = 1.20 and d = 460 nm. We don't know m or . It might 206
seem as if there isn't enough information to solve the problem, but we can. We need to find the wavelength in the visible range (400 nm to 700 nm) which has an integer m. Trial and error might work. If = 700 nm, then m is m= 2nd 2(1.20)(460 nm) +1= + 1 = 2.58 (700 nm)
But m needs to be an integer. If we increase m to 3, then = 2(1.20)(460 nm) = 552 nm (3  1)
which is in the visible range. So the oil slick will appear green. (b) One of the most profound aspects of thin film interference is that wavelengths which are maximally reflected are minimally transmitted, and vice versa. Finding the maximally transmitted wavelengths is the same as finding the minimally reflected wavelengths, or looking for values of m that are half integer. The most obvious choice is m = 3.5, and then = 2(1.20)(460 nm) = 442 nm. (3.5  1)
E4124 The condition for constructive interference is 2nd = (m  1/2). Assuming a minimum value of m = 1 one finds d = /4n = (560 nm)/4(2.0) = 70 nm. E4125 The top surface contributes a phase difference of , so the phase difference because of the thickness is 2, or one complete wavelength. Then 2d = /n, or d = (572 nm)/2(1.33) = 215 nm. E4126 The wave reflected from the first surface picks up a phase shift of . The wave which is reflected off of the second surface travels an additional path difference of 2d. The interference will be bright if 2d + n /2 = mn results in m being an integer. m = 2nd/ + 1/2 = 2(1.33)(1.21106 m)/(585109 m) + 1/2 = 6.00, so the interference is bright. E4127 As with the oil on the water in Ex. 4123, both the light which reflects off of the acetone and the light which reflects off of the glass undergoes a phase shift of . Then the maxima for reflection are given by 2nd = (m  1). We don't know m, but at some integer value of m we have = 700 nm. If m is increased by exactly 1 then we are at a minimum of = 600 nm. Consequently, 2 2(1.25)d = (m  1)(700 nm) and 2(1.25)d = (m  1/2)(600 nm), we can set these two expressions equal to each other to find m, (m  1)(700 nm) = (m  1/2)(600 nm), so m = 4. Then we can find the thickness, d = (4  1)(700 nm)/2(1.25) = 840 nm.
207
E4128 The wave reflected from the first surface picks up a phase shift of . The wave which is reflected off of the second surface travels an additional path difference of 2d. The interference will be bright if 2d + n /2 = mn results in m being an integer. Then 2nd = (m  1/2)1 is bright, and 2nd = m2 is dark. Divide one by the other and (m  1/2)1 = m2 , so m = 1 /2(1  2 ) = (600 nm)/2(600 nm  450 nm) = 2, then d = m2 /2n = (2)(450 nm)/2(1.33) = 338 nm. E4129 Constructive interference happens when 2d = (m  1/2). The minimum value for m is m = 1; the maximum value is the integer portion of 2d/+1/2 = 2(4.8105 m)/(680109 m)+1/2 = 141.67, so mmax = 141. There are then 141 bright bands. E4130 (a) A half wavelength phase shift occurs for both the air/water interface and the water/oil interface, so if d = 0 the two reflected waves are in phase. It will be bright! (b) 2nd = 3, or d = 3(475 nm)/2(1.20) = 594 nm. E4131 There is a phase shift on one surface only, so the bright bands are given by 2nd = (m  1/2). Let the first band be given by 2nd1 = (m1  1/2). The last bright band is then given by 2nd2 = (m1 + 9  1/2). Subtract the two equations to get the change in thickness: d = 9/2n = 9(630 nm)/2(1.50) = 1.89 m. E4132 Apply Eq. 4121: 2nd = m. In one case we have 2nair = (4001), in the other, 2nvac = (4000). Equating, nair = (4001)/(4000) = 1.00025. E4133 (a) We can start with the last equation from Sample Problem 415, r= and solve for m, r2 1 + R 2 In this exercise R = 5.0 m, r = 0.01 m, and = 589 nm. Then m= m= (0.01 m)2 = 34 (589 nm)(5.0 m) 1 (m  )R, 2
is the number of rings observed. (b) Putting the apparatus in water effectively changes the wavelength to (589 nm)/(1.33) = 443 nm, so the number of rings will now be m= (0.01 m)2 = 45. (443 nm)(5.0 m) 208
(10  1 )R, while (1.27 cm) = 2 the other, and (1.42 cm)/(1.27 cm) = n, or n = 1.25. E4134 (1.42 cm) = E4135 (0.162 cm) = (n  1 )R, while (0.368 cm) = 2 sions, the divide one by the other, and find
(10  1 )R/n. Divide one expression by 2
(n + 20  1 )R. Square both expres2
(n + 19.5)/(n  0.5) = (0.368 cm/0.162 cm)2 = 5.16 which can be rearranged to yield n= 19.5 + 5.16 0.5 = 5.308. 5.16  1
Oops! That should be an integer, shouldn't it? The above work is correct, which means that there really aren't bright bands at the specified locations. I'm just going to gloss over that fact and solve for R using the value of m = 5.308. Then R = r2 /(m  1/2) = (0.162 cm)2 /(5.308  0.5)(546 nm) = 1.00 m. Well, at least we got the answer which is in the back of the book... E4136 Pretend the ship is a two point source emitter, one h above the water, and one h below the water. The one below the water is out of phase by half a wavelength. Then d sin = , where d = 2h, gives the angle for theta for the first minimum. /2h = (3.43 m)/2(23 m) = 7.46102 = sin H/D, so D = (160 m)/(7.46102 ) = 2.14 km. E4137 The phase difference is 2/n times the path difference which is 2d, so = 4d/n = 4nd/. We are given that d = 100109 m and n = 1.38. (a) = 4(1.38)(100109 m)/(450109 m) = 3.85. Then (3.85) I = cos2 = 0.12. I0 2 The reflected ray is diminished by 1  0.12 = 88%. (b) = 4(1.38)(100109 m)/(650109 m) = 2.67. Then I (2.67) = cos2 = 0.055. I0 2 The reflected ray is diminished by 1  0.055 = 95%. E4138 The change in the optical path length is 2(d  d/n), so 7/n = 2d(1  1/n), or d= 7(589109 m) = 4.9106 m. 2(1.42)  2
209
E4139 When M2 moves through a distance of /2 a fringe has will be produced, destroyed, and then produced again. This is because the light travels twice through any change in distance. The wavelength of light is then 2(0.233 mm) = 588 nm. = 792 E4140 The change in the optical path length is 2(d  d/n), so 60 = 2d(1  1/n), or n= 1 1 = = 1.00030. 9 m)/2(5102 m) 1  60/2d 1  60(50010
P411 (a) This is a small angle problem, so we use Eq. 414. The distance to the screen is 2 20 m, because the light travels to the mirror and back again. Then d= D (632.8 nm)(40.0 m) = = 0.253 mm. y (0.1 m)
(b) Placing the cellophane over one slit will cause the interference pattern to shift to the left or right, but not disappear or change size. How does it shift? Since we are picking up 2.5 waves then we are, in effect, swapping bright fringes for dark fringes. P412 The change in the optical path length is d  d/n, so 7/n = d(1  1/n), or d= 7(550109 m) = 6.64106 m. (1.58)  1
P413 The distance from S1 to P is r1 = (x + d/2)2 + y 2 . The distance from S2 to P is 2 + y 2 . The difference in distances is fixed at some value, say c, so that r2 = (x  d/2) r 1  r2 2  2r1 r2 + r2 2 2 (r1 + r2  c2 )2 2 2 2 2 2 2 (r1  r2 )  2c (r1 + r2 ) + c4 (2xd)2  2c2 (2x2 + d2 /2 + 2y 2 ) + c4 4x2 d2  4c2 x2  c2 d2  4c2 y 2 + c4 4(d2  c2 )x2  4c2 y 2
2 r1
= = = = = = =
c, c2 , 2 2 4r1 r2 , 0, 0, 0, c2 (d2  c2 ).
Yes, that is the equation of a hyperbola. P414 The change in the optical path length for each slit is nt  t, where n is the corresponding index of refraction. The net change in the path difference is then n2 t  n1 t. Consequently, m = t(n2  n1 ), so (5)(480109 m) t= = 8.0106 m. (1.7)  (1.4) P415 The intensity is given by Eq. 4117, which, in the small angle approximation, can be written as d I = 4I0 cos2 .
210
The intensity will be half of the maximum when 1 = cos2 2 or d/2
d = , 4 2
which will happen if = /2d. P416 Follow the construction in Fig. 4110, except that one of the electric field amplitudes is twice the other. The resultant field will have a length given by E = (2E0 + E0 cos )2 + (E0 sin )2 , 5 + 4 cos ,
= E0 so squaring this yields I
2d sin , d sin = I0 1 + 8 cos2 , Im d sin = 1 + 8 cos2 . 9 = I0 5 + 4 cos
P417 mum is
We actually did this problem in Exercise 4127, although slightly differently. One maxi2(1.32)d = (m  1/2)(679 nm),
the other is 2(1.32)d = (m + 1/2)(485 nm). Set these equations equal to each other, (m  1/2)(679 nm) = (m + 1/2)(485 nm), and find m = 3. Then the thickness is d = (3  1/2)(679 nm)/2(1.32) = 643 nm. P418 (a) Since we are concerned with transmission there is a phase shift for two rays, so 2d = mn The minimum thickness occurs when m = 1; solving for d yields d= (525109 m) = = 169109 m. 2n 2(1.55)
(b) The wavelengths are different, so the other parts have differing phase differences. (c) The nearest destructive interference wavelength occurs when m = 1.5, or = 2nd = 2(1.55)1.5(169109 m) = 393109 m. This is blueviolet. 211
P419 It doesn't matter if we are looking at bright are dark bands. It doesn't even matter if we concern ourselves with phase shifts. All that cancels out. Consider 2d = m; then d = (10)(480 nm)/2 = 2.4 m. P4110 (a) Apply 2d = m. Then d = (7)(600109 m)/2 = 2100109 m. (b) When water seeps in it introduces an extra phase shift. Point A becomes then a bright fringe, and the equation for the number of bright fringes is 2nd = m. Solving for m, m = 2(1.33)(2100109 m)/(600109 m) = 9.3; this means that point B is almost, but not quite, a dark fringe, and there are nine of them. P4111 (a) Look back at the work for Sample Problem 415 where it was found rm = We can write this as rm = 1 1 2m mR 1 (m  )R, 2
and expand the part in parentheses in a binomial expansion, 1 1 rm 1  mR. 2 2m We will do the same with rm+1 = expanding rm+1 = to get rm+1 Then r or r 1+ 1 1 2 2m 1+ 1 2m mR 1 (m + 1  )R, 2
mR.
1 mR, 2m
1 R/m. 2 (b) The area between adjacent rings is found from the difference,
2 2 A = rm+1  rm ,
and into this expression we will substitute the exact values for rm and rm+1 , 1 1 A = (m + 1  )R  (m  )R , 2 2 = R. Unlike part (a), we did not need to assume m for all m. 1 in order to arrive at this expression; it is exact
212
P4112 The path length shift that occurs when moving the mirror as distance x is 2x. This means = 22x/ = 4x/. The intensity is then I = 4I0 cos2 2x
213
E421 = a sin = (0.022 mm) sin(1.8 ) = 6.91107 m. E422 a = / sin = (0.10109 m)/ sin(0.12103 rad/2) = 1.7 m. E423 (a) This is a valid small angle approximation problem: the distance between the points on the screen is much less than the distance to the screen. Then (0.0162 m) = 7.5 103 rad. (2.16 m)
(b) The diffraction minima are described by Eq. 423, a sin = m, a sin(7.5 10 rad) = (2)(441 109 m), a = 1.18 104 m.
3
E424 a = / sin = (633109 m)/ sin(1.97 /2) = 36.8 m. E425 (a) We again use Eq. 423, but we will need to throw in a few extra subscripts to distinguish between which wavelength we are dealing with. If the angles match, then so will the sine of the angles. We then have sin a,1 = sin b,2 or, using Eq. 423, (1)a (2)b = , a a from which we can deduce a = 2b . (b) Will any other minima coincide? We want to solve for the values of ma and mb that will be integers and have the same angle. Using Eq. 423 one more time, mb b ma a = , a a and then substituting into this the relationship between the wavelengths, ma = mb /2. whenever mb is an even integer ma is an integer. Then all of the diffraction minima from a are overlapped by a minima from b . E426 The angle is given by sin = 2/a. This is a small angle, so we can use the small angle approximation of sin = y/D. Then y = 2D/a = 2(0.714 m)(593109 m)/(420106 m) = 2.02 mm. E427 Small angles, so y/D = sin = /a. Then a = D/y = (0.823 m)(546109 m)/(5.20103 m/2) = 1.73104 m. E428 (b) Small angles, so y/D = m/a. Then a = mD/y = (5  1)(0.413 m)(546109 m)/(0.350103 m) = 2.58 mm. (a) = arcsin(/a) = arcsin[(546109 m)/(2.58 mm)] = 1.21102 . E429 Small angles, so y/D = m/a. Then y = mD/a = (2  1)(2.94 m)(589109 m)/(1.16103 m) = 1.49103 m. 214
E4210 Doubling the width of the slit results in a narrowing of the diffraction pattern. Since the width of the central maximum is effectively cut in half, then there is twice the energy in half the space, producing four times the intensity. E4211 (a) This is a small angle approximation problem, so = (1.13 cm)/(3.48 m) = 3.25 103 rad. (b) A convenient measure of the phase difference, is related to through Eq. 427, = (25.2 106 m) a sin(3.25 103 rad) = 0.478 rad sin = (538 109 m)
(c) The intensity at a point is related to the intensity at the central maximum by Eq. 428, I = Im sin
2
=
sin(0.478 rad) (0.478 rad)
2
= 0.926
E4212 Consider Fig. 4211; the angle with the vertical is given by (  )/2. For Fig. 4210(d) the circle has wrapped once around onto itself so the angle with the vertical is (3 )/2. Substitute into this expression and the angel against the vertical is 3/2  . Use the result from Problem 423 that tan = for the maxima. The lowest nonzero solution is = 4.49341 rad. The angle against the vertical is then 0.21898 rad, or 12.5 . E4213 Drawing heavily from Sample Problem 424, x = arcsin Finally, = 2x = 5.1 . E4214 (a) Rayleigh's criterion for resolving images (Eq. 4211) requires that two objects have an angular separation of at least R = sin1 1.22 d = sin1 1.22(540 109 ) (4.90 103 m) = 1.34 104 rad x a = arcsin 1.39 10 = 2.54 .
(b) The linear separation is y = D = (1.34 104 rad)(163103 m) = 21.9 m. E4215 (a) Rayleigh's criterion for resolving images (Eq. 4211) requires that two objects have an angular separation of at least R = sin1 1.22 d = sin1 1.22(562 109 ) (5.00 103 m) = 1.37 104 rad.
(b) Once again, this is a small angle, so we can use the small angle approximation to find the distance to the car. In that case R = y/D, where y is the headlight separation and D the distance to the car. Solving, D = y/R = (1.42 m)/(1.37 104 rad) = 1.04 104 m, or about six or seven miles. 215
E4216 y/D = 1.22/a; or D = (5.20103 m)(4.60103 /m)/1.22(542109 m) = 36.2 m. E4217 The smallest resolvable angular separation will be given by Eq. 4211, R = sin1 1.22 d = sin1 1.22(565 109 m) (5.08 m) = 1.36 107 rad,
The smallest objects resolvable on the Moon's surface by this telescope have a size y where y = DR = (3.84 108 m)(1.36 107 rad) = 52.2 m E4218 y/D = 1.22/a; or y = 1.22(1.57102 m)(6.25103 m)/(2.33 m) = 51.4 m E4219 y/D = 1.22/a; or D = (4.8102 m)(4.3103 /m)/1.22(0.12109 m) = 1.4106 m. E4220 y/D = 1.22/a; or d = 1.22(550109 m)(160103 m)/(0.30 m) = 0.36 m. E4221 Using Eq. 4211, we find the minimum resolvable angular separation is given by R = sin1 1.22 d = sin1 1.22(475 109 m) (4.4 103 m) = 1.32 104 rad
The dots are 2 mm apart, so we want to stand a distance D away such that D > y/R = (2 103 m)/(1.32 104 rad) = 15 m. E4222 y/D = 1.22/a; or y = 1.22(500109 m)(354103 m)/(9.14 m/2) = 4.73102 m. E4223 (a) = v/f . Now use Eq. 4211: = arcsin 1.22 (b) Following the same approach, = arcsin 1.22 has no real solution, so there is no minimum. (1450 m/s) (1103 Hz)(0.60 m) (1450 m/s) (25103 Hz)(0.60 m) = 6.77 .
216
E4224 (a) = v/f . Now use Eq. 4211: = arcsin 1.22 (3108 m/s) (220109 Hz)(0.55 m) = 0.173 .
This is the angle from the central maximum; the angular width is twice this, or 0.35 . (b) use Eq. 4211: (0.0157 m) = arcsin 1.22 = 0.471 . (2.33 m) This is the angle from the central maximum; the angular width is twice this, or 0.94 . E4225 The linear separation of the fringes is given by y D = = or y = D d d for sufficiently small d compared to . E4226 (a) d sin = 4 gives the location of the fourth interference maximum, while a sin = gives the location of the first diffraction minimum. Hence, if d = 4a there will be no fourth interference maximum! (b) Since d sin mi = mi gives the interference maxima and a sin md = md gives the diffraction minima, and d = 4a, then whenever mi = 4md there will be a missing maximum. E4227 (a) The central diffraction envelope is contained in the range = arcsin a
This angle corresponds to the mth maxima of the interference pattern, where sin = m/d = m/2a. Equating, m = 2, so there are three interference bands, since the m = 2 band is "washed out" by the diffraction minimum. (b) If d = a then = and the expression reduces to I = I m cos2 sin2 , 2 sin2 (2) = Im , 22 2 sin = 2I m ,
where = 2 , which is the same as replacing a by 2a. E4228 Remember that the central peak has an envelope width twice that of any other peak. Ignoring the central maximum there are (11  1)/2 = 5 fringes in any other peak envelope.
217
E4229 (a) The first diffraction minimum is given at an angle such that a sin = ; the order of the interference maximum at that point is given by d sin = m. Dividing one expression by the other we get d/a = m, with solution m = (0.150)/(0.030) = 5. The fact that the answer is exactly 5 implies that the fifth interference maximum is squelched by the diffraction minimum. Then there are only four complete fringes on either side of the central maximum. Add this to the central maximum and we get nine as the answer. (b) For the third fringe m = 3, so d sin = 3. Then is Eq. 4214 is 3, while in Eq. 4216 is a a 3 = = 3 , d d so the relative intensity of the third fringe is, from Eq. 4217, (cos 3)2 P421 y = mD/a. Then y = (10)(632.8109 m)(2.65 m)/(1.37103 m) = 1.224102 m. The separation is twice this, or 2.45 cm. P422 If a then the diffraction pattern is extremely tight, and there is effectively no light at P . In the event that either shape produces an interference pattern at P then the other shape must produce an equal but opposite electric field vector at that point so that when both patterns from both shapes are superimposed the field cancel. But the intensity is the field vector squared; hence the two patterns look identical. P423 (a) We want to take the derivative of Eq. 428 with respect to , so dI d = sin , sin cos sin = I m2  2 sin = I m 2 3 ( cos  sin ) . d Im d
2
sin(3a/d) (3a/d)
2
= 0.255.
,
This equals zero whenever sin = 0 or cos = sin ; the former is the case for a minima while the latter is the case for the maxima. The maxima case can also be written as tan = . (b) Note that as the order of the maxima increases the solutions get closer and closer to odd integers times /2. The solutions are = 0, 1.43, 2.46, etc. (c) The m values are m = /  1/2, and correspond to m = 0.5, 0.93, 1.96, etc. These values will get closer and closer to integers as the values are increased.
218
P424
The outgoing beam strikes the moon with a circular spot of radius r = 1.22D/a = 1.22(0.69106 m)(3.82108 m)/(2 1.3 m) = 123 m.
The light is not evenly distributed over this circle. If P0 is the power in the light, then
R
P0 =
I r dr d = 2
0
I r dr, we can write
where R is the radius of the central peak and I is the angular intensity. For a ar/D, then P0 = 2Im D a
2 0 /2
sin2 d 2Im
D a
2
(0.82).
Then the intensity at the center falls off with distance D as Im = 1.9 (a/D) P0 The fraction of light collected by the mirror on the moon is then P1 /P0 = 1.9 (2 1.3 m) (0.69106 m)(3.82108 m)
2 2
(0.10 m)2 = 5.6106 .
The fraction of light collected by the mirror on the Earth is then P2 /P1 = 1.9 Finally, P2 /P0 = 31011 . P425 (a) The ring is reddish because it occurs at the blue minimum. (b) Apply Eq. 4211 for blue light: d = 1.22/ sin = 1.22(400 nm)/ sin(0.375 ) = 70 m. (c) Apply Eq. 4211 for red light: = arcsin (1.22(700 nm)/(70 m)) 0.7 , which occurs 3 lunar radii from the moon. P426 The diffraction pattern is a property of the speaker, not the interference between the speakers. The diffraction pattern should be unaffected by the phase shift. The interference pattern, however, should shift up or down as the phase of the second speaker is varied. P427 (a) The missing fringe at = 5 is a good hint as to what is going on. There should be some sort of interference fringe, unless the diffraction pattern has a minimum at that point. This would be the first minimum, so a sin(5 ) = (440 109 m) would be a good measure of the width of each slit. Then a = 5.05 106 m. (2 0.10 m) (0.69106 m)(3.82108 m)
2
(1.3 m)2 = 5.6106 .
219
(b) If the diffraction pattern envelope were not present we could expect that the fourth interference maxima beyond the central maximum would occur at this point, and then d sin(5 ) = 4(440 109 m) yielding d = 2.02 105 m. (c) Apply Eq. 4217, where = m and = Then for m = 1 we have I1 = (7) while for m = 2 we have I2 = (7) These are in good agreement with the figure. sin(2/4) (2/4) sin(/4) (/4) a m a a sin = =m = m/4. d d
2
= 5.7;
2
= 2.8.
220
E431 (a) d = (21.5103 m)/(6140) = 3.50106 m. (b) There are a number of angles allowed: = = = = = arcsin[(1)(589109 m)/(3.50106 m)] = 9.7 , arcsin[(2)(589109 m)/(3.50106 m)] = 19.5 , arcsin[(3)(589109 m)/(3.50106 m)] = 30.3 , arcsin[(4)(589109 m)/(3.50106 m)] = 42.3 , arcsin[(5)(589109 m)/(3.50106 m)] = 57.3 .
E432 The distance between adjacent rulings is d= The number of lines is then N = D/d = (2.86102 m)/(2.235106 m) = 12, 800. E433 We want to find a relationship between the angle and the order number which is linear. We'll plot the data in this representation, and then use a least squares fit to find the wavelength. The data to be plotted is m 1 2 3 17.6 37.3 65.2 sin 0.302 0.606 0.908 m 1 2 3 17.6 37.1 65.0 sin 0.302 0.603 0.906 (2)(612109 m) = 2.235106 m. sin(33.2 )
On my calculator I get the best straight line fit as 0.302m + 8.33 104 = sin m , which means that = (0.302)(1.73 m) = 522 nm. E434 Although an approach like the solution to Exercise 3 should be used, we'll assume that each measurement is perfect and error free. Then randomly choosing the third maximum, = d sin (5040109 m) sin(20.33 ) = = 586109 m. m (3)
E435
(a) The principle maxima occur at points given by Eq. 431, sin m = m . d
The difference of the sine of the angle between any two adjacent orders is sin m+1  sin m = (m + 1) Using the information provided we can find d from d= (600 109 ) = = 6 m. sin m+1  sin m (0.30)  (0.20) 221 m = . d d d
It doesn't take much imagination to recognize that the second and third order maxima were given. (b) If the fourth order maxima is missing it must be because the diffraction pattern envelope has a minimum at that point. Any fourth order maxima should have occurred at sin 4 = 0.4. If it is a diffraction minima then a sin m = m where sin m = 0.4 We can solve this expression and find a=m (600 109 m) =m = m1.5 m. sin m (0.4)
The minimum width is when m = 1, or a = 1.5 m. (c) The visible orders would be integer values of m except for when m is a multiple of four. E436 (a) Find the maximum integer value of m = d/ = (930 nm)/(615 nm) = 1.5, hence m = 1, 0, +1; there are three diffraction maxima. (b) The first order maximum occurs at = arcsin(615 nm)/(930 nm) = 41.4 . The width of the maximum is = or 0.0451 . E437 The fifth order maxima will be visible if d/ 5; this means d (1103 m) = = 635109 m. 5 (315 rulings)(5) (615 nm) = 7.87104 rad, (1120)(930 nm) cos(41.4 )
E438 (a) The maximum could be the first, and then = (1103 m) sin(28 ) d sin = = 2367109 m. m (200)(1)
That's not visible. The first visible wavelength is at m = 4, then = The next is at m = 5, then = d sin (1103 m) sin(28 ) = = 469109 m. m (200)(5) d sin (1103 m) sin(28 ) = = 589109 m. m (200)(4)
Trying m = 6 results in an ultraviolet wavelength. (b) Yelloworange and blue.
222
E439
A grating with 400 rulings/mm has a slit separation of d= 1 = 2.5 103 mm. 400 mm1
To find the number of orders of the entire visible spectrum that will be present we need only consider the wavelength which will be on the outside of the maxima. That will be the longer wavelengths, so we only need to look at the 700 nm behavior. Using Eq. 431, d sin = m, and using the maximum angle 90 , we find m< (2.5 106 m) d = = 3.57, (700 109 m)
so there can be at most three orders of the entire spectrum. E4310 In this case d = 2a. Since interference maxima are given by sin = m/d while diffraction minima are given at sin = m /a = 2m /d then diffraction minima overlap with interference maxima whenever m = 2m . Consequently, all even m are at diffraction minima and therefore vanish. E4311 If the secondorder spectra overlaps the thirdorder, it is because the 700 nm secondorder line is at a larger angle than the 400 nm thirdorder line. Start with the wavelengths multiplied by the appropriate order parameter, then divide both side by d, and finally apply Eq. 431. 2(700 nm) > 3(400 nm), 2(700 nm) 3(400 nm) > , d d sin 2,=700 > sin 3,=400 , regardless of the value of d. E4312 Fig. 322 shows the path length difference for the right hand side of the grating as d sin . If the beam strikes the grating at ang angle then there will be an additional path length difference of d sin on the right hand side of the figure. The diffraction pattern then has two contributions to the path length difference, these add to give d(sin + sin psi) = m. E4313 E4314 Let d sin i = i and 1 + 20 = 2 . Then sin 2 = sin 1 cos(20 ) + cos 1 sin(20 ). Rearranging, sin 2 = sin 1 cos(20 ) + 1  sin2 1 sin(20 ).
Substituting the equations together yields a rather nasty expression, 2 1 = cos(20 ) + d d 1  (1 /d)2 sin(20 ). 223
Rearranging, (2  1 cos(20 )) = d2  2 sin2 (20 ). 1 Use 1 = 430 nm and 2 = 680 nm, then solve for d to find d = 914 nm. This corresponds to 1090 rulings/mm. E4315 The shortest wavelength passes through at an angle of 1 = arctan(50 mm)/(300 mm) = 9.46 . This corresponds to a wavelength of 1 = (1103 m) sin(9.46 ) = 470109 m. (350)
2
The longest wavelength passes through at an angle of 2 = arctan(60 mm)/(300 mm) = 11.3 . This corresponds to a wavelength of 2 = (1103 m) sin(11.3 ) = 560109 m. (350)
E4316 (a) = /R = /N m, so = (481 nm)/(620 rulings/mm)(5.05 mm)(3) = 0.0512 nm. (b) mm is the largest integer smaller than d/, or mm 1/(481109 m)(620 rulings/mm) = 3.35, so m = 3 is highest order seen. E4317 The required resolving power of the grating is given by Eq. 4310 R= (589.0 nm) = = 982. (589.6 nm)  (589.0 nm)
Our resolving power is then R = 1000. Using Eq. 4311 we can find the number of grating lines required. We are looking at the secondorder maxima, so R (1000) N= = = 500. m (2) E4318 (a) N = R/m = /m, so N= (415.5 nm) = 23100. (2)(415.496 nm  415.487 nm)
(b) d = w/N , where w is the width of the grating. Then = arcsin m (23100)(2)(415.5109 m) = arcsin = 27.6 . d (4.15102 m) 224
E4319 N = R/m = /m, so N= E4320 Start with Eq. 439: D= E4321 d sin / tan m = = . d cos d cos (656.3 nm) = 3650 (1)(0.180 nm)
(a) We find the ruling spacing by Eq. 431, d= m (3)(589 nm) = = 9.98 m. sin m sin(10.2 )
(b) The resolving power of the grating needs to be at least R = 1000 for the thirdorder line; see the work for Ex. 4317 above. The number of lines required is given by Eq. 4311, N= R (1000) = = 333, m (3)
so the width of the grating (or at least the part that is being used) is 333(9.98 m) = 3.3 mm. E4322 (a) Condition (1) is satisfied if d 2(600 nm)/ sin(30 ) = 2400 nm. The dispersion is maximal for the smallest d, so d = 2400 nm. (b) To remove the third order requires d = 3a, or a = 800 nm. E4323 (a) The angles of the first three orders are 1 2 3 = = = (1)(589109 m)(40000) = 18.1 , (76103 m) (2)(589109 m)(40000) = 38.3 , arcsin (76103 m) (3)(589109 m)(40000) arcsin = 68.4 . (76103 m) arcsin
The dispersion for each order is D1 D2 D3 (b) R = N m, so R1 R2 R3 = = = (40000)(1) = 40000, (40000)(2) = 80000, (40000)(3) = 120000. 225 = = = (1)(40000) 360 = 3.2102 /nm, (76106 nm) cos(18.1 ) 2 (2)(40000) 360 = 7.7102 /nm, (76106 nm) cos(38.3 ) 2 (3)(40000) 360 = 2.5101 /nm. (76106 nm) cos(68.4 ) 2
E4324 d = m/2 sin , so d= (2)(0.122 nm) = 0.259 nm. 2 sin(28.1 )
E4325
Bragg reflection is given by Eq. 4312 2d sin = m,
where the angles are measured not against the normal, but against the plane. The value of d depends on the family of planes under consideration, but it is at never larger than a0 , the unit cell dimension. We are looking for the smallest angle; this will correspond to the largest d and the smallest m. That means m = 1 and d = 0.313 nm. Then the minimum angle is = sin1 (1)(29.3 1012 m) = 2.68 . 2(0.313 109 m)
E4326 2d/ = sin 1 and 2d/2 = sin 2 . Then 2 = arcsin[2 sin(3.40 )] = 6.81 . E4327 We apply Eq. 4312 to each of the peaks and find the product m = 2d sin . The four values are 26 pm, 39 pm, 52 pm, and 78 pm. The last two values are twice the first two, so the wavelengths are 26 pm and 39 pm. E4328 (a) 2d sin = m, so d= (3)(96.7 pm) = 171 pm. 2 sin(58.0 )
(b) = 2(171 pm) sin(23.2 )/(1) = 135 pm. E4329 The angle against the face of the crystal is 90  51.3 = 38.7 . The wavelength is = 2(39.8 pm) sin(38.7 )/(1) = 49.8 pm. E4330 If > 2d then /2d > 1. But /2d = sin /m. This means that sin > m, but the sine function can never be greater than one. E4331 There are too many unknowns. It is only possible to determine the ratio d/. E4332 A wavelength will be diffracted if m = 2d sin . The possible solutions are 3 4 = = 2(275 pm) sin(47.8)/(3) = 136 pm, 2(275 pm) sin(47.8)/(4) = 102 pm.
226
E4333
We use Eq. 4312 to first find d; d= m (1)(0.261 109 m) = = 1.45 1010 m. 2 sin 2 sin(63.8 )
d is the spacing between the planes in Fig. 4328; it correspond to half of the diagonal distance between two cell centers. Then (2d)2 = a2 + a2 , 0 0 or a0 = 2d = 2(1.45 1010 m) = 0.205 nm.
E4334 Diffraction occurs when 2d sin = m. The angles in this case are then given by sin = m (0.125109 m) = (0.248)m. 2(0.252109 m)
There are four solutions to this equation. They are 14.4 , 29.7 , 48.1 , and 82.7 . They involve rotating the crystal from the original orientation (90  42.4 = 47.6 ) by amounts 47.6  14.4 47.6  29.7 47.6  48.1 47.6  82.7 = = = = 33.2 , 17.9 , 0.5 , 35.1 .
P431 Since the slits are so narrow we only need to consider interference effects, not diffraction effects. There are three waves which contribute at any point. The phase angle between adjacent waves is = 2d sin /. We can add the electric field vectors as was done in the previous chapters, or we can do it in a different order as is shown in the figure below.
Then the vectors sum to E(1 + 2 cos ). We need to square this quantity, and then normalize it so that the central maximum is the maximum. Then (1 + 4 cos + 4 cos2 ) I = Im . 9 227
P432
(a) Solve for I = I m /2, this occurs when 3 = 1 + 2 cos , 2
or = 0.976 rad. The corresponding angle x is x But = 2x , so . 3.2d (b) For the two slit pattern the half width was found to be = /2d. The half width in the three slit case is smaller. P433 (a) and (b) A plot of the intensity quickly reveals that there is an alternation of large maximum, then a smaller maximum, etc. The large maxima are at = 2n, the smaller maxima are half way between those values. (c) The intensity at these secondary maxima is then I = Im (1 + 4 cos + 4 cos2 ) Im = . 9 9 (0.976) = = . 2d 2d 6.44d
Note that the minima are not located halfway between the maxima! P434 Covering up the middle slit will result in a two slit apparatus with a slit separation of 2d. The half width, as found in Problem 415, is then = /2(2d), = /4d, which is narrower than before covering up the middle slit by a factor of 3.2/4 = 0.8. P435 (a) If N is large we can treat the phasors as summing to form a flexible "line" of length N E. We then assume (incorrectly) that the secondary maxima occur when the loop wraps around on itself as shown in the figures below. Note that the resultant phasor always points straight up. This isn't right, but it is close to reality.
228
The length of the resultant depends on how many loops there are. For k = 0 there are none. For k = 1 there are one and a half loops. The circumference of the resulting circle is 2N E/3, the diameter is N E/3. For k = 2 there are two and a half loops. The circumference of the resulting circle is 2N E/5, the diameter is N E/5. The pattern for higher k is similar: the circumference is 2N E/(2k + 1), the diameter is N E/(k + 1/2). The intensity at this "approximate" maxima is proportional to the resultant squared, or Ik but I m is proportional to (N E)2 , so Ik = I m 1 . (k + 1/2)2 2 (N E)2 . (k + 1/2)2 2
(b) Near the middle the vectors simply fold back on one another, leaving a resultant of E. Then Ik (E)2 = so (N E)2 , N2
Im , N2 (c) Let have the values which result in sin = 1, and then the two expressions are identical! Ik =
P436 (a) v = f , so v = f + f . Assuming v = 0, we have f /f = /. Ignore the negative sign (we don't need it here). Then R= and then f c = = , f f
c c = . R N m (b) The ray on the top gets there first, the ray on the bottom must travel an additional distance of N d sin . It takes a time t = N d sin /c f =
to do this. (c) Since m = d sin , the two resulting expression can be multiplied together to yield (f )(t) = c N d sin = 1. N m c
This is almost, but not quite, one of Heisenberg's uncertainty relations! P437 (b) We sketch parallel lines which connect centers to form almost any right triangle similar to the one shown in the Fig. 4318. The triangle will have two sides which have integer multiple lengths of the lattice spacing a0 . The hypotenuse of the triangle will then have length h2 + k 2 a0 , where h and k are the integers. In Fig. 4318 h = 2 while k = 1. The number of planes which cut the diagonal is equal to h2 + k 2 if, and only if, h and k are relatively prime. The interplanar spacing is then h2 + k 2 a0 a0 . d= = 2 + k2 2 + k2 h h
229
(a) The next five spacings are then h = 1, h = 1, h = 1, h = 2, h = 1, k = 1, k = 2, k = 3, k = 3, k = 4, d d d d d = a0 / 2, = a0 / 5, = a0 / 10, = a0 / 13, = a0 / 17.
P438 The middle layer cells will also diffract a beam, but this beam will be exactly out of phase with the top layer. The two beams will then cancel out exactly because of destructive interference.
230
E441 (a) The direction of propagation is determined by considering the argument of the sine function. As t increases y must decrease to keep the sine function "looking" the same, so the wave is propagating in the negative y direction. (b) The electric field is orthogonal (perpendicular) to the magnetic field (so Ex = 0) and the direction of motion (so Ey = 0); Consequently, the only nonzero term is Ez . The magnitude of E will be equal to the magnitude of B times c. Since S = E B/0 , when B points in the positive x direction then E must point in the negative z direction in order that S point in the negative y direction. Then Ez = cB sin(ky + t). (c) The polarization is given by the direction of the electric field, so the wave is linearly polarized in the z direction. E442 Let one wave be polarized in the x direction and the other in the y direction. Then the net 2 2 electric field is given by E 2 = Ex + Ey , or
2 E 2 = E0 sin2 (kz  t) + sin2 (kz  t + ) ,
where is the phase difference. We can consider any point in space, including z = 0, and then average the result over a full cycle. Since merely shifts the integration limits, then the result is independent of . Consequently, there are no interference effects. E443 (a) The transmitted intensity is I0 /2 = 6.1103 W/m2 . The maximum value of the electric field is Em = 20 cI = 2(1.26106 H/m)(3.00108 m/s)(6.1103 W/m2 ) = 2.15 V/m.
(b) The radiation pressure is caused by the absorbed half of the incident light, so p = I/c = (6.1103 W/m2 )/(3.00108 m/s) = 2.031011 Pa. E444 The first sheet transmits half the original intensity, the second transmits an amount proportional to cos2 . Then I = (I0 /2) cos2 , or = arccos 2I/I0 = arccos 2(I0 /3)/I0 35.3 .
E445 The first sheet polarizes the unpolarized light, half of the intensity is transmitted, so I1 = 1 I0 . 2 The second sheet transmits according to Eq. 441, I2 = I1 cos2 = 1 1 I0 cos2 (45 ) = I0 , 2 4
and the transmitted light is polarized in the direction of the second sheet. The third sheet is 45 to the second sheet, so the intensity of the light which is transmitted through the third sheet is 1 1 I3 = I2 cos2 = I0 cos2 (45 ) = I0 . 4 8
231
E446 The transmitted intensity through the first sheet is proportional to cos2 , the transmitted intensity through the second sheet is proportional to cos2 (90  ) = sin2 . Then I = I0 cos2 sin2 = (I0 /4) sin2 2, 1 1 arcsin 4I/I0 = arcsin 2 2 Note that 70.4 is also a valid solution! = or 4(0.100I0 )/I0 = 19.6 .
E447 The first sheet transmits half of the original intensity; each of the remaining sheets transmits an amount proportional to cos2 , where = 30 . Then 1 I = cos2 I0 2
3
=
1 6 (cos(30 )) = 0.211 2
E448 The first sheet transmits an amount proportional to cos2 , where = 58.8 . The second sheet transmits an amount proportional to cos2 (90  ) = sin2 . Then I = I0 cos2 sin2 = (43.3 W/m2 ) cos2 (58.8 ) sin2 (58.8 ) = 8.50 W/m2 . E449 Since the incident beam is unpolarized the first sheet transmits 1/2 of the original intensity. The transmitted beam then has a polarization set by the first sheet: 58.8 to the vertical. The second sheet is horizontal, which puts it 31.2 to the first sheet. Then the second sheet transmits cos2 (31.2 ) of the intensity incident on the second sheet. The final intensity transmitted by the second sheet can be found from the product of these terms, I = (43.3 W/m2 ) E4410 p = arctan(1.53/1.33) = 49.0 . E4411 (a) The angle for complete polarization of the reflected ray is Brewster's angle, and is given by Eq. 443 (since the first medium is air) p = tan1 n = tan1 (1.33) = 53.1 . (b) Since the index of refraction depends (slightly) on frequency, then so does Brewster's angle. E4412 (b) Since r + p = 90 , p = 90  (31.8 ) = 58.2 . (a) n = tan p = tan(58.2 ) = 1.61. E4413 The angles are between p = tan1 n = tan1 (1.472) = 55.81 . and p = tan1 n = tan1 (1.456) = 55.52 . E4414 The smallest possible thickness t will allow for one half a wavelength phase difference for the o and e waves. Then nt = /2, or t = (525109 m)/2(0.022) = 1.2105 m. 232 1 2 cos2 (31.2 ) = 15.8 W/m2 .
E4415 (a) The incident wave is at 45 to the optical axis. This means that there are two components; assume they originally point in the +y and +z direction. When they travel through the half wave plate they are now out of phase by 180 ; this means that when one component is in the +y direction the other is in the z direction. In effect the polarization has been rotated by 90 . (b) Since the half wave plate will delay one component so that it emerges 180 "later" than it should, it will in effect reverse the handedness of the circular polarization. (c) Pretend that an unpolarized beam can be broken into two orthogonal linearly polarized components. Both are then rotated through 90 ; but when recombined it looks like the original beam. As such, there is no apparent change. E4416 The quarter wave plate has a thickness of x = /4n, so the number of plates that can be cut is given by N = (0.250103 m)4(0.181)/(488109 m) = 371. P441 Intensity is proportional to the electric field squared, so the original intensity reaching the eye is I0 , with components I h = (2.3)2 I v , and then I0 = I h + I v = 6.3I v or I v = 0.16I0 . Similarly, I h = (2.3)2 I v = 0.84I0 . (a) When the sunbather is standing only the vertical component passes, while (b) when the sunbather is lying down only the horizontal component passes. P442 The intensity of the transmitted light which was originally unpolarized is reduced to I u /2, regardless of the orientation of the polarizing sheet. The intensity of the transmitted light which was originally polarized is between 0 and I p , depending on the orientation of the polarizing sheet. Then the maximum transmitted intensity is I u /2 + I p , while the minimum transmitted intensity is I u /2. The ratio is 5, so I u /2 + I p Ip 5= =1+2 , I u /2 Iu or I p /I u = 2. Then the beam is 1/3 unpolarized and 2/3 polarized. P443 Each sheet transmits a fraction cos2 = cos2 N .
There are N sheets, so the fraction transmitted through the stack is cos2 N
N
.
We want to evaluate this in the limit as N . As N gets larger we can use a small angle approximation to the cosine function, 1 cos x 1  x2 for x 2 The the transmitted intensity is 1 1 2 2 N2 233
2N
1
.
This expression can also be expanded in a binomial expansion to get 1  2N 1 2 , 2 N2
which in the limit as N approaches 1. The stack then transmits all of the light which makes it past the first filter. Assuming the light is originally unpolarized, then the stack transmits half the original intensity. P444 (a) Stack several polarizing sheets so that the angle between any two sheets is sufficiently small, but the total angle is 90 . (b) The transmitted intensity fraction needs to be 0.95. Each sheet will transmit a fraction cos2 , where = 90 /N , with N the number of sheets. Then we want to solve 0.95 = cos2 (90 /N )
N
for N . For large enough N , will be small, so we can expand the cosine function as cos2 = 1  sin2 1  2 , so 0.95 1  (/2N )2 which has solution N = 2 /4(0.05) = 49. P445 Since passing through a quarter wave plate twice can rotate the polarization of a linearly polarized wave by 90 , then if the light passes through a polarizer, through the plate, reflects off the coin, then through the plate, and through the polarizer, it would be possible that when it passes through the polarizer the second time it is 90 to the polarizer and no light will pass. You won't see the coin. On the other hand if the light passes first through the plate, then through the polarizer, then is reflected, the passes again through the polarizer, all the reflected light will pass through he polarizer and eventually work its way out through the plate. So the coin will be visible. Hence, side A must be the polarizing sheet, and that sheet must be at 45 to the optical axis. P446 (a) The displacement of a ray is given by tan k = yk /t, so the shift is y = t(tan e  tan o ). Solving for each angle, e o The shift is then y = (1.12102 m) (tan(24.94)  tan(22.21)) = 6.35104 m. (b) The eray bends less than the oray. (c) The rays have polarizations which are perpendicular to each other; the owave being polarized along the direction of the optic axis. (d) One ray, then the other, would disappear. 234 = = arcsin arcsin 1 sin(38.8 ) (1.486) 1 sin(38.8 ) (1.658) = 24.94 , = 22.21 .
N
1  N (/2N )2 ,
P447 The method is outline in Sample Problem 4424; use a polarizing sheet to pick out the oray or the eray.
235
E451
(a) The energy of a photon is given by Eq. 451, E = hf , so E = hf = hc .
Putting in "best" numbers hc = (6.626068761034 J s) (2.99792458108 m/s) = 1.23984106 eV m. (1.6021764621019 C)
This means that hc = 1240 eV nm is accurate to almost one part in 8000! (b) E = (1240 eV nm)/(589 nm) = 2.11 eV. E452 Using the results of Exercise 451, = which is in the infrared. E453 Using the results of Exercise 451, E1 = and E2 = (1240 eV nm) = 3.31 eV, (375 nm) (1240 eV nm) = 2.14 eV, (580 nm) (1240 eV nm) = 2100 nm, (0.60 eV)
The difference is E = (3.307 eV)  (2.138 eV) = 1.17 eV. E454 P = E/t, so, using the result of Exercise 451, P = (100/s) That's a small 3.681017 W. E455 When talking about the regions in the sun's spectrum it is more common to refer to wavelengths than frequencies. So we will use the results of Exercise 451(a), and solve = hc/E = (1240 eV nm)/E. The energies are between E = (1.01018 J)/(1.61019 C) = 6.25 eV and E = (1.01016 J)/(1.6 1019 C) = 625 eV. These energies correspond to wavelengths between 198 nm and 1.98 nm; this is the ultraviolet range. E456 The energy per photon is E = hf = hc/. The intensity is power per area, which is energy per time per area, so P E nhc hc n I= = = = . A At At A t But R = n/t is the rate of photons per unit time. Since h and c are constants and I and A are equal for the two beams, we have R1 /1 = R2 /2 , or R1 /R2 = 1 /2 . 236 (1240 eV nm) = 230 eV/s. (540 nm)
E457 (a) Since the power is the same, the bulb with the larger energy per photon will emits fewer photons per second. Since longer wavelengths have lower energies, the bulb emitting 700 nm must be giving off more photons per second. (b) How many more photons per second? If E1 is the energy per photon for one of the bulbs, then N1 = P/E1 is the number of photons per second emitted. The difference is then N1  N2 = or N1 N2 = (130 W) ((700109 m)  (400109 m)) = 1.961020 . (6.631034 Js)(3.00108 m/s) P P P  = (1  2 ), E1 E2 hc
E458 Using the results of Exercise 451, the energy of one photon is E= (1240 eV nm) = 1.968 eV, (630 nm)
The total light energy given off by the bulb is E t = P t = (0.932)(70 W)(730 hr)(3600 s/hr) = 1.71108 J. The number of photons is n= Et (1.71108 J) = = 5.431026 . E0 (1.968 eV)(1.61019 J/eV)
E459 Apply Wien's law, Eq. 454, max T = 2898 m K; so T = (2898 m K) = 91106 K. (321012 m)
Actually, the wavelength was supposed to be 32 m. Then the temperature would be 91 K. E4510 Apply Wien's law, Eq. 454, max T = 2898 m K; so = (2898 m K) = 1.45 m. (0.0020 K)
This is in the radio region, near 207 on the FM dial. E4511 The wavelength of the maximum spectral radiancy is given by Wien's law, Eq. 454, max T = 2898 m K. Applying to each temperature in turn, (a) = 1.06103 m, which is in the microwave; (b) = 9.4106 m, which is in the infrared; (c) = 1.6106 m, which is in the infrared; (d) = 5.0107 m, which is in the visible; (e) = 2.91010 m, which is in the xray; (f) = 2.91041 m, which is in a hard gamma ray.
237
E4512 (a) Apply Wien's law, Eq. 454, max T = 2898 m K.; so = (2898 m K) = 5.00107 m. (5800 K)
That's bluegreen. (b) Apply Wien's law, Eq. 454, max T = 2898 m K.; so T = E4513 I = T 4 and P = IA. Then P = (5.67108 W/m2 K4 )(1900 K)4 (0.5103 m)2 = 0.58 W. E4514 Since I T 4 , doubling T results in a 24 = 16 times increase in I. Then the new power level is (16)(12.0 mW) = 192 mW. E4515 (a) We want to apply Eq. 456, R(, T ) = 1 2c2 h . 5 hc/kT  1 e (2898 m K) = 5270 K. (550109 m)
We know the ratio of the spectral radiancies at two different wavelengths. Dividing the above equation at the first wavelength by the same equation at the second wavelength, 3.5 = 5 ehc/1 kT  1 1 , 5 ehc/2 kT  1 2
where 1 = 200 nm and 2 = 400 nm. We can considerably simplify this expression if we let x = ehc/2 kT , because since 2 = 21 we would have ehc/1 kT = e2hc/2 kT = x2 . Then we get 3.5 = 1 2
5
x2  1 1 = (x + 1). x1 32
We will use the results of Exercise 451 for the exponents and then rearrange to get T = hc (3.10 eV) = = 7640 K. 1 k ln(111) (8.62105 eV/K) ln(111)
(b) The method is the same, except that instead of 3.5 we have 1/3.5; this means the equation for x is 1 1 = (x + 1), 3.5 32 with solution x = 8.14, so then T = hc (3.10 eV) = = 17200 K. 1 k ln(8.14) (8.62105 eV/K) ln(8.14) 238
E4516 hf = , so f= (5.32 eV) = = 1.281015 Hz. h (4.141015 eV s)
E4517 We'll use the results of Exercise 451. Visible red light has an energy of E= (1240 eV nm) = 1.9 eV. (650 nm)
The substance must have a work function less than this to work with red light. This means that only cesium will work with red light. Visible blue light has an energy of E= (1240 eV nm) = 2.75 eV. (450 nm)
This means that barium, lithium, and cesium will work with blue light. E4518 Since K m = hf  , K m = (4.141015 eV s)(3.191015 Hz)  (2.33 eV) = 10.9 eV. E4519 (a) Use the results of Exercise 451 to find the energy of the corresponding photon, E= hc (1240 eV nm) = = 1.83 eV. (678 nm)
Since this energy is less than than the minimum energy required to remove an electron then the photoelectric effect will not occur. (b) The cutoff wavelength is the longest possible wavelength of a photon that will still result in the photoelectric effect occurring. That wavelength is = (1240 eV nm) (1240 eV nm) = = 544 nm. E (2.28 eV)
This would be visible as green. E4520 (a) Since K m = hc/  , Km = (1240 eV nm) (4.2 eV) = 2.0 eV. (200 nm)
(b) The minimum kinetic energy is zero; the electron just barely makes it off the surface. (c) V s = K m /q = 2.0 V. (d) The cutoff wavelength is the longest possible wavelength of a photon that will still result in the photoelectric effect occurring. That wavelength is = (1240 eV nm) (1240 eV nm) = = 295 nm. E (4.2 eV)
E4521 K m = qV s = 4.92 eV. But K m = hc/  , so = (1240 eV nm) = 172 nm. (4.92 eV + 2.28 eV) 239
E4522 (a) K m = qV s and K m = hc/  . We have two different values for qV s and , so subtracting this equation from itself yields q(V s,1  V s,2 ) = hc/1  hc/2 . Solving for 2 , 2 = = = hc , hc/1  q(V s,1  V s,2 ) (1240 eV nm) , (1240 eV nm)/(491 nm)  (0.710 eV) + (1.43 eV) 382 nm.
(b) K m = qV s and K m = hc/  , so = (1240 eV nm)/(491 nm)  (0.710 eV) = 1.82 eV. E4523 (a) The stopping potential is given by Eq. 4511, V0 = so V0 = h f , e e
(1240 eV nm) (1.85 eV  = 1.17 V. e(410 nm e
(b) These are not relativistic electrons, so v= or v = 64200 m/s. E4524 It will have become the stopping potential, or V0 = so V0 = E4525 E4526 (a) Using the results of Exercise 451, = (b) This is in the xray region. E4527 (a) Using the results of Exercise 451, E= (1240 eV nm) = 29, 800 eV. (41.6103 nm) (1240 eV nm) = 62 pm. (20103 eV) h f , e e 2K/m = c 2K/mc2 = c 2(1.17 eV)/(0.511106 eV) = 2.14103 c,
(2.49 eV) (4.141015 eV m) (6.331014 /s)  = 0.131 V. (1.0e) (1.0e)
(b) f = c/ = (3108 m/s)/(41.6 pm) = 7.211018 /s. (c) p = E/c = 29, 800 eV/c = 2.98104 eV/c. 240
E4528 (a) E = hf , so f= (0.511106 eV) = 1.231020 /s. (4.141015 eV s)
(b) = c/f = (3108 m/s)/(1.231020 /s) = 2.43 pm. (c) p = E/c = (0.511106 eV)/c. E4529 The initial momentum of the system is the momentum of the photon, p = h/. This momentum is imparted to the sodium atom, so the final speed of the sodium is v = p/m, where m is the mass of the sodium. Then v= h (6.631034 J s) = = 2.9 cm/s. m (589109 m)(23)(1.71027 kg)
E4530 (a) C = h/mc = hc/mc2 , so C = (1240 eV nm) = 2.43 pm. (0.511106 eV)
(c) Since E = hf = hc/, and = h/mc = hc/mc2 , then E = hc/ = mc2 . (b) See part (c). E4531 The change in the wavelength of a photon during Compton scattering is given by Eq. 4517, h =+ (1  cos ). mc We'll use the results of Exercise 4530 to save some time, and let h/mc = C , which is 2.43 pm. (a) For = 35 , = (2.17 pm) + (2.43 pm)(1  cos 35 ) = 2.61 pm. (b) For = 115 , = (2.17 pm) + (2.43 pm)(1  cos 115 ) = 5.63 pm. E4532 (a) We'll use the results of Exercise 451: = (1240 eV nm) = 2.43 pm. (0.511106 eV)
(b) The change in the wavelength of a photon during Compton scattering is given by Eq. 4517, =+ h (1  cos ). mc
We'll use the results of Exercise 4530 to save some time, and let h/mc = C , which is 2.43 pm. = (2.43 pm) + (2.43 pm)(1  cos 72 ) = 4.11 pm. (c) We'll use the results of Exercise 451: E= (1240 eV nm) = 302 keV. (4.11 pm) 241
E4533 4517,
The change in the wavelength of a photon during Compton scattering is given by Eq. =
h (1  cos ). mc We are not using the expression with the form because and E are not simply related. The wavelength is related to frequency by c = f , while the frequency is related to the energy by Eq. 451, E = hf . Then E = E  E = hf  hf , 1 1 = hc  ,  = hc . h2 (1  cos ) . m
Into this last expression we substitute the Compton formula. Then E =
Now E = hf = hc/, and we can divide this on both sides of the above equation. Also, = c/f , and we can substitute this into the right hand side of the above equation. Both of these steps result in E hf = (1  cos ). E mc2 Note that mc2 is the rest energy of the scattering particle (usually an electron), while hf is the energy of the scattered photon. E4534 The wavelength is related to frequency by c = f , while the frequency is related to the energy by Eq. 451, E = hf . Then E = E  E = hf  hf , 1 1 = hc  ,  , = hc = , + 3 + 3 = 4, or = 3. E4535 The maximum shift occurs when = 180 , so m = 2 h (1240 eV nm) =2 = 2.641015 m. mc 938 MeV)
E E But E/E = 3/4, so
E4536 Since E = hf frequency shifts are identical to energy shifts. Then we can use the results of Exercise 4533 to get (0.9999)(6.2 keV) (0.0001) = (1  cos ), (511 keV) which has solution = 7.4 . (b) (0.0001)(6.2 keV) = 0.62 eV. 242
E4537 4517,
(a) The change in wavelength is independent of the wavelength and is given by Eq. = (1240 eV nm) hc (1  cos ) = 2 = 4.85103 nm. 2 mc (0.511106 eV)
(b) The change in energy is given by E hc hc  , f i 1 1  = hc i + i = = (1240 eV nm)
, = 42.1 keV
1 1  (9.77 pm) + (4.85 pm) (9.77 pm)
(c) This energy went to the electron, so the final kinetic energy of the electron is 42.1 keV. E4538 For = 90 = h/mc. Then E E = = 1 hf =1 , hf + h/mc . + h/mc
But h/mc = 2.43 pm for the electron (see Exercise 4530). (a) E/E = (2.43 pm)/(3.00 cm + 2.43 pm) = 8.11011 . (b) E/E = (2.43 pm)/(500 nm + 2.43 pm) = 4.86106 . (c) E/E = (2.43 pm)/(0.100 nm + 2.43 pm) = 0.0237. (d) E/E = (2.43 pm)/(1.30 pm + 2.43 pm) = 0.651. E4539 We can use the results of Exercise 4533 to get (0.10) = which has solution = 42/6 . E4540 (a) A crude estimate is that the photons can't arrive more frequently than once every 10  8s. That would provide an emission rate of 108 /s. (b) The power output would be P = (108 ) which is 3.61011 W! E4541 We can follow the example of Sample Problem 456, and apply = 0 (1  v/c). (a) Solving for 0 , 0 = (588.995 nm) = 588.9944 nm. (1  (300 m/s)(3108 m/s) 243 (1240 eV nm) = 2.3108 eV/s, (550 nm) (0.90)(215 keV) (1  cos ), (511 keV)
(b) Applying Eq. 4518, v =  h (6.61034 J s) = = 3102 m/s. m (22)(1.71027 kg)(590109 m)
(c) Emitting another photon will slow the sodium by about the same amount. E4542 (a) (430 m/s)/(0.15 m/s) 2900 interactions. (b) If the argon averages a speed of 220 m/s, then it requires interactions at the rate of (2900)(220 m/s)/(1.0 m) = 6.4105 /s if it is going to slow down in time. P451 The radiant intensity is given by Eq. 453, I = T 4 . The power that is radiated through the opening is P = IA, where A is the area of the opening. But energy goes both ways through the opening; it is the difference that will give the net power transfer. Then
4 4 P net = (I0  I1 )A = A T0  T1 .
Put in the numbers, and P net = (5.67108 W/m2 K4 )(5.20 104 m2 ) (488 K)4  (299 K)4 = 1.44 W. P452 (a) I = T 4 and P = IA. Then T 4 = P/A, or T =
4
(100 W) = 3248 K. (5.67108 W/m2 K4 )(0.28103 m)(1.8102 m)
That's 2980 C. (b) The rate that energy is radiated off is given by dQ/dt = mC dT /dt. The mass is found from m = V , where V is the volume. This can be combined with the power expression to yield AT 4 = V CdT /dt, which can be integrated to yield t = Putting in numbers, t = = (19300kg/m3 )(0.28103 m)(132J/kgC) [1/(2748 K)3  1/(3248 K)3 ], 3(5.67108 W/m2 K4 )(4) 20 ms. V C 3 3 (1/T2  1/T1 ). 3A
P453 Light from the sun will "heatup" the thin black screen. As the temperature of the screen increases it will begin to radiate energy. When the rate of energy radiation from the screen is equal to the rate at which the energy from the sun strikes the screen we will have equilibrium. We need first to find an expression for the rate at which energy from the sun strikes the screen. The temperature of the sun is T S . The radiant intensity is given by Eq. 453, I S = T S 4 . The total power radiated by the sun is the product of this radiant intensity and the surface area of the sun, so P S = 4rS 2 T S 4 , 244
where rS is the radius of the sun. Assuming that the lens is on the surface of the Earth (a reasonable assumption), then we can find the power incident on the lens if we know the intensity of sunlight at the distance of the Earth from the sun. That intensity is PS PS IE = = , A 4RE 2 where RE is the radius of the Earth's orbit. Combining, I E = T S 4 The total power incident on the lens is then P lens = I E Alens = T S 4 rS RE
2
rS RE
2
rl 2 ,
where rl is the radius of the lens. All of the energy that strikes the lens is focused on the image, so the power incident on the lens is also incident on the image. The screen radiates as the temperature increases. The radiant intensity is I = T 4 , where T is the temperature of the screen. The power radiated is this intensity times the surface area, so P = IA = 2ri 2 T 4 . The factor of "2" is because the screen has two sides, while ri is the radius of the image. Set this equal to P lens , 2 rS 2ri 2 T 4 = T S 4 rl 2 , RE or 2 1 rS rl T 4 = T S4 . 2 RE r i The radius of the image of the sun divided by the radius of the sun is the magnification of the lens. But magnification is also related to image distance divided by object distance, so ri i = m = , rS o Distances should be measured from the lens, but since the sun is so far from the Earth, we won't be far off in stating o RE . Since the object is so far from the lens, the image will be very, very close to the focal point, so we can also state i f . Then ri f = , rS RE so the expression for the temperature of the thin black screen is considerably simplified to T4 = Now we can put in some of the numbers. T = 1 (5800 K) 21/4 (1.9 cm) = 1300 K. (26 cm) 1 4 TS 2 rl f
2
.
245
P454
The derivative of R with respect to is 10 c2 h 6 (e( k T )  1)
hc
+
2 c3 h2 e( k T ) 7 (e( k T )  1)2 k T
hc
hc
.
Ohh, that's ugly. Setting it equal to zero allows considerable simplification, and we are left with (5  x)ex = 5, where x = hc/kT . The solution is found numerically to be x = 4.965114232. Then = (1240 eV nm) 2.898103 m K = . 5 eV/K)T (4.965)(8.6210 T
P455 (a) If the planet has a temperature T , then the radiant intensity of the planet will be IT 4 , and the rate of energy radiation from the planet will be P = 4R2 T 4 , where R is the radius of the planet. A steady state planet temperature requires that the energy from the sun arrive at the same rate as the energy is radiated from the planet. The intensity of the energy from the sun a distance r from the sun is P sun /4r2 , and the total power incident on the planet is then P = R2 Equating, 4R2 T 4 T4 = R2 = P sun , 4r2 P sun . 4r2
P sun . 16r2
(b) Using the last equation and the numbers from Problem 3, 1 T = (5800 K) 2 That's about 43 F. P456 (a) Change variables as suggested, then = hc/xkT and d = (hc/x2 kT )dx. Integrate (note the swapping of the variables of integration picks up a minus sign): I = = = 2c2 h (hc/x2 kT )dx , (hc/xkT )5 ex  1 2k 4 T 4 x3 dx , h3 c2 ex  1 2 5 k 4 4 T . 15h3 c2 246 (6.96108 m) = 279 K. (1.51011 m)
P457
(a) P = E/t = nhf /t = (hc/)(n/t), where n/t is the rate of photon emission. Then n/t = (100 W)(589109 m) = 2.961020 /s. (6.631034 J s)(3.00108 m/s)
(b) The flux at a distance r is the rate divided by the area of the sphere of radius r, so r= (2.961020 /s) = 4.8107 m. 4(1104 /m2 s)
(c) The photon density is the flux divided by the speed of light; the distance is then r= (d) The flux is given by (2.961020 /s) = 5.891018 /m2 s. 4(2.0 m)2 The photon density is (5.891018 m2 s)/(3.00108 m/s) = 1.961010 /m3 . P458 Momentum conservation requires p = pe , while energy conservation requires E + mc2 = Ee . Square both sides of the energy expression and
2 E + 2E mc2 + m2 c4 2 E + 2E mc2 2 2 p c + 2E mc2 2 = Ee = p2 c2 + m2 c4 , e 2 2 = pe c , = p2 c2 . e
(2.961020 /s) = 280 m. 4(1106 /m3 )(3108 m/s)
But the momentum expression can be used here, and the result is 2E mc2 = 0. Not likely. P459 be or K= (a) Since qvB = mv 2 /r, v = (q/m)rB The kinetic energy of (nonrelativistic) electrons will K= 1 1 q 2 (rB)2 mv 2 = , 2 2 m
1 (1.61019 C) (188106 T m)2 = 3.1103 eV. 2 (9.11031 kg)
(b) Use the results of Exercise 451, = (1240 eV nm)  3.1103 eV = 1.44104 eV. (71103 nm) 247
P4510 P4511 then (a) The maximum value of is 2h/mc. The maximum energy lost by the photon is hc hc  , f i 1 1 = hc  i + i 2h/mc = hc , ( + 2h/mc)
E
=
,
where in the last line we wrote for i . The energy given to the electron is the negative of this, so Kmax = 2h2 . m( + 2h/mc)
Multiplying through by 12 = (E/hc)2 we get Kmax = or Kmax = (b) The answer is Kmax = (17.5 keV)2 = 1.12 keV. (511 eV)/2 + (17.5 keV) 2E 2 . mc2 (1 + 2hc/mc2 ) E2 . mc2 /2 + E
248
E461
(a) Apply Eq. 461, = h/p. The momentum of the bullet is p = mv = (0.041 kg)(960 m/s) = 39kg m/s,
so the corresponding wavelength is = h/p = (6.631034 J s)/(39kg m/s) = 1.71035 m. (b) This length is much too small to be significant. How much too small? If the radius of the galaxy were one meter, this distance would correspond to the diameter of a proton. E462 (a) = h/p and p2 /2m = K, then = (b) K = eV , so = 1.226 nm = eV 1.5 V nm. V hc 2mc2 K = 1.226 nm (1240 eV nm) = . K 2(511 keV) K
E463 For nonrelativistic particles = h/p and p2 /2m = K, so = hc/ 2mc2 K. (a) For the electron, (1240 eV nm) = = 0.0388 nm. 2(511 keV)(1.0 keV) (c) For the neutron, = (1240 MeV fm) 2(940 MeV)(0.001 MeV) = 904 fm.
(b) For ultrarelativistic particles K E pc, so = hc (1240 eV nm) = = 1.24 nm. E (1000 eV)
E464 For nonrelativistic particles p = h/ and p2 /2m = K, so K = (hc)2 /2mc2 2 . Then K= (1240 eV nm)2 = 4.34106 eV. 2(5.11106 eV)(589 nm)2
E465
(a) Apply Eq. 461, p = h/. The proton speed would then be v= h hc (1240 MeV fm) =c 2 =c = 0.0117c. m mc (938 MeV)(113 fm)
This is good, because it means we were justified in using the nonrelativistic equations. Then v = 3.51106 m/s. (b) The kinetic energy of this electron would be K= 1 1 mv 2 = (938 MeV)(0.0117)2 = 64.2 keV. 2 2
The potential through which it would need to be accelerated is 64.2 kV.
249
E466 (a) K = qV and p = p= (b) = h/p, so
2mK. Then
2(22)(932 MeV/c2 )(325 eV) = 3.65106 eV/c. (1240 eV nm) hc = = 3.39104 nm. pc (3.65106 eV/c)c
=
E467 (a) For nonrelativistic particles = h/p and p2 /2m = K, so = hc/ 2mc2 K. For the alpha particle, (1240 MeV fm) = = 5.2 fm. 2(4)(932 MeV)(7.5 MeV) (b) Since the wavelength of the alpha is considerably smaller than the distance to the nucleus we can ignore the wave nature of the alpha particle. E468 (a) For nonrelativistic particles p = h/ and p2 /2m = K, so K = (hc)2 /2mc2 2 . Then K= (1240 keV pm)2 = 15 keV. 2(511keV)(10 pm)2
(b) For ultrarelativistic particles K E pc, so E= (1240 keV pm) hc = = 124 keV. (10 pm)
E469
The relativistic relationship between energy and momentum is E 2 = p2 c2 + m2 c4 ,
and if the energy is very large (compared to mc2 ), then the contribution of the mass to the above expression is small, and E 2 p2 c2 . Then from Eq. 461, = h hc hc (1240 MeV f m) = = = = 2.5102 fm. p pc E (50103 MeV) 2mK, and = h/p, so
E4610 (a) K = 3kT /2, p = = =
hc h = , 3mkT 3mc2 kT (1240 MeV f m) 3(4)(932MeV)(8.621011 MeV/K)(291 K)
= 74 pm.
(b) pV = N kT ; assuming that each particle occupies a cube of volume d3 = V0 then the interparticle spacing is d, so d=
3
V /N =
3
(1.381023 J/K)(291 K) = 3.4 nm. (1.01105 Pa)
250
E4611 p = mv and p = h/, so m = h/v. Taking the ratio, v me = = (1.813104 )(3) = 5.439104 . m e ve The mass of the unknown particle is then m= That would make it a neutron. E4612 (a) For nonrelativistic particles = h/p and p2 /2m = K, so = hc/ 2mc2 K. For the electron, (1240 eV nm) = = 1.0 nm. 2(5.11105 eV)(1.5 eV) For ultrarelativistic particles K E pc, so for the photon = hc (1240 eV nm) = = 830 nm. E (1.5 eV) (0.511 MeV/c2 ) = 939.5 MeV. (5.439104 )
(b) Electrons with energies that high are ultrarelativistic. Both the photon and the electron will then have the same wavelength; = hc (1240 MeV fm) = = 0.83 fm. E (1.5 GeV)
E4613
(a) The classical expression for kinetic energy is p = 2mK, h hc = = p 2mc2 K (1240 keV pm) 2(511 keV)(25.0 keV)
so =
= 7.76 pm.
(a) The relativistic expression for momentum is pc = sqrtE 2  m2 c4 = Then = hc = pc (mc2 + K)2  m2 c4 = (1240 keV pm) (25.0 keV)2 + 2(511 keV)(25.0 keV) K 2 + 2mc2 K.
= 7.66 pm.
E4614 We want to match the wavelength of the gamma to that of the electron. For the gamma, = hc/E . For the electron, K = p2 /2m = h2 /2m2 . Combining, K= With numbers, K= (136keV)2 = 18.1 keV. 2(511 keV)
2 E h2 2 E = . 2mh2 c2 2mc2
That would require an accelerating potential of 18.1 kV. 251
E4615 First find thewavelength of the neutrons. For nonrelativistic particles = h/p and p2 /2m = K, so = hc/ 2mc2 K. Then = (1240 keV pm) 2(940103 keV)(4.2103 keV) = 14 pm.
Bragg reflection occurs when 2d sin = , so = arcsin(14 pm)/2(73.2 pm) = 5.5 . E4616 This is merely a Bragg reflection problem. Then 2d sin = m, or = arcsin(1)(11 pm)/2(54.64 pm) = 5.78 , = arcsin(2)(11 pm)/2(54.64 pm) = 11.6 , = arcsin(3)(11 pm)/2(54.64 pm) = 17.6 .
E4617 (a) Since sin 52 = 0.78, then 2(/d) = 1.57 > 1, so there is no diffraction order other than the first. (b) For an accelerating potential of 54 volts we have /d = 0.78. Increasing the potential will increase the kinetic energy, increase the momentum, and decrease the wavelength. d won't change. The kinetic energy is increased by a factor of 60/54 = 1.11, the momentum increases by a factor of 1.11 = 1.05, so the wavelength changes by a factor of 1/1.05 = 0.952. The new angle is then = arcsin(0.952 0.78) = 48 . E4618 First find the wavelength of the electrons. For nonrelativistic particles = h/p and p2 /2m = K, so = hc/ 2mc2 K. Then = (1240 keV pm) 2(511 keV)(0.380 keV) = 62.9 pm.
This is now a Bragg reflection problem. Then 2d sin = m, or = = = = = = = = = arcsin(1)(62.9 arcsin(2)(62.9 arcsin(3)(62.9 arcsin(4)(62.9 arcsin(5)(62.9 arcsin(6)(62.9 arcsin(7)(62.9 arcsin(8)(62.9 arcsin(9)(62.9 pm)/2(314 pm)/2(314 pm)/2(314 pm)/2(314 pm)/2(314 pm)/2(314 pm)/2(314 pm)/2(314 pm)/2(314 pm) = 5.74 , pm) = 11.6 , pm) = 17.5 , pm) = 23.6 , pm) = 30.1 , pm) = 36.9 , pm) = 44.5 , pm) = 53.3 , pm) = 64.3 .
But the odd orders vanish (see Chapter 43 for a discussion on this). E4619 Since f t 1/2, we have f = 1/2(0.23 s) = 0.69/s.
252
E4620 Since f t 1/2, we have f = 1/2(0.10109 s) = 1.61010 /s. The bandwidth wouldn't fit in the frequency allocation! E4621 Apply Eq. 469, E h 4.141015 eV s) = = 7.6105 eV. 2t 2(8.71012 s)
This is much smaller than the photon energy. E4622 Apply Heisenberg twice: E1 = and E2 = 4.141015 eV s) = 5.49108 eV. 2(12109 s) 4.141015 eV s) = 2.86108 eV. 2(23109 s)
The sum is E transition = 8.4108 eV. E4623 Apply Heisenberg: p = 6.631034 J s) = 8.81024 kg m/s. 2(121012 m)
E4624 p = (0.5 kg)(1.2 s) = 0.6 kg m/s. The position uncertainty would then be x = (0.6 J/s) = 0.16 m. 2(0.6 kg m/s)
E4625
We want v v, which means p p. Apply Eq. 468, and x h h . 2p 2p
According to Eq. 461, the de Broglie wavelength is related to the momentum by = h/p, so x . 2
E4626 (a) A particle confined in a (one dimensional) box of size L will have a position uncertainty of no more than x L. The momentum uncertainty will then be no less than p so p h h . 2x 2L
(6.631034 J s) = 11024 kg m/s. 2(1010 m) 253
(b) Assuming that p p, we have h , 2L and then the electron will have a (minimum) kinetic energy of p E or E h2 p2 . 2 mL2 2m 8
(hc)2 (1240 keV pm)2 = = 0.004 keV. 8 2 mc2 L2 8 2 (511 keV)(100 pm)2
E4627 (a) A particle confined in a (one dimensional) box of size L will have a position uncertainty of no more than x L. The momentum uncertainty will then be no less than p so p h h . 2x 2L
(6.631034 J s) = 11020 kg m/s. 2(1014 m) p
(b) Assuming that p p, we have h , 2L and then the electron will have a (minimum) kinetic energy of E or E p2 h2 . 2 mL2 2m 8
(1240 MeV fm)2 (hc)2 = = 381 MeV. 8 2 mc2 L2 8 2 (0.511 MeV)(10 fm)2
This is so large compared to the mass energy of the electron that we must consider relativistic effects. It will be very relativistic (381 0.5!), so we can use E = pc as was derived in Exercise 9. Then E= hc (1240 MeV fm) = = 19.7 MeV. 2L 2(10 fm)
This is the total energy; so we subtract 0.511 MeV to get K = 19 MeV. E4628 We want to find L when T = 0.01. This means solving T (0.01) = E E 1 e2kL , U0 U0 (5.0 eV) (5.0 eV) = 16 1 (6.0 eV) (6.0 eV) 16
e2k L ,
= 2.22e2k L , ln(4.5103 ) = 2(5.12109 /m)L, 5.31010 m = L.
254
E4629
The wave number, k, is given by k= 2 hc 2mc2 (U0  E).
(a) For the proton mc2 = 938 MeV, so k= 2 (1240 MeV fm) 2(938 MeV)(10 MeV  3.0 MeV) = 0.581 fm1 .
The transmission coefficient is then T = 16 (3.0 MeV) (10 MeV) 1 (3.0 MeV) (10 MeV)
1 e2(0.581 fm )(10 fm) = 3.0105 .
(b) For the deuteron mc2 = 2 938 MeV, so k= 2 (1240 MeV fm) 2(2)(938 MeV)(10 MeV  3.0 MeV) = 0.821 fm1 .
The transmission coefficient is then T = 16 (3.0 MeV) (10 MeV) 1 (3.0 MeV) (10 MeV)
1 e2(0.821 fm )(10 fm) = 2.5107 .
E4630 The wave number, k, is given by k= 2 hc 2mc2 (U0  E).
(a) For the proton mc2 = 938 MeV, so k= 2 (1240 keV pm) 2(938 MeV)(6.0 eV  5.0 eV) = 0.219 pm1 .
We want to find T . This means solving T = = = E E 1 e2kL , U0 U0 (5.0 eV) (5.0 eV) 16 1 (6.0 eV) (6.0 eV) 16 1.610133 .
e2(0.21910
12
)(0.7109 )
,
A current of 1 kA corresponds to N = (1103 C/s)/(1.61019 C) = 6.31021 /s protons per seconds. The time required for one proton to pass is then t = 1/(6.31021 /s)(1.610133 ) = 9.910110 s. That's 10104 years!
255
P461
We will interpret low energy to mean nonrelativistic. Then = h h . = p 2mn K
The diffraction pattern is then given by d sin = m = mh/ 2mn K,
where m is diffraction order while mn is the neutron mass. We want to investigate the spread by taking the derivative of with respect to K, mh d cos d =  dK. 2 2mn K 3 Divide this by the original equation, and then cos dK d =  . sin 2K Rearrange, change the differential to a difference, and then = tan K . 2K
We dropped the negative sign out of laziness; but the angles are in radians, so we need to multiply by 180/ to convert to degrees. P462 P463 We want to solve T = 16
E U0
1
E U0
e2kL ,
for E. Unfortunately, E is contained in k since k= 2 hc 2mc2 (U0  E).
We can do this by iteration. The maximum possible value for E U0 1 E U0
is 1/4; using this value we can get an estimate for k: (0.001) = 16(0.25)e2kL , ln(2.5104 ) = 2k(0.7 nm), 5.92/ nm = k. Now solve for E: E = U0  (hc)2 k 2 8mc2 2 , (1240 eV nm)2 (5.92/nm)2 = (6.0 eV)  , 8 2 (5.11105 eV) = 4.67 eV. 256
Put this value for E back into the transmission equation to find a new k: T (0.001) = 16 = E E 1 e2kL , U0 U0 (4.7 eV) (4.7 eV) 16 1 (6.0 eV) (6.0 eV)
e2kL ,
ln(3.68104 ) = 2k(0.7 nm), 5.65/ nm = k. Now solve for E using this new, improved, value for k: E = U0  (hc)2 k 2 8mc2 2 , (1240 eV nm)2 (5.65/nm)2 = (6.0 eV)  , 8 2 (5.11105 eV) = 4.78 eV.
Keep at it. You'll eventually stop around E = 5.07 eV. P464 (a) A one percent increase in the barrier height means U0 = 6.06 eV. For the electron mc2 = 5.11105 eV, so k= 2 (1240 eV nm) 2(5.11105 eV)(6.06 eV  5.0 eV) = 5.27 nm1 .
We want to find T . This means solving T = = = E E 1 e2kL , U0 U0 (5.0 eV) (5.0 eV) 16 1 (6.06 eV) (6.06 eV) 16 1.44103 .
e2(5.27)(0.7) ,
That's a 16% decrease. (b) A one percent increase in the barrier thickness means L = 0.707 nm. For the electron mc2 = 5.11105 eV, so k= 2 (1240 eV nm) 2(5.11105 eV)(6.0 eV  5.0 eV) = 5.12 nm1 .
We want to find T . This means solving T = = = E E 1 e2kL , U0 U0 (5.0 eV) (5.0 eV) 16 1 (6.0 eV) (6.0 eV) 16 1.59103 .
e2(5.12)(0.707) ,
That's a 8.1% decrease. (c) A one percent increase in the incident energy means E = 5.05 eV. For the electron mc2 = 5.11105 eV, so k= 2 (1240 eV nm) 2(5.11105 eV)(6.0 eV  5.05 eV) = 4.99 nm1 . 257
We want to find T . This means solving T = = = That's a 14% increase. P465 First, the rule for exponents ei(a+b) = eia eib . Then apply Eq. 4612, ei = cos + i sin , cos(a + b) + i sin(a + b) = (cos a + i sin a)(sin b + i sin b). Expand the right hand side, remembering that i2 = 1, cos(a + b) + i sin(a + b) = cos a cos b + i cos a sin b + i sin a cos b  sin a sin b. Since the real part of the left hand side must equal the real part of the right and the imaginary part of the left hand side must equal the imaginary part of the right, we actually have two equations. They are cos(a + b) = cos a cos b  sin a sin b and sin(a + b) = cos a sin b + sin a cos b. P466 E E 1 e2kL , U0 U0 (5.05 eV) (5.05 eV) 16 1 (6.0 eV) (6.0 eV) 16 1.97103 .
e2(4.99)(0.7) ,
258
E471
(a) The ground state energy level will be given by E1 = (6.63 1034 J s)2 h2 = = 3.1 1010 J. 2 8mL 8(9.11 1031 kg)(1.4 1014 m)2
The answer is correct, but the units make it almost useless. We can divide by the electron charge to express this in electron volts, and then E = 1900 MeV. Note that this is an extremely relativistic quantity, so the energy expression loses validity. (b) We can repeat what we did above, or we can apply a "trick" that is often used in solving these problems. Multiplying the top and the bottom of the energy expression by c2 we get E1 = Then (hc)2 8(mc2 )L2
(1240 MeV fm)2 = 1.0 MeV. 8(940 MeV)(14 fm)2 (c) Finding an neutron inside the nucleus seems reasonable; but finding the electron would not. The energy of such an electron is considerably larger than binding energies of the particles in the nucleus. E1 = E472 Solve En = for L, then L = = = nhc , 8mc2 En (3)(1240 eV nm) n2 (hc)2 8(mc2 )L2
8(5.11105 eV)(4.7 eV) 0.85 nm.
,
E473 Solve for E4  E1 : E4  E1 = = = 42 (hc)2 12 (hc)2  , 8(mc2 )L2 8(mc2 )L2 (16  1)(1240 eV nm)2 , 8(5.11105 )(0.253 nm)2 88.1 eV.
E474 Since E 1/L2 , doubling the width of the well will lower the ground state energy to (1/2)2 = 1/4, or 0.65 eV. E475 (a) Solve for E2  E1 : E2  E1 = = = 22 h2 12 h2  , 8mL2 8mL2 (3)(6.631034 J s)2 , 8(40)(1.671027 kg)(0.2 m)2 6.21041 J.
(b) K = 3kT /2 = 3(1.381023 J/K)(300 K)/2 = 6.211021 . The ratio is 11020 . (c) T = 2(6.21041 J)/3(1.381023 J/K) = 3.01018 K. 259
E476 (a) The fractional difference is (En+1  En )/En , or En En = = = h2 h2 h2  n2 / n2 , 2 2 8mL 8mL 8mL2 (n + 1)2  n2 , n2 2n + 1 . n2 (n + 1)2
(b) As n the fractional difference goes to zero; the system behaves as if it is continuous. E477 Then (a) We will take advantage of the "trick" that was developed in part (b) of Exercise 471. En = n 2 (1240 eV nm)2 (hc)2 = (15)2 = 8.72 keV. 8mc2 L 8(0.511 106 eV)(0.0985 nm)2
(b) The magnitude of the momentum is exactly known because E = p2 /2m. This momentum is given by pc = 2mc2 E = 2(511 keV)(8.72 keV) = 94.4 keV. What we don't know is in which direction the particle is moving. It is bouncing back and forth between the walls of the box, so the momentum could be directed toward the right or toward the left. The uncertainty in the momentum is then p = p which can be expressed in terms of the box size L by p = p = 2mE = n 2 h2 nh = . 2 4L 2L
(c) The uncertainty in the position is 98.5 pm; the electron could be anywhere inside the well. E478 The probability distribution function is P2 = We want to integrate over the central third, or
L/6
2 2x sin2 . L L
P
=
L/6
2 2x sin2 dx, L L
= =
1 /3 sin2 d, /3 0.196.
E479 (a) Maximum probability occurs when the argument of the cosine (sine) function is k ([k + 1/2]). This occurs when x = N L/2n for odd N . (b) Minimum probability occurs when the argument of the cosine (sine) function is [k + 1/2] (k). This occurs when x = N L/2n for even N . 260
E4710 In Exercise 4721 we show that the hydrogen levels can be written as En = (13.6 eV)/n2 . (a) The Lyman series is the series which ends on E1 . The least energetic state starts on E2 . The transition energy is E2  E1 = (13.6 eV)(1/12  1/22 ) = 10.2 eV. The wavelength is = (b) The series limit is 0  E1 = (13.6 eV)(1/12 ) = 13.6 eV. The wavelength is = hc (1240 eV nm) = = 91.2 nm. E (13.6 eV) (1240 eV nm) hc = = 121.6 nm. E (10.2 eV)
E4711
The ground state of hydrogen, as given by Eq. 4721, is E1 =  me4 (9.109 1031 kg)(1.602 1019 C)4 = = 2.179 1018 J. 8 2 h2 8(8.854 1012 F/m)2 (6.626 1034 J s)2 0
In terms of electron volts the ground state energy is E1 = (2.179 1018 J)/(1.602 1019 C) = 13.60 eV. E4712 In Exercise 4721 we show that the hydrogen levels can be written as En = (13.6 eV)/n2 . (c) The transition energy is E = E3  E1 = (13.6 eV)(1/12  1/32 ) = 12.1 eV. (a) The wavelength is = (b) The momentum is p = E/c = 12.1 eV/c. E4713 In Exercise 4721 we show that the hydrogen levels can be written as En = (13.6 eV)/n2 . (a) The Balmer series is the series which ends on E2 . The least energetic state starts on E3 . The transition energy is E3  E2 = (13.6 eV)(1/22  1/32 ) = 1.89 eV. The wavelength is = hc (1240 eV nm) = = 656 nm. E (1.89 eV) 261 hc (1240 eV nm) = = 102.5 nm. E (12.1 eV)
(b) The next energetic state starts on E4 . The transition energy is E4  E2 = (13.6 eV)(1/22  1/42 ) = 2.55 eV. The wavelength is = hc (1240 eV nm) = = 486 nm. E (2.55 eV)
(c) The next energetic state starts on E5 . The transition energy is E5  E2 = (13.6 eV)(1/22  1/52 ) = 2.86 eV. The wavelength is = hc (1240 eV nm) = = 434 nm. E (2.86 eV)
(d) The next energetic state starts on E6 . The transition energy is E6  E2 = (13.6 eV)(1/22  1/62 ) = 3.02 eV. The wavelength is = hc (1240 eV nm) = = 411 nm. E (3.02 eV)
(e) The next energetic state starts on E7 . The transition energy is E7  E2 = (13.6 eV)(1/22  1/72 ) = 3.12 eV. The wavelength is = hc (1240 eV nm) = = 397 nm. E (3.12 eV)
E4714 In Exercise 4721 we show that the hydrogen levels can be written as En = (13.6 eV)/n2 . The transition energy is E = hc (1240 eV nm) = = 10.20 eV. (121.6 nm)
This must be part of the Lyman series, so the higher state must be En = (10.20 eV)  (13.6 eV) = 3.4 eV. That would correspond to n = 2. E4715 The binding energy is the energy required to remove the electron. If the energy of the electron is negative, then that negative energy is a measure of the energy required to set the electron free. The first excited state is when n = 2 in Eq. 4721. It is not necessary to reevaluate the constants in this equation every time, instead, we start from En = Then the first excited state has energy E2 = The binding energy is then 3.4 eV. 262 (13.6 eV) = 3.4 eV. (2)2 E1 where E1 = 13.60 eV. n2
E4716 rn = a0 n2 , so n= E4717 (847 pm)/(52.9 pm) = 4.
(a) The energy of this photon is E= hc (1240 eV nm) = = 0.96739 eV. (1281.8 nm)
The final state of the hydrogen must have an energy of no more than 0.96739, so the largest possible n of the final state is n< 13.60 eV/0.96739 eV = 3.75,
so the final n is 1, 2, or 3. The initial state is only slightly higher than the final state. The jump from n = 2 to n = 1 is too large (see Exercise 15), any other initial state would have a larger energy difference, so n = 1 is not the final state. So what level might be above n = 2? We'll try n= 13.6 eV/(3.4 eV  0.97 eV) = 2.36,
which is so far from being an integer that we don't need to look farther. The n = 3 state has energy 13.6 eV/9 = 1.51 eV. Then the initial state could be n= 13.6 eV/(1.51 eV  0.97 eV) = 5.01,
which is close enough to 5 that we can assume the transition was n = 5 to n = 3. (b) This belongs to the Paschen series. E4718 In Exercise 4721 we show that the hydrogen levels can be written as En = (13.6 eV)/n2 . (a) The transition energy is E = E4  E1 = (13.6 eV)(1/12  1/42 ) = 12.8 eV. (b) All transitions n m are allowed for n 4 and m < n. The transition energy will be of the form En  Em = (13.6 eV)(1/m2  1/n2 ). The six possible results are 12.8 eV, 12.1 eV, 10.2 eV, 2.55 eV, 1.89 eV, and 0.66 eV. E4719 E = h/2t, so E = (4.141015 eV s)/2(1108 s) = 6.6108 eV. E4720 (a) According to electrostatics and uniform circular motion, mv 2 /r = e2 /4 0 r2 , or v= e2 == 4 0 mr 263 e4 e2 = . 4 2 h2 n 2 2 0 hn 0
Putting in the numbers, v= In this case n = 1. (b) = h/mv, = (6.631034 J s)/(9.111031 kg)(2.18106 m/s) = 3.341010 m. (c) /a0 = (3.341010 m)/(5.291011 ) = 6.31 2. Actually, it is exactly 2. E4721 In order to have an inelastic collision with the 6.0 eV neutron there must exist a transition with an energy difference of less than 6.0 eV. For a hydrogen atom in the ground state E1 = 13.6 eV the nearest state is E2 = (13.6 eV)/(2)2 = 3.4 eV. Since the difference is 10.2 eV, it will not be possible for the 6.0 eV neutron to have an inelastic collision with a ground state hydrogen atom. E4722 (a) The atom is originally in the state n given by n= (13.6 eV)/(0.85 eV) = 4. (1.61019 C)2 2.18106 m/s = . 2(8.851012 F/m)(6.631034 J s)n n
The state with an excitation energy of 10.2 eV, is n= The transition energy is then E = (13.6 eV)(1/22  1/42 ) = 2.55 eV. E4723 According to electrostatics and uniform circular motion, mv 2 /r = e2 /4 0 r2 , or v= The de Broglie wavelength is then = The ratio of /r is 2 0 hn = = kn, r me2 a0 n2 where k is a constant. As n the ratio goes to zero. h 2 0 hn = . mv me2 e2 == 4 0 mr e4 4
2 h2 n 2 0
(13.6 eV)/(13.6 eV  10.2 eV) = 2.
=
e2 . 2 0 hn
264
E4724 In Exercise 4721 we show that the hydrogen levels can be written as En = (13.6 eV)/n2 . The transition energy is E = E4  E1 = (13.6 eV)(1/12  1/42 ) = 12.8 eV. The momentum of the emitted photon is p = E/c = (12.8 eV)/c. This is the momentum of the recoiling hydrogen atom, which then has velocity v= p pc (12.8 eV) = c= (3.00108 m/s) = 4.1 m/s. m mc2 (932 MeV)
E4725 The first Lyman line is the n = 1 to n = 2 transition. The second Lyman line is the n = 1 to n = 3 transition. The first Balmer line is the n = 2 to n = 3 transition. Since the photon frequency is proportional to the photon energy (E = hf ) and the photon energy is the energy difference between the two levels, we have fnm = Em  E n h
where the En is the hydrogen atom energy level. Then f13 = E 3  E1 , h E 3  E2 + E2  E1 E3  E2 E2  E 1 = = + , h h h = f23 + f12 .
E4726 Use En = Z 2 (13.6 eV)/n2 . (a) The ionization energy of the ground state of He+ is En = (2)2 (13.6 eV)/(1)2 = 54.4 eV. (b) The ionization energy of the n = 3 state of Li2+ is En = (3)2 (13.6 eV)/(3)2 = 13.6 eV. E4727 (a) The energy levels in the He+ spectrum are given by En = Z 2 (13.6 eV)/n2 , where Z = 2, as is discussed in Sample Problem 476. The photon wavelengths for the n = 4 series are then hc hc/E4 = = , En  E 4 1  En /E4
265
which can also be written as = = = 16hc/(54.4 eV) , 1  16/n2 16hcn2 /(54.4 eV) , n2  16 Cn2 , n2  16
where C = hc/(3.4 eV) = 365 nm. (b) The wavelength of the first line is the transition from n = 5, = (365 nm)(5)2 = 1014 nm. (5)2  (4)2
The series limit is the transition from n = , so = 365 nm. (c) The series starts in the infrared (1014 nm), and ends in the ultraviolet (365 nm). So it must also include some visible lines. E4728 We answer these questions out of order! (a) n = 1. (b) r = a0 = 5.291011 m. (f) According to electrostatics and uniform circular motion, mv 2 /r = e2 /4 0 r2 , or v= Putting in the numbers, v= (1.61019 C)2 = 2.18106 m/s. 2(8.851012 F/m)(6.631034 J s)(1) e2 == 4 0 mr e4 4
2 h2 n 2 0
=
e2 . 2 0 hn
(d) p = (9.111031 kg)(2.18106 m/s) = 1.991024 kg m/s. (e) = v/r = (2.18106 m/s)/(5.291011 m) = 4.121016 rad/s. (c) l = pr = (1.991024 kg m/s)(5.291011 m) = 1.051034 J s. (g) F = mv 2 /r, so F = (9.111031 kg)(2.18106 m/s)2 /(5.291011 m) = 8.18108 N. (h) a = (8.18108 N)/(9.111031 kg) = 8.981022 m/s2 . (i) K = mv 2 /r, or K= (9.111031 kg)(2.18106 m/s)2 = 2.161018 J = 13.6 eV. 2
(k) E = 13.6 eV. (j) P = E  K = (13.6 eV)  (13.6 eV) = 27.2 eV.
266
E4729 For each r in the quantity we have a factor of n2 . (a) n is proportional to n. (b) r is proportional to n2 . (f) v is proportional to 1/r, or 1/n. (d) p is proportional to v, or 1/n. (e) is proportional to v/r, or 1/n3 . (c) l is proportional to pr, or n. (g) f is proportional to v 2 /r, or 1/n4 . (h) a is proportional to F , or 1/n4 . (i) K is proportional to v 2 , or 1/n2 . (j) E is proportional to 1/n2 . (k) P is proportional to 1/n2 . E4730 (a) Using the results of Exercise 451, E1 = (1240 eV nm) = 1.24105 eV. (0.010 nm)
(b) Using the results of Problem 4511, Kmax = E2 (1.24105 eV)2 = = 40.5104 eV. mc2 /2 + E (5.11105 eV)/2 + (1.24105 eV)
(c) This would likely knock the electron way out of the atom. E4731 The energy of the photon in the series limit is given by E limit = (13.6 eV)/n2 , where n = 1 for Lyman, n = 2 for Balmer, and n = 3 for Paschen. The wavelength of the photon is limit = (1240 eV nm) 2 n = (91.17 nm)n2 . (13.6 eV)
The energy of the longest wavelength comes from the transition from the nearest level, or E long = (13.6 eV) (13.6 eV) 2n + 1  = (13.6 eV) . (n + 1)2 n2 [n(n + 1)]2
The wavelength of the photon is long = (1240 eV nm)[n(n + 1)]2 [n(n + 1)]2 = (91.17 nm) . 2 (13.6 eV)n 2n + 1
(a) The wavelength interval long  limit , or = (91.17 nm) n2 (n + 1)2  n2 (2n + 1) n4 = (91.17 nm) . 2n + 1 2n + 1
For n = 1, = 30.4 nm. For n = 2, = 292 nm. For n = 3, = 1055 nm. (b) The frequency interval is found from f = E limit  E long (13.6 eV) 1 (3.291015 /s) = = . 15 eV s) (n + 1)2 h (4.1410 (n + 1)2
For n = 1, f = 8.231014 Hz. For n = 2, f = 3.661014 Hz. For n = 3, f = 2.051014 Hz. 267
E4732 E4733 (a) We'll use Eqs. 4725 and 4726. At r = 0 2 (0) = while P (0) = 4(0)2 2 (0) = 0. (b) At r = a0 we have 2 (a0 ) = f rac1a3 e2(a0 )/a0 = 0 and P (a0 ) = 4(a0 )2 2 (a0 ) = 10.2 nm1 . E4734 Assume that (a0 ) is a reasonable estimate for (r) everywhere inside the small sphere. Then e2 0.1353 = . 2 = a3 a3 0 0 The probability of finding it in a sphere of radius 0.05a0 is
0.05a0 0
1 2(0)/a0 1 = = 2150 nm3 , 3e a0 a3 0
e2 = 291 nm3 , a3 0
4 (0.1353)4r2 dr = (0.1353)(0.05)3 = 2.26105 . a3 3 0
E4735 Using Eq. 4726 the ratio of the probabilities is e2 P (a0 ) (a0 )2 e2(a0 )/a0 = = 4 = 1.85. 2 e2(2a0 )/a0 P (2a0 ) 4e (2a0 ) E4736 The probability is
1.016a0
P
=
a0
4r2 e2r/a0 dr, a3 0
1 2.032 2 u u e du, 2 2 = 0.00866. = E4737 If l = 3 then ml can be 0, 1, 2, or 3. (a) From Eq. 4730, Lz = ml h/2.. So Lz can equal 0, h/2, h/, or 3h/2. (b) From Eq. 4731, = arccos(ml / l(l + 1)), so can equal 90 , 73.2 , 54.7 , or 30.0 . (c) The magnitude of L is given by Eq. 4728, L= l(l + 1) h = 3h/. 2
E4738 The maximum possible value of ml is 5. Apply Eq. 4731: = arccos (5) (5)(5 + 1) 268 = 24.1 .
E4739 Use the hint. p x = r p x = r x p r = r L = h , 2 h , 2 h , 2 h . 2
E4740 Note that there is a typo in the formula; P (r) must have dimensions of one over length. The probability is
P
=
0
r4 er/a0 dr, 24a5 0
1 = u4 eu du, 24 0 = 1.00
What does it mean? It means that if we look for the electron, we will find it somewhere. E4741 (a) Find the maxima by taking the derivative and setting it equal to zero. r(2a  r)(4a2  6ra + r2 ) r dP = e = 0. dr 8a6 0 The solutions are r = 0, r = 2a, and 4a2  6ra + r2 = 0. The first two correspond to minima (see Fig. 4714). The other two are the solutions to the quadratic, or r = 0.764a0 and r = 5.236a0 . (b) Substitute these two values into Eq. 4736. The results are P (0.764a0 ) = 0.981 nm1 . and P (5.236a0 ) = 3.61 nm1 . E4742 The probability is
5.01a0
P
=
5.00a0
r2 (2  r/a0 )2 er/a0 dr, 8a3 0
=
0.01896.
E4743 n = 4 and l = 3, while ml can be any of 3, 2, 1, 0, 1, 2, 3, while ms can be either 1/2 or 1/2. There are 14 possible states. E4744 n must be greater than l, so n 4. ml  must be less than or equal to l, so ml  3. ms is 1/2 or 1/2. E4745 If ml = 4 then l 4. But n l + 1, so n > 4. We only know that ms = 1/2. 269
E4746 There are 2n2 states in a shell n, so if n = 5 there are 50 states. E4747 Each is in the n = 1 shell, the l = 0 angular momentum state, and the ml = 0 state. But one is in the state ms = +1/2 while the other is in the state ms = 1/2. E4748 Apply Eq. 4731: = arccos and = arccos E4749 All of the statements are true. E4750 There are n possible values for l (start at 0!). For each value of l there are 2l + 1 possible values for ml . If n = 1, the sum is 1. If n = 2, the sum is 1 + 3 = 4. If n = 3, the sum is 1 + 3 + 5 = 9. The pattern is clear, the sum is n2 . But there are two spin states, so the number of states is 2n2 . P471 We can simplify the energy expression as E = E0 n 2 + n2 + n 2 x y z where E0 = h2 . 8mL2 (+1/2) (1/2)(1/2 + 1) (1/2) (1/2)(1/2 + 1) = 54.7
= 125.3 .
To find the lowest energy levels we need to focus on the values of nx , ny , and nz . It doesn't take much imagination to realize that the set (1, 1, 1) will result in the smallest value for n2 + n2 + n2 . The next choice is to set one of the values equal to 2, and try the set (2, 1, 1). x y z Then it starts to get harder, as the next lowest might be either (2, 2, 1) or (3, 1, 1). The only way to find out is to try. I'll tabulate the results for you: nx 1 2 2 3 2 ny 1 1 2 1 2 nz 1 1 1 1 2 n2 + n2 + n2 x y z 3 6 9 11 12 Mult. 1 3 3 3 1 nx 3 3 4 3 4 ny 2 2 1 3 2 nz 1 2 1 1 1 n2 + n2 + n2 x y z 14 17 18 19 21 Mult. 6 3 3 3 6
We are now in a position to state the five lowest energy levels. The fundamental quantity is E0 = (hc)2 (1240 eV nm)2 = = 6.02106 eV. 2 L2 8mc 8(0.511106 eV)(250 nm)2
The five lowest levels are found by multiplying this fundamental quantity by the numbers in the table above. P472 (a) Write the states between 0 and L. Then all states, odd or even, can be written with probability distribution function 2 nx P (x) = sin2 , L L
270
we find the probability of finding the particle in the region 0 x L/3 is
L/3
P
=
0
=
1 3
nx 2 cos2 dx, L L sin(2n/3) 1 . 2n/3
(b) If n = 1 use the formula and P = 0.196. (c) If n = 2 use the formula and P = 0.402. (d) If n = 3 use the formula and P = 0.333. (e) Classically the probability distribution function is uniform, so there is a 1/3 chance of finding it in the region 0 to L/3. P473 The region of interest is small compared to the variation in P (x); as such we can approximate the probability with the expression P = P (x)x. (b) Evaluating, P = = = (b) Evaluating, P = = = P474 (a) P = , or P = A2 e2mx 0 (b) Integrating, 1 = A2 0 = A2 0 = A2 0
4 2
2 4x sin2 x, L L 2 4(L/8) sin2 (0.0003L), L L 0.0006.
2 4x sin2 x, L L 2 4(3L/16) sin2 (0.0003L), L L 0.0003.
/h
.

e2mx

2
/h
dx,
2
h 2m h 2m
eu du,
pi,
2m h
= A0 .
(c) x = 0. P475 We will want an expression for d2 0 . dx2
271
Doing the math one derivative at a time, d2 0 dx2 d d 0 , dx dx 2 d = A0 (2mx/h)emx /h , dx 2 2 = A0 (2mx/h)2 emx /h + A0 (2m/h)emx /h , = = = (2mx/h)2  (2m/h) A0 emx (2mx/h)  (2m/h) 0 .
2
2
/h
,
In the last line we factored out 0 . This will make our lives easier later on. Now we want to go to Schrdinger's equation, and make some substitutions. o   h2 d 2 0 + U 0 8 2 m dx2 = E0 , = E0 , = E,
h2 (2mx/h)2  (2m/h) 0 + U 0 8 2 m h2  2 (2mx/h)2  (2m/h) + U 8 m
where in the last line we divided through by 0 . Now for some algebra, U = E+ h2 (2mx/h)2  (2m/h) , 8 2 m m 2 x2 h = E+  . 2 4
But we are given that E = h/4, so this simplifies to U= m 2 x2 2
which looks like a harmonic oscillator type potential. P476 Assume the electron is originally in the state n. The classical frequency of the electron is f0 , where f0 = v/2r. According to electrostatics and uniform circular motion, mv 2 /r = e2 /4 0 r2 , or v= Then f0 = e2 == 4 0 mr e4 e2 = . 4 2 h2 n 2 2 0 hn 0
e2 1 me2 me4 2E1 = 2 3 3 = 2 0 hn 2 0 h2 n2 4 0h n hn3
Here E1 = 13.6 eV. Photon frequency is related to energy according to f = Enm /h, where Enm is the energy of transition from state n down to state m. Then f= E1 h 1 1  2 2 n m 272 ,
where E1 = 13.6 eV. Combining the fractions and letting m = n  , where is an integer, f = = = = E1 m2  n2 , h m2 n2 E1 (n  m)(m + n) , h m2 n2 E1 (2n + ) , h (n + )2 n2 E1 (2n) , h (n)2 n2 2E1 = f0 . hn3
P477 We need to use the reduced mass of the muon since the muon and proton masses are so close together. Then (207)(1836) me = 186me . m= (207) + (1836) (a) Apply Eq. 4720 1/2: a = a0 /(186) = (52.9 pm)/(186) = 0.284 pm. (b) Apply Eq. 4721: E = E1 (186) = (13.6 eV)(186) = 2.53 keV. (c) = (1240 keV pm)/(2.53 pm) = 490 pm. P478 (a) The reduced mass of the electron is m= (1)(1) me = 0.5me . (1) + (1)
The spectrum is similar, except for this additional factor of 1/2; hence pos = 2H . (b) apos = a0 /(186) = (52.9 pm)/(1/2) = 105.8 pm. This is the distance between the particles, but they are both revolving about the center of mass. The radius is then half this quantity, or 52.9 pm. P479 This problem isn't really that much of a problem. Start with the magnitude of a vector in terms of the components, L2 + L2 + L2 = L2 , x y z and then rearrange, L2 + L2 = L2  L2 . x y z According to Eq. 4728 L2 = l(l + 1)h2 /4 2 , while according to Eq. 4730 Lz = ml h/2. Substitute that into the equation, and L2 + L2 = l(l + 1)h2 /4 2  m2 h2 /4 2 = l(l + 1)  m2 x y l l Take the square root of both sides of this expression, and we are done. 273 h2 . 4 2
The maximum value for ml is l, while the minimum value is 0. Consequently, L2 + L2 = x y and L2 + L2 = x y P4710 Then l(l + 1)  m2 h/2 l l(l + 1)  m2 h/2 l l(l + 1) h/2,
l h/2.
Assume that (0) is a reasonable estimate for (r) everywhere inside the small sphere. 2 = e0 1 = . a3 a3 0 0
The probability of finding it in a sphere of radius 1.11015 m is
1.11015 m 0
4r2 dr 4 (1.11015 m)3 = = 1.21014 . 3 a0 3 (5.291011 m)3
P4711 Then
Assume that (0) is a reasonable estimate for (r) everywhere inside the small sphere. 2 = (2)2 e0 1 = . 32a3 8a3 0 0
The probability of finding it in a sphere of radius 1.11015 m is
1.11015 m 0
4r2 dr 1 (1.11015 m)3 = = 1.51015 . 8a3 6 (5.291011 m)3 0
P4712
(a) The wave function squared is 2 = e2r/a0 a3 0
The probability of finding it in a sphere of radius r = xa0 is
xa0
P
=
0 x
4r2 e2r/a0 dr , a3 0
=
0
4x2 e2x dx,
= 1  e2x (1 + 2x + 2x2 ). (b) Let x = 1, then P = 1  e2 (5) = 0.323. P4713 We want to evaluate the difference between the values of P at x = 2 and x = 2. Then P (2)  P (1) = = 1  e4 (1 + 2(2) + 2(2)2 )  1  e2 (1 + 2(1) + 2(1)2 ) , 5e2  13e4 = 0.439.
274
P4714
Using the results of Problem 4712, 0.5 = 1  e2x (1 + 2x + 2x2 ),
or e2x = 1 + 2x + 2x2 . The result is x = 1.34, or r = 1.34a0 . P4715 The probability of finding it in a sphere of radius r = xa0 is
xa0
P
=
0
r2 (2  r/a0 )2 er/a0 dr 8a3 0
= = The minimum occurs at x = 2, so
1 x 2 x (2  x)2 ex dx 8 0 1  ex (y 4 /8 + y 2 /2 + y + 1).
P = 1  e2 (2 + 2 + 2 + 1) = 0.0527.
275
E481 The highest energy xray photon will have an energy equal to the bombarding electrons, as is shown in Eq. 481, hc min = eV Insert the appropriate values into the above expression, min = The expression is then 1240 109 V m 1240 kV pm = . V V So long as we are certain that the "V " will be measured in units of kilovolts, we can write this as min = min = 1240 pm/V. E482 f = c/ = (3.00108 m/s)/(31.11012 m) = 9.6461018 /s. Planck's constant is then h= E (40.0 keV) = = 4.141015 eV s. f (9.6461018 /s) (4.14 1015 eV s)(3.00 108 m/s) 1240 109 eV m = . eV eV
E483 Applying the results of Exercise 481, V = (1240kV pm) = 9.84 kV. (126 pm)
E484 (a) Applying the results of Exercise 481, min = (1240kV pm) = 35.4 pm. (35.0 kV)
(b) Applying the results of Exercise 451, K = (1240keV pm) = 49.6 pm. (25.51 keV)  (0.53 keV)
(c) Applying the results of Exercise 451, K = (1240keV pm) = 56.5 pm. (25.51 keV)  (3.56 keV)
E485 (a) Changing the accelerating potential of the xray tube will decrease min . The new value will be (using the results of Exercise 481) min = 1240 pm/(50.0) = 24.8 pm. (b) K doesn't change. It is a property of the atom, not a property of the accelerating potential of the xray tube. The only way in which the accelerating potential might make a difference is if K < min for which case there would not be a K line. (c) K doesn't change. See part (b).
276
E486 (a) Applying the results of Exercise 451, E = (1240keV pm) = 64.2 keV. (19.3 pm)
(b) This is the transition n = 2 to n = 1, so E = (13.6 eV)(1/12  1/22 ) = 10.2 eV. E487 Applying the results of Exercise 451, E = and E = The difference is E = (19.8 keV)  (17.6 keV) = 2.2 eV. E488 Since E = hf = hc/, and = h/mc = hc/mc2 , then E = hc/ = mc2 . or V = E /e = mc2 /e = 511 kV. E489 The 50.0 keV electron makes a collision and loses half of its energy to a photon, then the photon has an energy of 25.0 keV. The electron is now a 25.0 keV electron, and on the next collision again loses loses half of its energy to a photon, then this photon has an energy of 12.5 keV. On the third collision the electron loses the remaining energy, so this photon has an energy of 12.5 keV. The wavelengths of these photons will be given by = which is a variation of Exercise 451. E4810 (a) The xray will need to knock free a K shell electron, so it must have an energy of at least 69.5 keV. (b) Applying the results of Exercise 481, min = (1240kV pm) = 17.8 pm. (69.5 kV) (1240 keV pm) , E (1240keV pm) = 19.8 keV. (62.5 pm) (1240keV pm) = 17.6 keV. (70.5 pm)
(c) Applying the results of Exercise 451, K = (1240keV pm) = 18.5 pm. (69.5 keV)  (2.3 keV)
Applying the results of Exercise 451, K = (1240keV pm) = 21.3 pm. (69.5 keV)  (11.3 keV) 277
E4811 (a) Applying the results of Exercise 451, EK = (1240keV pm) = 19.7 keV. (63 pm)
Again applying the results of Exercise 451, EK = (1240keV pm) = 17.5 keV. (71 pm)
(b) Zr or Nb; the others will not significantly absorb either line. E4812 Applying the results of Exercise 451, K = (1240keV pm) = 154.5 pm. (8.979 keV)  (0.951 keV)
Applying the Bragg reflection relationship, d= (154.5 pm) = = 282 pm. 2 sin 2 sin(15.9 ) f,
E4813 Plot the data. The plot should look just like Fig 484. Note that the vertical axis is which is related to the wavelength according to f = c/.
E4814 Remember that the m in Eq. 484 refers to the electron, not the nucleus. This means that the constant C in Eq. 485 is the same for all elements. Since f = c/, we have 1 = 2 For Ga and Nb the wavelength ratio is then Nb = Ga (31)  1 (41)  1
2
Z2  1 Z1  1
2
.
= 0.5625.
E4815 (a) The ground state question is fairly easy. The n = 1 shell is completely occupied by the first two electrons. So the third electron will be in the n = 2 state. The lowest energy angular momentum state in any shell is the s subshell, corresponding to l = 0. There is only one choice for ml in this case: ml = 0. There is no way at this level of coverage to distinguish between the energy of either the spin up or spin down configuration, so we'll arbitrarily pick spin up. (b) Determining the configuration for the first excited state will require some thought. We could assume that one of the K shell electrons (n = 1) is promoted to the L shell (n = 2). Or we could assume that the L shell electron is promoted to the M shell. Or we could assume that the L shell electron remains in the L shell, but that the angular momentum value is changed to l = 1. The question that we would need to answer is which of these possibilities has the lowest energy. The answer is the last choice: increasing the l value results in a small increase in the energy of multielectron atoms. E4816 Refer to Sample Problem 476: r1 = a0 (1)2 (5.291011 m) = = 5.751013 m. Z (92) 278
E4817 We will assume that the ordering of the energy of the shells and subshells is the same. That ordering is 1s < 2s < 2p < 3s < 3p < 4s < 3d < 4p < 5s < 4d < 5p < 6s < 4f < 5d < 6p < 7s < 5f < 6d < 7p < 8s. If there is no spin the s subshell would hold 1 electron, the p subshell would hold 3, the d subshell 5, and the f subshell 7. inert gases occur when a p subshell has filled, so the first three inert gases would be element 1 (Hydrogen), element 1 + 1 + 3 = 5 (Boron), and element 1 + 1 + 3 + 1 + 3 = 9 (Fluorine). Is there a pattern? Yes. The new inert gases have half of the atomic number of the original inert gases. The factor of onehalf comes about because there are no longer two spin states for each set of n, l, ml quantum numbers. We can save time and simply divide the atomic numbers of the remaining inert gases in half: element 18 (Argon), element 27 (Cobalt), element 43 (Technetium), element 59 (Praseodymium). E4818 The pattern is 2 + 8 + 8 + 18 + 18 + 32 + 32+? or 2(12 + 22 + 22 + 33 + 33 + 42 + 42 + x2 ) The unknown is probably x = 5, the next noble element is probably 118 + 2 52 = 168. E4819 (a) Apply Eq. 4723, which can be written as En = For the valence electron of sodium n = 3, Z= (5.14 eV)(3)2 = 1.84, (13.6 eV) (13.6 eV)Z 2 . n2
while for the valence electron of potassium n = 4, Z= (4.34 eV)(4)2 = 2.26, (13.6 eV)
(b) The ratios with the actual values of Z are 0.167 and 0.119, respectively. E4820 (a) There are three ml states allowed, and two ms states. The first electron can be in any one of these six combinations of M1 and m2 . The second electron, given no exclusion principle, could also be in any one of these six states. The total is 36. Unfortunately, this is wrong, because we can't distinguish electrons. Of this total of 36, six involve the electrons being in the same state, while 30 involve the electron being in different states. But if the electrons are in different states, then they could be swapped, and we won't know, so we must divide this number by two. The total number of distinguishable states is then (30/2) + 6 = 21. (b) Six. See the above discussion. 279
E4821 (a) The Bohr orbits are circular orbits of radius rn = a0 n2 (Eq. 4720). The electron is orbiting where the force is e2 Fn = , 2 4 0 rn and this force is equal to the centripetal force, so mv 2 e2 = . 2 rn 4 0 rn where v is the velocity of the electron. Rearranging, v= e2 . 4 0 mrn
The time it takes for the electron to make one orbit can be used to calculate the current, i= q e e = = t 2rn /v 2rn e2 . 4 0 mrn
The magnetic moment of a current loop is the current times the area of the loop, so = iA = which can be simplified to = But rn = a0 n2 , so =n This might not look right, but a0 = =n
0h 2
e 2rn
e2 r2 , 4 0 mrn n
e 2
e2 rn . 4 0 mrn e 2 a0 e2 . 4 0 m
/me2 , so the expression can simplify to h2 =n 4 2 m2 eh 4m = nB .
e 2
(b) In reality the magnetic moments depend on the angular momentum quantum number, not the principle quantum number. Although the Bohr theory correctly predicts the magnitudes, it does not correctly predict when these values would occur. E4822 (a) Apply Eq. 4814: Fz = z dBz = (9.271024 J/T)(16103 T/m) = 1.51025 N. dz
(b) a = F/m, z = at2 /2, and t = y/vy . Then z = F y2 (1.51025 N)(0.82 m)2 = = 3.2105 m. 2 2mvy 2(1.671027 kg)(970 m/s)2
E4823 a = (9.271024 J/T)(1.4103 T/m)/(1.71025 kg) = 7.6104 m/s2 . 280
E4824 (a) U = 2B, or U = 2(5.79105 eV/T)(0.520 T) = 6.02105 eV. (b) f = E/h = (6.02105 eV)(4.141015 eV s) = 1.451010 Hz. (c) = c/f = (3108 m/s)/(1.451010 Hz) = 2.07102 m. E4825 The energy change can be derived from Eq. 4813; we multiply by a factor of 2 because the spin is completely flipped. Then E = 2z Bz = 2(9.271024 J/T)(0.190 T) = 3.521024 J. The corresponding wavelength is = hc (6.631034 J s)(3.00108 m/s) = = 5.65102 m. E (3.521024 J)
This is somewhere near the microwave range. E4826 The photon has an energy E = hc/. This energy is related to the magnetic field in the vicinity of the electron according to E = 2B, so B= hc (1240 eV nm) = = 0.051 T. 2 2(5.79105 J/T)(21107 nm)
E4827 Applying the results of Exercise 451, E= The production rate is then R= (5.0103 W) = 2.01016 /s. (1.55 eV)(1.61019 J/eV) (1240 eV nm) = 1.55 eV. (800nm)
E4828 (a) x = (3108 m/s)(121012 s) = 3.6103 m. (b) Applying the results of Exercise 451, E= (1240 eV nm) = 1.786 eV. (694.4nm)
The number of photons in the pulse is then N = (0.150J)/(1.786 eV)(1.61019 J/eV) = 5.251017 . E4829 We need to find out how many 10 MHz wide signals can fit between the two wavelengths. The lower frequency is f1 = c (3.00 108 m/s) = = 4.29 1014 Hz. 1 700 109 m)
281
The higher frequency is f1 = c (3.00 108 m/s) = = 7.50 1014 Hz. 1 400 109 m)
The number of signals that can be sent in this range is f2  f1 (7.50 1014 Hz)  (4.29 1014 Hz) = = 3.21 107 . (10 MHz) (10 106 Hz) That's quite a number of television channels. E4830 Applying the results of Exercise 451, E= (1240 eV nm) = 1.960 eV. (632.8nm)
The number of photons emitted in one minute is then N= (2.3103 W)(60 s) = 4.41017 . (1.960 eV)(1.61019 J/eV)
E4831 Apply Eq. 4819. E1 3  E1 1 = 2(1.2 eV).. The ratio is then
5 n1 3 = e(2.4 eV)/(8.6210 eV/K)(2000 K) = 9107 . n1 1
E4832 (a) Population inversion means that the higher energy state is more populated; this can only happen if the ratio in Eq. 4819 is greater than one, which can only happen if the argument of the exponent is positive. That would require a negative temperature. (b) If n2 = 1.1n1 then the ratio is 1.1, so T = (2.26 eV = 2.75105 K. (8.62105 eV/K) ln(1.1)
E4833
(a) At thermal equilibrium the population ratio is given by N2 eE2 /kT = E /kT = eE/kT . N1 e 1
But E can be written in terms of the transition photon wavelength, so this expression becomes N2 = N1 ehc/kT . Putting in the numbers,
5 N2 = (4.01020 )e(1240 eVnm)/(582 nm)(8.6210 eV/K)(300 K)) = 6.621016 .
That's effectively none. (b) If the population of the upper state were 7.01020 , then in a single laser pulse E=N hc (6.631034 J s)(3.00108 m/s) = (7.01020 ) = 240 J. (582109 m)
282
E4834 The allowed wavelength in a standing wave chamber are n = 2L/n. For large n we can write 2L 2L 2L n+1 =  2. n+1 n n The wavelength difference is then 2 2L = 2 = n , n 2L which in this case is (533109 m)2 = = 1.71012 m. 2(8.3102 m) E4835 (a) The central disk will have an angle as measured from the center given by d sin = (1.22), and since the parallel rays of the laser are focused on the screen in a distance f , we also have R/f = sin . Combining, and rearranging, 1.22f . d (b) R = 1.22(3.5 cm)(515 nm)/(3 mm) = 7.2106 m. (c) I = P/A = (5.21 W)/(1.5 mm)2 = 7.37105 W/m2 . (d) I = P/A = (0.84)(5.21 W)/(7.2 m)2 = 2.71010 W/m2 . R= E4836 P481 Let 1 be the wavelength of the first photon. Then 2 = 1 + 130 pm. The total energy transfered to the two photons is then hc hc E1 + E2 = + = 20.0 keV. 1 2 We can solve this for 1 , 20.0 keV 1 1 = + , hc 1 1 + 130 pm 21 + 130 pm = , 1 (1 + 130 pm) which can also be written as 2 1 1 (1 + 130 pm) = (62 pm)(21 + 130 pm), + (6 pm)1  (8060 pm2 ) = 0. 1 = 86.8 pm and  92.8 pm. Only the positive answer has physical meaning. The energy of this first photon is then E1 = (1240 keV pm) = 14.3 keV. (86.8 pm)
This equation has solutions
(a) After this first photon is emitted the electron still has a kinetic energy of 20.0 keV  14.3 keV = 5.7 keV. (b) We found the energy and wavelength of the first photon above. The energy of the second photon must be 5.7 keV, with wavelength 2 = (86.8 pm) + 130 pm = 217 pm. 283
P482
Originally, = 1 1 (2.73108 m/s)2 /(3108 m/s)2 = 2.412.
The energy of the electron is E0 = mc2 = (2.412)(511 keV) = 1232 keV. Upon emitting the photon the new energy is E = (1232 keV)  (43.8 keV) = 1189 keV, so the new gamma factor is = (1189 keV)/(511 keV) = 2.326, and the new speed is v = c 1  1/(2.326)2 = (0.903)c. P483 Switch to a reference frame where the electron is originally at rest. Momentum conservation requires 0 = p + pe = 0, while energy conservation requires mc2 = E + Ee . Rearrange to Ee = mc2  E . Square both sides of this energy expression and
2 E  2E mc2 + m2 c4 2 E  2E mc2 p2 c2  2E mc2 2 = Ee = p2 c2 + m2 c4 , e = p2 c2 , e = p2 c2 . e
But the momentum expression can be used here, and the result is 2E mc2 = 0. Not likely. P484 (a) In the Bohr theory we can assume that the K shell electrons "see" a nucleus with charge Z. The L shell electrons, however, are shielded by the one electron in the K shell and so they "see" a nucleus with charge Z  1. Finally, the M shell electrons are shielded by the one electron in the K shell and the eight electrons in the K shell, so they "see" a nucleus with charge Z  9. The transition wavelengths are then 1 = = and 1 = = E E0 = hc hc 1 1  2 32 1 , E E0 (Z  1)2 = hc hc 2 E0 (Z  1) 3 . hc 4 1 1  2 22 1 ,
E0 (Z  9)2 8 . hc 9 284
The ratio of these two wavelengths is 27 (Z  1)2 = . 32 (Z  9)2 Note that the formula in the text has the square in the wrong place! P485 (a) E = hc/; the energy difference is then E 1 1  1 2 2  1 = hc . 2 1 hc = . 2 1 = hc ,
Since 1 and 2 are so close together we can treat the product 1 2 as being either 2 or 2 . Then 1 2 E = (1240 eV nm) (0.597 nm) = 2.1103 eV. (589 nm)2
(b) The same energy difference exists in the 4s 3p doublet, so = (1139 nm)2 (2.1103 eV) = 2.2 nm. (1240 eV nm)
P486 (a) We can assume that the K shell electron "sees" a nucleus of charge Z  1, since the other electron in the shell screens it. Then, according to the derivation leading to Eq. 4722, rK = a0 /(Z  1). (b) The outermost electron "sees" a nucleus screened by all of the other electrons; as such Z = 1, and the radius is r = a0 P487 We assume in this crude model that one electron moves in a circular orbit attracted to the helium nucleus but repelled from the other electron. Look back to Sample Problem 476; we need to use some of the results from that Sample Problem to solve this problem. The factor of e2 in Eq. 4720 (the expression for the Bohr radius) and the factor of (e2 )2 in Eq. 4721 (the expression for the Bohr energy levels) was from the Coulomb force between the single electron and the single proton in the nucleus. This force is F = e2 . 4 0 r2
In our approximation the force of attraction between the one electron and the helium nucleus is F1 = 2e2 . 4 0 r2
The factor of two is because there are two protons in the helium nucleus. There is also a repulsive force between the one electron and the other electron, F2 = e2 , 4 0 (2r)2 285
where the factor of 2r is because the two electrons are on opposite side of the nucleus. The net force on the first electron in our approximation is then F1  F2 = which can be rearranged to yield F net = e2 4 0 r2 2 1 4 = e2 4 0 r2 7 4 . 2e2 e2  , 4 0 r2 4 0 (2r)2
It is apparent that we need to substitute 7e2 /4 for every occurrence of e2 . (a) The ground state radius of the helium atom will then be given by Eq. 4720 with the appropriate substitution, 2 4 0h r= = a0 . 2 /4) m(7e 7 (b) The energy of one electron in this ground state is given by Eq. 4721 with the substitution of 7e2 /4 for every occurrence of e2 , then E= m(7e2 /4)2 49 me4 = . 8 4 h2 16 8 4 h2 0 0
We already evaluated all of the constants to be 13.6 eV. One last thing. There are two electrons, so we need to double the above expression. The ground state energy of a helium atom in this approximation is E0 = 2 49 (13.6 eV) = 83.3eV. 16
(c) Removing one electron will allow the remaining electron to move closer to the nucleus. The energy of the remaining electron is given by the Bohr theory for He+ , and is E He+ = (4)(13.60 eV) = 54.4 eV, so the ionization energy is 83.3 eV  54.4 eV = 28.9 eV. This compares well with the accepted value. P488 Applying Eq. 4819: T = (3.2 eV) = 1.0104 K. (8.62105 eV/K) ln(6.11013 /2.51015 )
P489 sin r/R, where r is the radius of the beam on the moon and R is the distance to the moon. Then 1.22(600109 m)(3.82108 m) r= = 2360 m. (0.118 m) The beam diameter is twice this, or 4740 m. P4810 (a) N = 2L/n , or N= 2(6102 m)(1.75) = 3.03105 . (694109 )
286
(b) N = 2nLf /c, so f = c (3108 m/s) = = 1.43109 /s. 2nL 2(1.75)(6102 m)
Note that the travel time to and fro is t = 2nL/c! (c) f /f is then (694109 ) f = = = 3.3106 . f 2nL 2(1.75)(6102 m)
287
E491
(a) Equation 492 is n(E) = 8 2m3/2 1/2 8 2(mc2 )3/2 1/2 E = E . h3 (hc)3
We can evaluate this by substituting in all known quantities, 8 2(0.511 106 eV)3/2 1/2 n(E) = E = (6.81 1027 m3 eV3/2 )E 1/2 . (1240 109 eV m)3 Once again, we simplified the expression by writing hc wherever we could, and then using hc = 1240 109 eV m. (b) Then, if E = 5.00 eV, n(E) = (6.81 1027 m3 eV3/2 )(5.00 eV)1/2 = 1.52 1028 m3 eV1 . E492 Apply the results of Ex. 491: n(E) = (6.81 1027 m3 eV3/2 )(8.00 eV)1/2 = 1.93 1028 m3 eV1 . E493 Monovalent means only one electron is available as a conducting electron. Hence we need only calculate the density of atoms: NA (19.3103 kg/m3 )(6.021023 mol1 ) N = = = 5.901028 /m3 . V Ar (0.197 kg/mol) E494 Use the ideal gas law: pV = N kT . Then p= E495 N kT = (8.491028 m3 )(1.381023 J/ K)(297 K) = 3.48108 Pa. V
(a) The approximate volume of a single sodium atom is V1 = (0.023 kg/mol) = 3.931029 m3 . (6.021023 part/mol)(971 kg/m3 )
The volume of the sodium ion sphere is 4 (981012 m)3 = 3.941030 m3 . 3 The fractional volume available for conduction electrons is V2 = V 1  V2 (3.931029 m3 )  (3.941030 m3 ) = = 90%. V1 (3.931029 m3 ) (b) The approximate volume of a single copper atom is V1 = (0.0635 kg/mol) = 1.181029 m3 . (6.021023 part/mol)(8960 kg/m3 )
The volume of the copper ion sphere is 4 (961012 m)3 = 3.711030 m3 . 3 The fractional volume available for conduction electrons is V2 = V 1  V2 (1.181029 m3 )  (3.711030 m3 ) = = 69%. V1 (1.181029 m3 ) (c) Sodium, since more of the volume is available for the conduction electron. 288
E496 (a) Apply Eq. 496:
5 p = 1/ e(0.0730 eV)/(8.6210 eV/K)(0 K) + 1 = 0.
(b) Apply Eq. 496:
5 p = 1/ e(0.0730 eV)/(8.6210 eV/K)(320 K) + 1 = 6.62102 .
E497 Apply Eq. 496, remembering to use the energy difference:
5 p = 1/ e(1.1) eV)/(8.6210 eV/K)(273 K) + 1 = 1.00,
5 p = 1/ e(0.1) eV)/(8.6210 eV/K)(273 K) + 1 = 0.986, 5 p = 1/ e(0.0) eV)/(8.6210 eV/K)(273 K) + 1 = 0.5, 5 p = 1/ e(0.1) eV)/(8.6210 eV/K)(273 K) + 1 = 0.014, 5 p = 1/ e(1.1) eV)/(8.6210 eV/K)(273 K) + 1 = 0.0.
(b) Inverting the equation, T = so T = E , k ln(1/p  1)
(0.1 eV) = 700 K (8.62105 eV/K) ln(1/(0.16)  1)
E498 The energy differences are equal, except for the sign. Then 1 e+E/kt +1 + 1 eE/kt +1 = , = , = 1.
eE/2kt e+E/2kt + E/2kt e+E/2kt + eE/2kt e + e+E/2kt E/2kt e + e+E/2kt eE/2kt + e+E/2kt E499 The Fermi energy is given by Eq. 495, EF = h2 8m 3n
2/3
,
where n is the density of conduction electrons. For gold we have n= (19.3 g/cm )(6.021023 part/mol) 3 3 = 5.901022 elect./cm = 59 elect./nm (197 g/mol)
3
The Fermi energy is then (1240 eV nm)2 EF = 8(0.511106 eV) 3(59 electrons/nm )
3 2/3
= 5.53 eV.
289
E4910 Combine the results of Ex. 491 and Eq. 496: C E no = E/kt . e +1 Then for each of the energies we have no = no = no = no = (6.811027 m3 eV3/2 ) (4 eV) = 1.361028 /m3 eV, e(3.06 eV)/(8.62105 eV/K)(1000 K) + 1 (6.811027 m3 eV3/2 ) (6.75 eV) = 1.721028 /m3 eV, e(0.31 eV)/(8.62105 eV/K)(1000 K) + 1 (6.811027 m3 eV3/2 ) (7 eV) = 9.021027 /m3 eV, e(0.06 eV)/(8.62105 eV/K)(1000 K) + 1 (6.811027 m3 eV3/2 ) (7.25 eV) = 1.821027 /m3 eV, e(0.19 eV)/(8.62105 eV/K)(1000 K) + 1 (6.811027 m3 eV3/2 ) (9 eV) = 3.431018 /m3 eV. e(1.94 eV)/(8.62105 eV/K)(1000 K) + 1
no = E4911 Solve
n2 (hc)2 8(mc2 )L2 for n = 50, since there are two electrons in each level. Then En = Ef = (50)2 (1240 eV nm)2 = 6.53104 eV. 8(5.11105 eV)(0.12 nm)2
E4912 We need to be much higher than T = (7.06 eV)/(8.62105 eV/K) = 8.2104 K. E4913 Equation 495 is EF = and if we collect the constants, EF = h2 8m 3
2/3
h2 8m
3n
2/3
,
n3/2 = An3/2 ,
where, if we multiply the top and bottom by c2 A= (hc)2 8mc2 3
2/3
=
(1240 109 eV m)2 8(0.511 106 eV)
3
2/3
= 3.65 1019 m2 eV.
E4914 (a) Inverting Eq. 496, E = kT ln(1/p  1), so E = (8.62105 eV/K)(1050 K) ln(1/(0.91)  1) = 0.209 eV. Then E = (0.209 eV) + (7.06 eV) = 6.85 eV. (b) Apply the results of Ex. 491: n(E) = (6.81 1027 m3 eV3/2 )(6.85 eV)1/2 = 1.78 1028 m3 eV1 . (c) no = np = (1.78 1028 m3 eV1 )(0.910) = 1.62 1028 m3 eV1 . 290
E4915 Equation 495 is EF = and if we rearrange, E F 3/2 = Equation 492 is then 8 2m3/2 1/2 3 n(E) = E = nE F 3/2 E 1/2 . 3 h 2 E4916 ph = 1  p, so ph = = = 1 1 , eE/kT + 1 3h3 n, 16 2m3/2 h2 8m 3n
2/3
,
eE/kT , eE/kT + 1 1 . E/kT 1+e
E4917 The steps to solve this exercise are equivalent to the steps for Exercise 499, except now the iron atoms each contribute 26 electrons and we have to find the density. First, the density is = Then n = = (26)(1.84106 g/cm )(6.021023 part/mol) 3 = 5.11029 elect./cm , (56 g/mol) 5.1108 elect./nm
3 3
m (1.991030 kg) = = 1.84109 kg/m3 4r3 /3 4(6.37106 m)3 /3
The Fermi energy is then (1240 eV nm)2 EF = 8(0.511106 eV) E4918 First, the density is = Then n = (9.51017 kg/m3 )/(1.671027 kg) = 5.691044 /m3 . The Fermi energy is then (1240 MeV fm)2 EF = 8(940 MeV) 3(5.69101 /fm )
3 2/3
3(5.1108 elect./nm )
3
2/3
= 230 keV.
m 2(1.991030 kg) = = 9.51017 kg/m3 3 /3 4r 4(10103 m)3 /3
= 137 MeV.
291
E4919 E4920 (a) E F = 7.06 eV, so f= 3(8.62105 eV K)(0 K) = 0, 2(7.06 eV)
(b) f = 3(8.62105 eV K)(300 K)/2(7.06 eV) = 0.0055. (c) f = 3(8.62105 eV K)(1000 K)/2(7.06 eV) = 0.0183. E4921 Using the results of Exercise 19, T = 2f E F 2(0.0130)(4.71 eV) = = 474 K. 3k 3(8.62105 eV K)
E4922 f = 3(8.62105 eV K)(1235 K)/2(5.5 eV) = 0.029. E4923 (a) Monovalent means only one electron is available as a conducting electron. Hence we need only calculate the density of atoms: N NA (10.5103 kg/m3 )(6.021023 mol1 ) = = = 5.901028 /m3 . V Ar (0.107 kg/mol) (b) Using the results of Ex. 4913, E F = (3.65 1019 m2 eV)(5.901028 /m3 )2/3 = 5.5 eV. (c) v = 2K/m, or v= (d) = h/p, or = (6.631034 J s) = 5.21012 m. (9.111031 kg)(1.4108 m/s) 2(5.5 eV)(5.11105 eV/c2 ) = 1.4108 m/s.
E4924 (a) Bivalent means two electrons are available as a conducting electron. Hence we need to double the calculation of the density of atoms: N NA 2(7.13103 kg/m3 )(6.021023 mol1 ) = = = 1.321029 /m3 . V Ar (0.065 kg/mol) (b) Using the results of Ex. 4913, E F = (3.65 1019 m2 eV)(1.321029 /m3 )2/3 = 9.4 eV. (c) v = 2K/m, or v= (d) = h/p, or = (6.631034 J s) = 4.01012 m. (9.111031 kg)(1.8108 m/s) 292 2(9.4 eV)(5.11105 eV/c2 ) = 1.8108 m/s.
E4925 (a) Refer to Sample Problem 495 where we learn that the mean free path can be written in terms of Fermi speed v F and mean time between collisions as = v F . The Fermi speed is v F = c 2EF /mc2 = c 2(5.51 eV)/(5.11105 eV) = 4.64103 c. The time between collisions is = m (9.111031 kg) = = 3.741014 s. 2 28 m3 )(1.601019 C)2 (1.62108 m) ne (5.8610
We found n by looking up the answers from Exercise 4923 in the back of the book. The mean free path is then = (4.64103 )(3.00108 m/s)(3.741014 s) = 52 nm. (b) The spacing between the ion cores is approximated by the cube root of volume per atom. This atomic volume for silver is V = (108 g/mol) (6.021023 part/mol)(10.5 3 g/cm )
3
= 1.711023 cm3 .
The distance between the ions is then l= The ratio is /l = 190. E4926 (a) For T = 1000 K we can use the approximation, so for diamond
5 p = e(5.5 eV)/2(8.6210 eV/K)(1000 K) = 1.41014 ,
V = 0.257 nm.
while for silicon,
5 p = e(1.1 eV)/2(8.6210 eV/K)(1000 K) = 1.7103 ,
(b) For T = 4 K we can use the same approximation, but now E function goes to zero.
kT and the exponential
E4927 (a) E  E F 0.67 eV/2 = 0.34 eV.. The probability the state is occupied is then
5 p = 1/ e(0.34) eV)/(8.6210 eV/K)(290 K) + 1 = 1.2106 .
(b) E  E F 0.67 eV/2 = 0.34 eV.. The probability the state is unoccupied is then 1  p, or
5 p = 1  1/ e(0.34) eV)/(8.6210 eV/K)(290 K) + 1 = 1.2106 .
E4928 (a) E  E F 0.67 eV/2 = 0.34 eV.. The probability the state is occupied is then
5 p = 1/ e(0.34) eV)/(8.6210 eV/K)(289 K) + 1 = 1.2106 .
293
E4929
(a) The number of silicon atoms per unit volume is n= (6.021023 part/mol)(2.33 g/cm ) 3 = 4.991022 part./cm . (28.1 g/mol)
3
If one out of 1.0eex7 are replaced then there will be an additional charge carrier density of 4.991022 part./cm /1.0107 = 4.991015 part./cm = 4.991021 m3 . (b) The ratio is (4.991021 m3 )/(2 1.51016 m3 ) = 1.7105 . The extra factor of two is because all of the charge carriers in silicon (holes and electrons) are charge carriers. E4930 Since one out of every 5106 silicon atoms needs to be replaced, then the mass of phosphorus would be 1 30 m= = 2.1107 g. 5106 28 E4931 l =
3
3
3
1/1022 /m3 = 4.6108 m.
E4932 The atom density of germanium is N NA (5.32103 kg/m3 )(6.021023 mol1 ) = = = 1.631028 /m3 . V Ar (0.197 kg/mol) The atom density of the impurity is (1.631028 /m3 )/(1.3109 ) = 1.251019 . The average spacing is l=
3
1/1.251019 /m3 = 4.3107 m.
E4933 The first one is an insulator because the lower band is filled and band gap is so large; there is no impurity. The second one is an extrinsic ntype semiconductor: it is a semiconductor because the lower band is filled and the band gap is small; it is extrinsic because there is an impurity; since the impurity level is close to the top of the band gap the impurity is a donor. The third sample is an intrinsic semiconductor: it is a semiconductor because the lower band is filled and the band gap is small. The fourth sample is a conductor; although the band gap is large, the lower band is not completely filled. The fifth sample is a conductor: the Fermi level is above the bottom of the upper band. The sixth one is an extrinsic ptype semiconductor: it is a semiconductor because the lower band is filled and the band gap is small; it is extrinsic because there is an impurity; since the impurity level is close to the bottom of the band gap the impurity is an acceptor. E4934 6.62105 eV/1.1 eV = 6.0105 electronhole pairs. E4935 (a) R = (1 V)/(501012 A) = 21010 . (b) R = (0.75 V)/(8 mA) = 90. 294
E4936 (a) A region with some potential difference exists that has a gap between the charged areas. (b) C = Q/V . Using the results in Sample Problem 499 for q and V , C= n0 eAd/2 = 2 0 A/d. n0 ed2 /4 0
E4937
(a) Apply that ever so useful formula = hc (1240 eV nm) = = 225 nm. E (5.5 eV)
Why is this a maximum? Because longer wavelengths would have lower energy, and so not enough to cause an electron to jump across the band gap. (b) Ultraviolet. E4938 Apply that ever so useful formula E= E4939 The photon energy is E= hc (1240 eV nm) = = 8.86 eV. (140 nm) hc (1240 eV nm) = = 4.20 eV. (295 nm)
which is enough to excite the electrons through the band gap. As such, the photon will be absorbed, which means the crystal is opaque to this wavelength. E4940 P491 We can calculate the electron density from Eq. 495, n = = = 3 3 8mc2 E F (hc)2
3/2
,
3/2
8(0.511106 eV)(11.66 eV) (1240 eV nm)2
3
,
181 electrons/nm .
From this we calculate the number of electrons per particle, (181 electrons/nm )(27.0 g/mol) (2.70 g/cm )(6.021023 particles/mol) which we can reasonably approximate as 3.
3 3
= 3.01,
295
P492 4915,
At absolute zero all states below E F are filled, an none above. Using the results of Ex. 1 n
EF
E av
= = = =
En(E) dE,
0
3 3/2 E F 3/2 EF E dE, 2 0 3 3/2 2 5/2 EF EF , 2 5 3 EF. 5
P493
(a) The total number of conduction electron is n= (0.0031 kg)(6.021023 mol1 ) = 2.941022 . (0.0635 kg/mol)
The total energy is E= 3 (7.06 eV)(2.941022 ) = 1.241023 eV = 2104 J. 5
(b) This will light a 100 W bulb for t = (2104 J)/(100 W) = 200 s. P494 (a) First do the easy part: nc = N c p(E c ), so Nc . e(E c E F )/kT + 1 Then use the results of Ex. 4916, and write nv = N v [1  p(E v )] = Nv . e(E v E F )/kT + 1
Since each electron in the conduction band must have left a hole in the valence band, then these two expressions must be equal. (b) If the exponentials dominate then we can drop the +1 in each denominator, and Nc (E c E F )/kT e Nc Nv EF = Nv (E v E F )/kT e ,
= e(E c 2E F +E v )/kT , = 1 (E c + E v + kT ln(N c /N v )) . 2
P495 (a) We want to use Eq. 496; although we don't know the Fermi energy, we do know the differences between the energies in question. In the undoped silicon E  E F = 0.55 eV for the bottom of the conduction band. The quantity kT = (8.62105 eV/K)(290 K) = 0.025 eV, which is a good number to remember at room temperature kT is 1/40 of an electronvolt. 296
1 = 2.81010 . e(0.55 eV)/(0.025 eV) + 1 In the doped silicon E  E F = 0.084 eV for the bottom of the conduction band. Then p= p= e(0.084 1 = 3.4102 . eV)/(0.025 eV) + 1
Then
(b) For the donor state E  E F = 0.066 eV, so p= P496 so E F = (1.1 eV  0.11 eV)  (8.62105 eV/K)(290 K) ln(1/(4.8105 )  1) = 0.74 eV above the valence band. (b) E  E F = (1.1 eV)  (0.74 eV) = 0.36 eV, so p= e(0.36 1 = 5.6107 . eV)/(0.025 eV) + 1 (a) Inverting Eq. 496, E  E F = kT ln(1/p  1), 1 = 0.93. e(0.066 eV)/(0.025 eV) + 1
P497 (a) Plot the graph with a spreadsheet. It should look like Fig. 4912. (b) kT = 0.025 eV when T = 290 K. The ratio is then if e(0.5 eV)/(0.025 eV) + 1 = (0.5 eV)/(0.025 eV) = 4.9108 . ir e +1 P498
297
E501 We want to follow the example set in Sample Problem 501. The distance of closest approach is given by d = = = That's pretty close. E502 (a) The gold atom can be treated as a point particle: F = = = (b) W = F d, so d= (5.3106 eV)(1.61019 J/eV) = 6.06107 m. (1.4106 N) q1 q2 , 4 0 r2 (2)(79)(1.601019 C)2 , 4(8.851012 C2 /Nm2 )(0.16109 m)2 1.4106 N. qQ , 4 0 K (2)(29)(1.601019 C)2 4(8.851012 C2 /Nm2 )(5.30MeV)(1.60 1.571014 m. 1013 J/MeV) ,
That's 1900 gold atom diameters. E503 Take an approach similar to Sample Problem 501: K = = = qQ , 4 0 d (2)(79)(1.601019 C)2 4(8.851012 C2 /Nm2 )(8.781015 m)(1.60 2.6107 eV.
88
1019 J/eV)
,
E504 All are stable except E505
Rb and
239
Pb.
We can make an estimate of the mass number A from Eq. 501, R = R0 A1/3 ,
where R0 = 1.2 fm. If the measurements indicate a radius of 3.6 fm we would have A = (R/R0 )3 = ((3.6 fm)/(1.2 fm)) = 27. E506 E507 The mass number of the sun is A = (1.991030 kg)/(1.671027 kg) = 1.21057 . The radius would be R = (1.21015 m)
3
3
1.21057 = 1.3104 m. 298
E508 239 Pu is composed of 94 protons and 239  94 = 145 neutrons. The combined mass of the free particles is M = Zmp + N mn = (94)(1.007825 u) + (145)(1.008665 u) = 240.991975 u. The binding energy is the difference E B = (240.991975 u  239.052156 u)(931.5 MeV/u) = 1806.9 MeV, and the binding energy per nucleon is then (1806.9 MeV)/(239) = 7.56 MeV. E509 62 Ni is composed of 28 protons and 62  28 = 34 neutrons. The combined mass of the free particles is M = Zmp + N mn = (28)(1.007825 u) + (34)(1.008665 u) = 62.513710 u. The binding energy is the difference E B = (62.513710 u  61.928349 u)(931.5 MeV/u) = 545.3 MeV, and the binding energy per nucleon is then (545.3 MeV)/(62) = 8.795 MeV. E5010 (a) Multiply each by 1/1.007825, so m1H = 1.00000, m12C = 11.906829, and m238U = 236.202500. E5011 (a) Since the binding energy per nucleon is fairly constant, the energy must be proportional to A. (b) Coulomb repulsion acts between pairs of protons; there are Z protons that can be chosen as first in the pair, and Z  1 protons remaining that can make up the partner in the pair. That makes for Z(Z  1) pairs. The electrostatic energy must be proportional to this. (c) Z 2 grows faster than A, which is roughly proportional to Z. E5012 Solve (0.7899)(23.985042) + x(24.985837) + (0.2101  x)(25.982593) = 24.305 for x. The result is x = 0.1001, and then the amount
26
Mg is 0.1100.
299
E5013 The neutron confined in a nucleus of radius R will have a position uncertainty on the order of x R. The momentum uncertainty will then be no less than p Assuming that p p, we have h h . 2x 2R p
h , 2R and then the neutron will have a (minimum) kinetic energy of E But R = R0 A1/3 , so E For an atom with A = 100 we get E 8 2 (940 (1240 MeV fm)2 = 0.668 MeV. MeV)(1.2 fm)2 (100)2/3 p2 h2 . 2 mR2 2m 8 (hc)2 . 2 8 2 mc2 R0 A2/3
This is about a factor of 5 or 10 less than the binding energy per nucleon. E5014 (a) To remove a proton, E = [(1.007825) + (3.016049)  (4.002603)] (931.5 MeV) = 19.81 MeV. To remove a neutron, E = [(1.008665) + (2.014102)  (3.016049)] (931.5 MeV) = 6.258 MeV. To remove a proton, E = [(1.007825) + (1.008665)  (2.014102)] (931.5 MeV) = 2.224 MeV. (b) E = (19.81 + 6.258 + 2.224)MeV = 28.30 MeV. (c) (28.30 MeV)/4 = 7.07 MeV. E5015 (a) = [(1.007825)  (1)](931.5 MeV) = 7.289 MeV. (b) = [(1.008665)  (1)](931.5 MeV) = 8.071 MeV. (c) = [(119.902197)  (120)](931.5 MeV) = 91.10 MeV. E5016 (a) E B = (ZmH + N mN  m)c2 . Substitute the definition for mass excess, mc2 = Ac2 + , and EB
197
= Z(c2 + H ) + N (c2 + N )  Ac2  , = ZH + N N  .
(b) For
Au,
E B = (79)(7.289 MeV) + (197  79)(8.071 MeV)  (31.157 MeV) = 1559 MeV, and the binding energy per nucleon is then (1559 MeV)/(197) = 7.92 MeV. 300
E5017 The binding energy of
63
Cu is given by
M = Zmp + N mn = (29)(1.007825 u) + (34)(1.008665 u) = 63.521535 u. The binding energy is the difference E B = (63.521535 u  62.929601 u)(931.5 MeV/u) = 551.4 MeV. The number of atoms in the sample is n= The total energy is then (2.871022 )(551.4 MeV)(1.61019 J/eV) = 2.531012 J. E5018 (a) For ultrarelativistic particles E = pc, so = (1240 MeV fm) = 2.59 fm. (480 MeV) (0.003 kg)(6.021023 mol1 ) = 2.871022 . (0.0629 kg/mol)
(b) Yes, since the wavelength is smaller than nuclear radii. E5019 We will do this one the easy way because we can. This method won't work except when there is an integer number of halflives. The activity of the sample will fall to onehalf of the initial decay rate after one halflife; it will fall to onehalf of onehalf (onefourth) after two halflives. So two halflives have elapsed, for a total of (2)(140 d) = 280 d. E5020 N = N0 (1/2)t/t1/2 , so N = (481019 )(0.5)(26)/(6.5) = 3.01019 . E5021 (a) t1/2 = ln 2/(0.0108/h) = 64.2 h. (b) N = N0 (1/2)t/t1/2 , so N/N0 = (0.5)(3) = 0.125. (c) N = N0 (1/2)t/t1/2 , so N/N0 = (0.5)(240)/(64.2) = 0.0749. E5022 (a) = (dN/dt)/N , or = (12/s)/(2.51018 ) = 4.81018 /s. (b) t1/2 = ln 2/, so t1/2 = ln 2/(4.81018 /s) = 1.441017 s, which is 4.5 billion years.
301
E5023
(a) The decay constant for =
67
Ga can be derived from Eq. 508,
ln 2 ln 2 = = 2.461106 s1 . t1/2 (2.817105 s)
The activity is given by R = N , so we want to know how many atoms are present. That can be found from 1 atom 1u = 3.0771022 atoms. 3.42 g 1.66051024 g 66.93 u So the activity is R = (2.461106 /s1 )(3.0771022 atoms) = 7.5721016 decays/s. (b) After 1.728105 s the activity would have decreased to R = R0 et = (7.5721016 decays/s)e(2.46110 E5024 N = N0 et , but = ln 2/t1/2 , so N = N0 e ln 2t/t1/2 = N0 (2)t/t1/2 = N0 E5025 The remaining
223
6
/s1 )(1.728105 s)
= 4.9491016 decays/s.
1 2
t/t1/2
.
is
N = (4.71021 )(0.5)(28)/(11.43) = 8.61020 . The number of decays, each of which produced an alpha particle, is (4.71021 )  (8.61020 ) = 3.841021 . E5026 The amount remaining after 14 hours is m = (5.50 g)(0.5)(14)/(12.7) = 2.562 g. The amount remaining after 16 hours is m = (5.50 g)(0.5)(16)/(12.7) = 2.297 g. The difference is the amount which decayed during the two hour interval: (2.562 g)  (2.297 g) = 0.265 g. E5027 (a) Apply Eq. 507, R = R0 et . We first need to know the decay constant from Eq. 508, = And the the time is found from t 1 R =  ln , R0 1 (170 counts/s) =  ln , (5.618107 s1 ) (3050 counts/s) = 5.139106 s 59.5 days. 302 ln 2 ln 2 = = 5.618107 s1 . t1/2 (1.234106 s)
Note that counts/s is not the same as decays/s. Not all decay events will be picked up by a detector and recorded as a count; we are assuming that whatever scaling factor which connects the initial count rate to the initial decay rate is valid at later times as well. Such an assumption is a reasonable assumption. (b) The purpose of such an experiment would be to measure the amount of phosphorus that is taken up in a leaf. But the activity of the tracer decays with time, and so without a correction factor we would record the wrong amount of phosphorus in the leaf. That correction factor is R0 /R; we need to multiply the measured counts by this factor to correct for the decay. In this case 7 1 5 R = et = e(5.61810 s )(3.00710 s) = 1.184. R0 E5028 The number of particles of n = (0.15) The decay constant is = (120/s)/(6.1431020 ) = 1.951019 /s. The halflife is t1/2 = ln 2/(1.951019 /s) = 3.551018 s, or 110 Gy. E5029 The number of particles of n0 = The number which decay is n0  n = (3.0251022 ) 1  (0.5)(20000)/(24100) = 1.321022 . The mass of helium produced is then m= (0.004 kg/mol)(1.321022 ) = 8.78105 kg. (6.021023 mol1 )
239 147
Sm is
(0.001 kg)(6.021023 mol1 ) = 6.1431020 . (0.147 kg/mol)
Pu is
(0.012 kg)(6.021023 mol1 ) = 3.0231022 . (0.239 kg/mol)
E5030 Let R33 /(R33 + R32) = x, where x0 = 0.1 originally, and we want to find out at what time x = 0.9. Rearranging, (R33 + R32)/R33 = 1/x, so R32/R33 = 1/x  1. Since R = R0 (0.5)
t/t1/2
we can write a ratio 1 1= x 1  1 (0.5)t/t32 t/t33 . x0
Put in some of the numbers, and ln[(1/9)/(9)] = ln[0.5]t which has solution t = 209 d. 303 1 1  14.3 25.3 ,
E5031 E5032 (a) N/N0 = (0.5)(4500)/(82) = 3.01017 . (b) N/N0 = (0.5)(4500)/(0.034) = 0. E5033 The Q values are Q3 Q4 Q5 = (235.043923  232.038050  3.016029)(931.5 MeV) = 9.46 MeV, = (235.043923  231.036297  4.002603)(931.5 MeV) = 4.68 MeV, = (235.043923  230.033127  5.012228)(931.5 MeV) = 1.33 MeV.
Only reactions with positive Q values are energetically possible. E5034 (a) For the
14
C decay,
Q = (223.018497  208.981075  14.003242)(931.5 MeV) = 31.84 MeV. For the 4 He decay, Q = (223.018497  219.009475  4.002603)(931.5 MeV) = 5.979 MeV. E5035 Q = (136.907084  136.905821)(931.5 MeV) = 1.17 MeV. E5036 Q = (1.008665  1.007825)(931.5 MeV) = 0.782 MeV. E5037 (a) The kinetic energy of this electron is significant compared to the rest mass energy, so we must use relativity to find the momentum. The total energy of the electron is E = K + mc2 , the momentum will be given by pc = = E 2  m2 c4 = K 2 + 2Kmc2 , (1.00 MeV)2 + 2(1.00 MeV)(0.511 MeV) = 1.42 MeV.
The de Broglie wavelength is then = hc (1240 MeV fm) = = 873 fm. pc (1.42 MeV)
(b) The radius of the emitting nucleus is R = R0 A1/3 = (1.2 fm)(150)1/3 = 6.4 fm. (c) The longest wavelength standing wave on a string fixed at each end is twice the length of the string. Although the rules for standing waves in a box are slightly more complicated, it is a fair assumption that the electron could not exist as a standing a wave in the nucleus. (d) See part (c).
304
E5038 The electron is relativistic, so pc = E 2  m2 c4 , = (1.71 MeV + 0.51 MeV)2  (0.51 MeV)2 , = 2.16 MeV. This is also the magnitude of the momentum of the recoiling 32 S. Nonrelativistic relations are K = p2 /2m, so (2.16 MeV)2 K= = 78.4 eV. 2(31.97)(931.5 MeV) E5039 N = mNA /Mr will give the number of atoms of = ln 2/t1/2 will give the decay constant. Combining, m= Then for the sample in question m= (250)(3.71010 /s)(2.693)(86400 s)(198 g/mol) = 1.02103 g. ln 2(6.021023 /mol)
198
Au; R = N will give the activity;
Rt1/2 Mr N Mr = . NA ln 2NA
E5040 R = (8722/60 s)/(3.71010 /s) = 3.93109 Ci. E5041 The radiation absorbed dose (rad) is related to the roentgen equivalent man (rem) by the quality factor, so for the chest xray (25 mrem) = 29 mrad. (0.85) This is well beneath the annual exposure average. Each rad corresponds to the delivery of 105 J/g, so the energy absorbed by the patient is (0.029)(105 J/g) 1 2 (88 kg) = 1.28102 J.
E5042 (a) (75 kg)(102 J/kg)(0.024 rad) = 1.8102 J. (b) (0.024 rad)(12) = 0.29 rem. E5043 R = R0 (0.5)t/t1/2 , so R0 = (3.94 Ci)(2)(6.04810 E5044 (a) N = mNA /MR , so N= (2103 g)(6.021023 /mol) = 5.081018 . (239 g/mol)
5
s)/(1.82105 s)
= 39.4 Ci.
(b) R = N = ln 2N/t1/2 , so R = ln 2(5.081018 )/(2.411104 y)(3.15107 s/y) = 4.64106 /s. (c) R = (4.64106 /s)/(3.71010 decays/s Ci) = 1.25104 Ci. 305
E5045 The hospital uses a 6000 Ci source, and that is all the information we need to find the number of disintegrations per second: (6000 Ci)(3.71010 decays/s Ci) = 2.221014 decays/s. We are told the half life, but to find the number of radioactive nuclei present we want to know the decay constant. Then ln 2 ln 2 = = = 4.17109 s1 . t1/2 (1.66108 s) The number of
60
Co nuclei is then N= R (2.221014 decays/s) = = 5.321022 . (4.17109 s1 )
E5046 The annual equivalent does is (12104 rem/h)(20 h/week)(52 week/y) = 1.25 rem. E5047 (a) N = mNA /MR and MR = (226) + 2(35) = 296, so N= (1101 g)(6.021023 /mol) = 2.031020 . (296 g/mol)
(b) R = N = ln 2N/t1/2 , so R = ln 2(2.031020 )/(1600 y)(3.15107 s/y) = 2.8109 Bq. (c) (2.8109 )/(3.71010 ) = 76 mCi. E5048 R = N = ln 2N/t1/2 , so N= N = mNA /MR , so m= (40 g/mol)(9.91021 ) = 0.658 g. (6.021023 /mol) (4.6106 )(3.71010 /s)(1.28109 y)(3.15107 s/y) = 9.91021 , ln 2
E5049
We can apply Eq. 5018 to find the age of the rock, t = = = t1/2 NF ln 1 + , ln 2 NI (4.47109 y) (2.00103 g)/(206 g/mol) ln 1 + ln 2 (4.20103 g)/(238 g/mol) 2.83109 y.
,
306
E5050 The number of atoms of N=
238
U originally present is
(3.71103 g)(6.021023 /mol) = 9.381018 . (238 g/mol)
The number remaining after 260 million years is N = (9.381018 )(0.5)(260 My)/(4470 My) = 9.011018 . The difference decays into lead (eventually), so the mass of lead present should be m= (206 g/mol)(0.371018 ) = 1.27104 g. (6.021023 /mol)
E5051 We can apply Eq. 5018 to find the age of the rock, t = = = t1/2 NF ln 1 + , ln 2 NI (150106 g)/(206 g/mol) (4.47109 y) ln 1 + ln 2 (860106 g)/(238 g/mol) 1.18109 y.
40
,
Inverting Eq. 5018 to find the mass of
K originally present,
NF = 2t/t1/2  1, NI so (since they have the same atomic mass) the mass of m=
40
K is
(1.6103 g) = 1.78103 g. 2(1.18)/(1.28)  1
E5052 (a) There is an excess proton on the left and an excess neutron, so the unknown must be a deuteron, or d. (b) We've added two protons but only one (net) neutron, so the element is Ti and the mass number is 43, or 43 Ti. (c) The mass number doesn't change but we swapped one proton for a neutron, so 7 Li. E5053 Do the math: Q = (58.933200 + 1.007825  58.934352  1.008665)(931.5 MeV) = 1.86 MeV. E5054 The reactions are
201
197
Hg(, )197 Pt, Au(n, p)197 Pt, 196 Pt(n, )197 Pt, 198 Pt(, n)197 Pt, 196 Pt(d, p)197 Pt, 198 Pt(p, d)197 Pt.
307
E5055 We will write these reactions in the same way as Eq. 5020 represents the reaction of Eq. 5019. It is helpful to work backwards before proceeding by asking the following question: what nuclei will we have if we subtract one of the allowed projectiles? The goal is 60 Co, which has 27 protons and 60  27 = 33 neutrons. 1. Removing a proton will leave 26 protons and 33 neutrons, which is unstable. 2. Removing a neutron will leave 27 protons and 32 neutrons, which is stable. 3. Removing a deuteron will leave 26 protons and 32 neutrons, which is stable.
59
Fe; but that nuclide is
59
Co; and that nuclide is Fe; and that nuclide is
58
It looks as if only 59 Co(n)60 Co and 58 Fe(d)60 Co are possible. If, however, we allow for the possibility of other daughter particles we should also consider some of the following reactions. 1. Swapping a neutron for a proton:
60
Ni(n,p)60 Co.
61
2. Using a neutron to knock out a deuteron:
Ni(n,d)60 Co.
63
3. Using a neutron to knock out an alpha particle:
Cu(n,)60 Co. Ni(d,)60 Co.
61
4. Using a deuteron to knock out an alpha particle:
62
E5056 (a) The possible results are 64 Zn, 66 Zn, 64 Cu, 66 Cu, (b) The stable results are 64 Zn, 66 Zn, 61 Ni, and 67 Zn. E5057 E5058 The resulting reactions are E5059
194
Ni,
63
Ni,
65
Zn, and
67
Zn.
Pt(d,)192 Ir,
196
Pt(d,)194 Ir, and
198
Pt(d,)196 Ir.
E5060 Shells occur at numbers 2, 8, 20, 28, 50, 82. The shells occur separately for protons and neutrons. To answer the question you need to know both Z and N = A  Z of the isotope. (a) Filled shells are 18 O, 60 Ni, 92 Mo, 144 Sm, and 207 Pb. (b) One nucleon outside a shell are 40 K, 91 Zr, 121 Sb, and 143 Nd. (c) One vacancy in a shell are 13 C, 40 K, 49 Ti, 205 Tl, and 207 Pb. E5061 (a) The binding energy of this neutron can be found by considering the Q value of the reaction 90 Zr(n)91 Zr which is (89.904704 + 1.008665  90.905645)(931.5 MeV) = 7.19 MeV.
89
(b) The binding energy of this neutron can be found by considering the Q value of the reaction Zr(n)90 Zr which is (88.908889 + 1.008665  89.904704)(931.5 MeV) = 12.0 MeV.
This neutron is bound more tightly that the one in part (a). (c) The binding energy per nucleon is found by dividing the binding energy by the number of nucleons: (401.007825 + 511.008665  90.905645)(931.5 MeV) = 8.69 MeV. 91 The neutron in the outside shell of 91 Zr is less tightly bound than the average nucleon in 91 Zr. 308
P501 Before doing anything we need to know whether or not the motion is relativistic. The rest mass energy of an particle is mc2 = (4.00)(931.5 MeV) = 3.73 GeV, and since this is much greater than the kinetic energy we can assume the motion is nonrelativistic, and we can apply nonrelativistic momentum and energy conservation principles. The initial velocity of the particle is then v= 2K/m = c 2K/mc2 = c 2(5.00 MeV)/(3.73 GeV) = 5.18102 c.
For an elastic collision where the second particle is at originally at rest we have the final velocity of the first particle as v 1,f = v 1,i m2  m1 (4.00u)  (197u) = (5.18102 c) = 4.97102 c, m2 + m1 (4.00u) + (197u)
while the final velocity of the second particle is v 2,f = v 1,i 2m1 2(4.00u) = (5.18102 c) = 2.06103 c. m2 + m1 (4.00u) + (197u)
(a) The kinetic energy of the recoiling nucleus is K= 1 1 mv 2 = m(2.06103 c)2 = (2.12106 )mc2 2 2 = (2.12106 )(197)(931.5 MeV) = 0.389 MeV.
(b) Energy conservation is the fastest way to answer this question, since it is an elastic collision. Then (5.00 MeV)  (0.389 MeV) = 4.61 MeV. P502 The gamma ray carries away a mass equivalent energy of m = (2.2233 MeV)/(931.5 MeV/u) = 0.002387 u. The neutron mass would then be mN = (2.014102  1.007825 + 0.002387)u = 1.008664 u. P503 (a) There are four substates: mj can be +3/2, +1/2, 1/2, and 3/2. (b) E = (2/3)(3.26)(3.15108 eV/T)(2.16 T) = 1.48107 eV. (c) = (1240 eV nm)/(1.48107 eV) = 8.38 m. (d) This is in the radio region. P504 (a) The charge density is = 3Q/4R3 . The charge on the shell of radius r is dq = 4r2 dr. The potential at the surface of a solid sphere of radius r is V = q r2 = . 4 0 r 3 0
The energy required to add a layer of charge dq is dU = V dq = 309 42 r4 dr, 3 0
which can be integrated to yield U= (b) For
239
42 R5 3Q2 = . 3 0 20 0 R
Pu, U= 3(94)2 (1.61019 C) = 1024106 eV. 20(8.851012 F/m)(7.451015 m)
(c) The electrostatic energy is 10.9 MeV per proton. P505 The decay rate is given by R = N , where N is the number of radioactive nuclei present. If R exceeds P then nuclei will decay faster than they are produced; but this will cause N to decrease, which means R will decrease until it is equal to P . If R is less than P then nuclei will be produced faster than they are decaying; but this will cause N to increase, which means R will increase until it is equal to P . In either case equilibrium occurs when R = P , and it is a stable equilibrium because it is approached no matter which side is larger. Then P = R = N at equilibrium, so N = P/. P506 (a) A = N ; at equilibrium A = P , so P = 8.881010 /s. (b) (8.881010 /s)(1e0.269t ), where t is in hours. The factor 0.269 comes from ln(2)/(2.58) = . (c) N = P/ = (8.881010 /s)(3600 s/h)/(0.269/h) = 1.191015 . (d) m = N Mr /NA , or m= P507 (a) A = N , so A= ln 2mNA ln 2(1103 g)(6.021023 /mol) = = 3.66107 /s. t1/2 Mr (1600)(3.15107 s)(226 g/mol) (1.191015 )(55.94 g/mol) = 1.10107 g. (6.021023 /mol)
(b) The rate must be the same if the system is in secular equilibrium. (c) N = P/ = t1/2 P/ ln 2, so m= P508 (3.82)(86400 s)(3.66107 /s)(222 g/mol) = 6.43109 g. (6.021023 /mol) ln 2
The number of water molecules in the body is N = (6.021023 /mol)(70103 g)/(18 g/mol) = 2.341027 .
There are ten protons in each water molecule. The activity is then A = (2.341027 ) ln 2/(11032 y) = 1.62105 /y. The time between decays is then 1/A = 6200 y.
310
P509 Assuming the 238 U nucleus is originally at rest the total initial momentum is zero, which means the magnitudes of the final momenta of the particle and the 234 Th nucleus are equal. The particle has a final velocity of v= 2K/m = c 2K/mc2 = c 2(4.196 MeV)/(4.0026931.5 MeV) = 4.744102 c.
234
Since the magnitudes of the final momenta are the same, the of (4.744102 c) The kinetic energy of the K=
234
Th nucleus has a final velocity
(4.0026 u) (234.04 u)
= 8.113104 c.
Th nucleus is
1 1 mv 2 = m(8.113104 c)2 = (3.291107 )mc2 2 2 = (3.291107 )(234.04)(931.5 MeV) = 71.75 keV.
The Q value for the reaction is then (4.196 MeV) + (71.75 keV) = 4.268 MeV, which agrees well with the Sample Problem. P5010 (a) The Q value is Q = (238.050783  4.002603  234.043596)(931.5 MeV) = 4.27 MeV. (b) The Q values for each step are Q = (238.050783  237.048724  1.008665)(931.5 MeV) = 6.153 MeV, Q = (237.048724  236.048674  1.007825)(931.5 MeV) = 7.242 MeV, Q = (236.048674  235.045432  1.008665)(931.5 MeV) = 5.052 MeV, Q = (235.045432  234.043596  1.007825)(931.5 MeV) = 5.579 MeV. (c) The total Q for part (b) is 24.026 MeV. The difference between (a) and (b) is 28.296 MeV. The binding energy for the alpha particle is E = [2(1.007825) + 2(1.008665)  4.002603](931.5 MeV) = 28.296 MeV. P5011 (a) The emitted positron leaves the atom, so the mass must be subtracted. But the daughter particle now has an extra electron, so that must also be subtracted. Hence the factor 2me . (b) The Q value is Q = [11.011434  11.009305  2(0.0005486)](931.5 MeV) = 0.961 MeV. P5012 (a) Capturing an electron is equivalent to negative beta decay in that the total number of electrons is accounted for on both the left and right sides of the equation. The loss of the K shell electron, however, must be taken into account as this energy may be significant. (b) The Q value is Q = (48.948517  48.947871)(931.5 MeV)  (0.00547 MeV) = 0.596 MeV. 311
P5013
The decay constant for =
90
Sr is
ln 2 ln 2 = = 7.581010 s1 . t1/2 (9.15108 s)
90
The number of nuclei present in 400 g of N = (400 g) so the overall activity of the 400 g of
90
Sr is
(6.021023 /mol) = 2.681024 , (89.9 g/mol)
Sr is
R = N = (7.581010 s1 )(2.681024 )/(3.71010 /Ci s) = 5.49104 Ci. This is spread out over a 2000 km2 area, so the "activity surface density" is (5.49104 Ci) = 2.74105 Ci/m2 . (20006 m2 ) If the allowable limit is 0.002 mCi, then the area of land that would contain this activity is (0.002103 Ci) = 7.30102 m2 . (2.74105 Ci/m2 ) P5014 (a) N = mNA /Mr , so N = (2.5103 g)(6.021023 /mol)/(239 g/mol) = 6.31018 . (b) A = ln 2N/t1/2 , so the number that decay in 12 hours is ln 2(6.31018 )(12)(3600 s) = 2.51011 . (24100)(3.15107 s) (c) The energy absorbed by the body is E = (2.51011 )(5.2 MeV)(1.61019 J/eV) = 0.20 J. (d) The dose in rad is (0.20 J)/(87 kg) = 0.23 rad. (e) The biological dose in rem is (0.23)(13) = 3 rem. P5015 (a) The amount of
238
U per kilogram of granite is
N= The activity is then
(4106 kg)(6.021023 /mol) = 1.011019 . (0.238 kg/mol) ln 2(1.011019 ) = 49.7/s. (4.47109 y)(3.15107 s/y)
A=
The energy released in one second is E = (49.7/s)(51.7 MeV) = 4.11010 J. The amount of
232
Th per kilogram of granite is N= (13106 kg)(6.021023 /mol) = 3.371019 . (0.232 kg/mol) 312
The activity is then A= ln 2(3.371019 ) = 52.6/s. (1.411010 y)(3.15107 s/y)
The energy released in one second is E = (52.6/s)(42.7 MeV) = 3.61010 J. The amount of
40
K per kilogram of granite is N= (4106 kg)(6.021023 /mol) = 6.021019 . (0.040 kg/mol) ln 2(6.021019 ) = 1030/s. (1.28109 y)(3.15107 s/y)
The activity is then A=
The energy released in one second is E = (1030/s)(1.32 MeV) = 2.21010 J. The total of the three is 9.91010 W per kilogram of granite. (b) The total for the Earth is 2.71013 W. P5016 (a) Since only a is moving originally then the velocity of the center of mass is V = ma va + mX (0) ma = va . mX + ma ma + mX
No, since momentum is conserved. (b) Moving to the center of mass frame gives the velocity of X as V , and the velocity of a as va  V . The kinetic energy is now K cm 1 mX V 2 + ma (va  V )2 , 2 2 va m2 m2 a X = mX + ma 2 2 (ma + mX ) (ma + mX )2 2 ma va ma mX + m2 X = , 2 (ma + mX )2 mX = K lab . ma + mX =
,
Yes; kinetic energy is not conserved. (c) va = 2K/m, so va = The center of mass velocity is V = (0.130c) Finally, K cm = (15.9 MeV) (90) = 15.6 MeV. (2) + (90) 313 (2) = 2.83103 c. (2) + (90) 2(15.9 MeV)/(1876 MeV)c = 0.130c.
P5017 P5018
Let Q = K cm in the result of Problem 5016, and invert, solving for K lab . (a) Removing a proton from
209
Bi:
E = (207.976636 + 1.007825  208.980383)(931.5 MeV) = 3.80 MeV. Removing a proton from
208
Pb:
E = (206.977408 + 1.007825  207.976636)(931.5 MeV) = 8.01 MeV. (b) Removing a neutron from
209
Pb:
E = (207.976636 + 1.008665  208.981075)(931.5 MeV) = 3.94 MeV. Removing a neutron from
208
Pb:
E = (206.975881 + 1.008665  207.976636)(931.5 MeV) = 7.37 MeV.
314
E511 (a) For the coal, m = (1109 J)/(2.9107 J/kg) = 34 kg. (b) For the uranium, m = (1109 J)/(8.21013 J/kg) = 1.2105 kg. E512 (a) The energy from the coal is E = (100 kg)(2.9107 J/kg) = 2.9109 J. (b) The energy from the uranium in the ash is E = (3106 )(100 kg)(8.21013 J) = 2.51010 J. E513 (a) There are (1.00 kg)(6.021023 mol1 ) = 2.561024 (235g/mol) atoms in 1.00 kg of 235 U. (b) If each atom releases 200 MeV, then (200106 eV)(1.61019 J/ eV)(2.561024 ) = 8.191013 J of energy could be released from 1.00 kg of 235 U. (c) This amount of energy would keep a 100W lamp lit for t= (8.191013 J) = 8.191011 s 26, 000 y! (100 W)
E514 2 W = 1.251019 eV/s. This requires (1.251019 eV/s)/(200106 eV) = 6.251010 /s as the fission rate. E515 There are (1.00 kg)(6.021023 mol1 ) = 2.561024 (235g/mol)
235
atoms in 1.00 kg of
U. If each atom releases 200 MeV, then
(200106 eV)(1.61019 J/ eV)(2.561024 ) = 8.191013 J of energy could be released from 1.00 kg of 235 U. This amount of energy would keep a 100W lamp lit for (8.191013 J) t= = 8.191011 s 30, 000 y! (100 W) E516 There are (1.00 kg)(6.021023 mol1 ) = 2.521024 (239g/mol)
239
atoms in 1.00 kg of
Pu. If each atom releases 180 MeV, then
(180106 eV)(1.61019 J/ eV)(2.521024 ) = 7.251013 J of energy could be released from 1.00 kg of
239
Pu. 315
E517 When the 233 U nucleus absorbs a neutron we are given a total of 92 protons and 142 neutrons. Gallium has 31 protons and around 39 neutrons; chromium has 24 protons and around 28 neutrons. There are then 37 protons and around 75 neutrons left over. This would be rubidium, but the number of neutrons is very wrong. Although the elemental identification is correct, because we must conserve proton number, the isotopes are wrong in our above choices for neutron numbers. E518 Beta decay is the emission of an electron from the nucleus; one of the neutrons changes into a proton. The atom now needs one more electron in the electron shells; by using atomic masses (as opposed to nuclear masses) then the beta electron is accounted for. This is only true for negative beta decay, not for positive beta decay. E519 (a) There are (1.0 g)(6.021023 mol1 ) = 2.561021 (235g/mol) atoms in 1.00 g of
235
U. The fission rate is
A = ln 2N/t1/2 = ln 2(2.561021 )/(3.51017 y)(365d/y) = 13.9/d. (b) The ratio is the inverse ratio of the halflives: (3.51017 y)/(7.04108 y) = 4.97108 . E5110 (a) The atomic number of Y must be 92  54 = 38, so the element is Sr. The mass number is 235 + 1  140  1 = 95, so Y is 95 Sr. (b) The atomic number of Y must be 92  53 = 39, so the element is Y. The mass number is 235 + 1  139  2 = 95, so Y is 95 Y. (c) The atomic number of X must be 92  40 = 52, so the element is Te. The mass number is 235 + 1  100  2 = 134, so X is 134 Te. (d) The mass number difference is 235 + 1  141  92 = 3, so b = 3. E5111 The Q value is Q = [51.94012  2(25.982593)](931.5 MeV) = 23 MeV. The negative value implies that this fission reaction is not possible. E5112 The Q value is Q = [97.905408  2(48.950024)](931.5 MeV) = 4.99 MeV. The two fragments would have a very large Coulomb barrier to overcome. E5113 The energy released is (235.043923  140.920044  91.919726  21.008665)(931.5 MeV) = 174 MeV. E5114 Since En > Eb fission is possible by thermal neutrons. E5115 (a) The uranium starts with 92 protons. The two end products have a total of 58 + 44 = 102. This means that there must have been ten beta decays. (b) The Q value for this process is Q = (238.050783 + 1.008665  139.905434  98.905939)(931.5 MeV) = 231 MeV. 316
E5116 (a) The other fragment has 92  32 = 60 protons and 235 + 1  83 = 153 neutrons. That element is 153 Nd. (b) Since K = p2 /2m and momentum is conserved, then 2m1 K1 = 2m2 K2 . This means that K2 = (m1 /m2 )K1 . But K1 + K2 = Q, so K1 or K1 = with a similar expression for K2 . Then for K= while for
153 83
m2 + m1 = Q, m2 m2 Q, m1 + m2
Ge
(153) (170 MeV) = 110 MeV, (83 + 153) (83) (170 MeV) = 60 MeV, (83 + 153) 2K = m 2K = m 2(110 MeV) c = 0.053c, (83)(931 MeV) 2(60 MeV) c = 0.029c. (153)(931 MeV)
Nd K=
(c) For
83
Ge, v=
while for
153
Nd v=
E5117 Since 239 Pu is one nucleon heavier than 238 U only one neutron capture is required. The atomic number of Pu is two more than U, so two beta decays will be required. The reaction series is then
238
U+n 239 U 239 Np
239 239
U, Np +  + , 239 Pu +  + .
E5118 Each fission releases 200 MeV. The total energy released over the three years is (190106 W)(3)(3.15107 s) = 1.81016 J. That's (1.81016 J)/(1.61019 J/eV)(200106 eV) = 5.61026 fission events. That requires m = (5.61026 )(0.235 kg/mol)/(6.021023 /mol) = 218 kg. But this is only half the original amount, or 437 kg. E5119 According to Sample Problem 513 the rate at which nonfission thermal neutron capture occurs is one quarter that of fission. Hence the mass which undergoes nonfission thermal neutron capture is one quarter the answer of Ex. 5118. The total is then (437 kg)(1 + 0.25) = 546 kg. 317
E5120 (a) Qeff = E/N , where E is the total energy released and N is the number of decays. This can also be written as P t1/2 P t1/2 Mr P = = , Qeff = A ln 2N ln 2NA m where A is the activity and P the power output from the sample. Solving, Qeff = (2.3 W)(29 y)(3.15107 s)(90 g/mol) = 4.531013 J = 2.8 MeV. ln 2(6.021023 /mol)(1 g)
(b) P = (0.05)m(2300 W/kg), so m= (150 W) = 1.3 kg. (0.05)(2300 W/kg)
E5121 Let the energy released by one fission be E1 . If the average time to the next fission event is tgen , then the "average" power output from the one fission is P1 = E1 /tgen . If every fission event results in the release of k neutrons, each of which cause a later fission event, then after every time period tgen the number of fission events, and hence the average power output from all of the fission events, will increase by a factor of k. For long enough times we can write P (t) = P0 k t/tgen . E5122 Invert the expression derived in Exercise 5121: k= P P0
tgen /t
=
(350) (1200)
(1.3103 s)/(2.6 s)
= 0.99938.
E5123 Each fission releases 200 MeV. Then the fission rate is (500106 W)/(200106 eV)(1.61019 J/eV) = 1.61019 /s The number of neutrons in "transit" is then (1.61019 /s)(1.0103 s) = 1.61016 . E5124 Using the results of Exercise 5121: P = (400 MW)(1.0003)(300 s)/(0.03 s) = 8030 MW. E5125 The time constant for this decay is = ln 2 = 2.501010 s1 . (2.77109 s)
The number of nuclei present in 1.00 kg is N= The decay rate is then R = N = (2.501010 s1 )(2.531024 ) = 6.331014 s1 . The power generated is the decay rate times the energy released per decay, P = (6.331014 s1 )(5.59106 eV)(1.61019 J/eV) = 566 W. 318 (1.00 kg)(6.021023 mol1 ) = 2.531024 . (238 g/mol)
E5126 The detector detects only a fraction of the emitted neutrons. This fraction is A (2.5 m2 ) = = 1.62104 . 2 4R 4(35 m)2 The total flux out of the warhead is then (4.0/s)/(1.62104 ) = 2.47104 /s. The number of
239
Pu atoms is (2.47104 /s)(1.341011 y)(3.15107 s/y) A = = 6.021022 . ln 2(2.5)
N=
That's one tenth of a mole, so the mass is (239)/10 = 24 g. E5127 Using the results of Sample Problem 514, t= so t= ln[R(0)/R(t)] , 5  8
ln[(0.03)/(0.0072)] = 1.72109 y. (0.984  0.155)(1109 /y)
E5128 (a) (15109 W y)(2105 y) = 7.5104 W. (b) The number of fissions required is N= The mass of
235
(15109 W y)(3.15107 s/y) = 1.51028 . (200 MeV)(1.61019 J/eV)
U consumed is m = (1.51028 )(0.235kg/mol)/(6.021023 /mol) = 5.8103 kg.
E5129 and then
239
If 238 U absorbs a neutron it becomes 239 U, which will decay by beta decay to first 239 Np Pu; we looked at this in Exercise 5117. This can decay by alpha emission according to
239
Pu 235 U + .
E5130 The number of atoms present in the sample is N = (6.021023 /mol)(1000 kg)/(2.014g/mol) = 2.991026 . It takes two to make a fusion, so the energy released is (3.27 MeV)(2.991026 )/2 = 4.891026 MeV. That's 7.81013 J, which is enough to burn the lamp for t = (7.81013 J)/(100 W) = 7.81011 s = 24800 y. E5131 The potential energy at closest approach is U= (1.61019 C)2 = 9105 eV. 4(8.851012 F/m)(1.61015 m) 319
E5132 The ratio can be written as n(K1 ) = n(K2 ) so the ratio is (5000 eV) (3100 eV)/(8.62105 eV/K)(1.5107 K) e = 0.15. (1900 eV) E5133 (a) See Sample Problem 515. E5134 Add up all of the Q values in the cycle of Fig. 5110. E5135 The energy released is (34.002603  12.0000000)(931.5 MeV) = 7.27 MeV. E5136 (a) The number of particle of hydrogen in 1 m3 is N = (0.35)(1.5105 kg)(6.021023 /mol)/(0.001 kg/mol) = 3.161031 (b) The density of particles is N/V = p/kT ; the ratio is (3.161031 )(1.381023 J/K)(298 K) = 1.2106 . (1.01105 Pa) E5137 (a) There are (1.00 kg)(6.021023 mol1 ) = 6.021026 (1g/mol) atoms in 1.00 kg of 1 H. If four atoms fuse to releases 26.7 MeV, then (26.7 MeV)(6.021026 )/4 = 4.01027 MeV of energy could be released from 1.00 kg of 1 H. (b) There are (1.00 kg)(6.021023 mol1 ) = 2.561024 (235g/mol) atoms in 1.00 kg of
235
K1 (K2 K1 )/kT e , K2
U. If each atom releases 200 MeV, then (200 MeV)(2.561024 ) = 5.11026 MeV
of energy could be released from 1.00 kg of E5138 (a) E = mc2 , so m =
235
U.
(3.91026 J/s) = 4.3109 kg/s. (3.0108 m/s)2
(b) The fraction of the Sun's mass "lost" is (4.3109 kg/s)(3.15107 s/y)(4.5109 y) = 0.03 %. (2.01030 kg) 320
E5139 The rate of consumption is 6.21011 kg/s, the core has 1/8 the mass but only 35% is hydrogen, so the time remaining is t = (0.35)(1/8)(2.01030 kg)/(6.21011 kg/s) = 1.41017 s, or about 4.5109 years. E5140 For the first two reactions into one: Q = [2(1.007825)  (2.014102)](931.5 MeV) = 1.44 MeV. For the second, Q = [(1.007825) + (2.014102)  (3.016029)](931.5 MeV) = 5.49 MeV. For the last, Q = [2(3.016029)  (4.002603)  2(1.007825)](931.5 MeV) = 12.86 MeV. E5141 (a) Use mNA /Mr = N , so (3.3107 J/kg) 1 (0.012 kg/mol) = 4.1 eV. (6.021023 /mol) (1.61019 J/eV)
(b) For every 12 grams of carbon we require 32 grams of oxygen, the total is 44 grams. The total mass required is then 40/12 that of carbon alone. The energy production is then (3.3107 J/kg)(12/44) = 9106 J/kg. (c) The sun would burn for (21030 kg)(9106 J/kg) = 4.61010 s. (3.91026 W) That's only 1500 years! E5142 The rate of fusion events is (5.31030 W) = 4.561042 /s. (7.27106 eV)(1.61019 J/eV) The carbon is then produced at a rate (4.561042 /s)(0.012 kg/mol)/(6.021023 /mol) = 9.081016 kg/s. The process will be complete in (4.61032 kg) = 1.6108 y. (9.081016 kg/s)(3.15107 s/y) E5143 (a) For the reaction dd, Q = [2(2.014102)  (3.016029)  (1.008665)](931.5 MeV) = 3.27 MeV. (b) For the reaction dd, Q = [2(2.014102)  (3.016029)  (1.007825)](931.5 MeV) = 4.03 MeV. (c) For the reaction dt, Q = [(2.014102) + (3.016049)  (4.002603)  (1.008665)](931.5 MeV) = 17.59 MeV. 321
E5144 One liter of water has a mass of one kilogram. The number of atoms of 2 H is (0.00015 kg) The energy available is (3.27106 eV)(1.61019 J/eV)(4.51022 )/2 = 1.181010 J. The power output is then (1.181010 J) = 1.4105 W (86400 s) E5145 Assume momentum conservation, then p = pn or v n /v = m /mn . The ratio of the kinetic energies is then Kn mn v 2 m n = = 4. 2 K m v mn Then K n = 4Q/5 = 14.07 MeV while K = Q/5 = 3.52 MeV. E5146 The Q value is Q = (6.015122 + 1.008665  3.016049  4.002603)(931.5 MeV) = 4.78 MeV. Combine the two reactions to get a net Q = 22.37 MeV. The amount of 6 Li required is N = (2.61028 MeV)/(22.37 MeV) = 1.161027 . The mass of LiD required is m= (1.161027 )(0.008 kg/mol) = 15.4 kg. (6.021023 /mol) (6.021023 /mol) = 4.51022 . (0.002 kg/mol)
P511
(a) Equation 501 is R = R0 A1/3 ,
where R0 = 1.2 fm. The distance between the two nuclei will be the sum of the radii, or R0 (140)1/3 + (94)1/3 . The potential energy will be U = = = = 1 q1 q2 , 4 0 r e2 (54)(38) , 4 0 R0 (140)1/3 + (94)1/3 (1.601019 C)2 211, 4(8.851012 C2 /Nm2 )(1.2 fm) 253 MeV.
(b) The energy will eventually appear as thermal energy. 322
P512 (a) Since R = R0 3 A, the surface area a is proportional to A2/3 . The fractional change in surface area is (a1 + a2 )  a0 (140)2/3 + (96)2/3  (236)2/3 = = 25 %. a0 (236)2/3 (b) Nuclei have a constant density, so there is no change in volume. (c) Since U Q2 /R, U Q2 / 3 A. The fractional change in the electrostatic potential energy is U1 + U2  U0 (54)2 (140)1/3 + (38)2 (96)1/3  (92)2 (236)1/3 = = 36 %. U0 (92)2 (236)1/3 P513 (a) There are (2.5 kg)(6.021023 mol1 ) = 6.291024 (239g/mol) atoms in 2.5 kg of
239
Pu. If each atom releases 180 MeV, then
(180 MeV)(6.291024 )/(2.61028 MeV/megaton) = 44 kiloton is the bomb yield. P514 (a) In an elastic collision the nucleus moves forward with a speed of v = v0 so the kinetic energy when it moves forward is K = 4m2 mn m m 2 n v0 =K , 2 (m + mn )2 (mn + m)2 2mn , mn + m
where we can write K because in an elastic collision whatever energy kinetic energy the nucleus carries off had to come from the neutron. (b) For hydrogen, K 4(1)(1) = = 1.00. K (1 + 1)2 For deuterium, K 4(1)(2) = = 0.89. K (1 + 2)2 For carbon, K 4(1)(12) = = 0.28. K (1 + 12)2 For lead, K 4(1)(206) = = 0.019. K (1 + 206)2 (c) If each collision reduces the energy by a factor of 10.89 = 0.11, then the number of collisions required is the solution to (0.025 eV) = (1106 eV)(0.11)N , which is N = 8.
323
P515
The radii of the nuclei are 3 R = (1.2 fm) 7 = 2.3 fm.
The using the derivation of Sample Problem 515, K= P516 (3)2 (1.61019 C)2 = 1.4106 eV. 16(8.851012 F/m)(2.31015 m)
(a) Add up the six equations to get
12
C
+1 H +13 N +13 C +1 H +14 N +1 H +15 O +15 N +1 H 13 N + +13 C + e+ + +14 N + +15 O + +15 N + e+ + +12 C +4 He.
Cancel out things that occur on both sides and get
1
H +1 H +1 H +1 H + e+ + + + + e+ + +4 He.
(b) Add up the Q values, and then add on 4(0.511 MeV for the annihilation of the two positrons. P517 (a) Demonstrating the consistency of this expression is considerably easier than deriving it from first principles. From Problem 504 we have that a uniform sphere of charge Q and radius R has potential energy 3Q2 U= . 20 0 R This expression was derived from the fundamental expression dU = For gravity the fundamental expression is dU = Gm dm , r 1 q dq . 4 0 r
so we replace 1/4 0 with G and Q with M . But like charges repel while all masses attract, so we pick up a negative sign. (b) The initial energy would be zero if R = , so the energy released is U= 3GM 2 3(6.71011 Nm2 /kg2 )(2.01030 kg)2 = = 2.31041 J. 5R 5(7.0108 m)
At the current rate (see Sample Problem 516), the sun would be t= or 187 million years old. (2.31041 J) = 5.91014 s, (3.91026 W)
324
P518
(a) The rate of fusion events is (3.91026 W) = 9.31037 /s. (26.2106 eV)(1.61019 J/eV)
Each event produces two neutrinos, so the rate is 1.861038 /s. (b) The rate these neutrinos impinge on the Earth is proportional to the solid angle subtended by the Earth as seen from the Sun: r2 (6.37106 m)2 = = 4.51010 , 2 4R 4(1.501011 m)2 so the rate of neutrinos impinging on the Earth is (1.861038 /s)(4.51010 ) = 8.41028 /s. P519 (a) Reaction A releases, for each d (1/2)(4.03 MeV) = 2.02 MeV, Reaction B releases, for each d (1/3)(17.59 MeV) + (1/3)(4.03 MeV) = 7.21 MeV. Reaction B is better, and releases (7.21 MeV)  (2/02 MeV) = 5.19 MeV more for each N . P5110 (a) The mass of the pellet is m= The number of dt pairs is N= (6.71012 kg)(6.021023 /mol) = 8.061014 , (0.005 kg/mol) 4 (2.0105 m)3 (200 kg/m3 ) = 6.71012 kg. 3
and if 10% fuse then the energy release is (17.59 MeV)(0.1)(8.061014 )(1.61019 J/eV) = 230 J. (b) That's (230 J)/(4.6106 J/kg) = 0.05 kg of TNT. (c) The power released would be (230 J)(100/s) = 2.3104 W.
325
E521 (a) The gravitational force is given by Gm2 /r2 , while the electrostatic force is given by q 2 /4 0 r2 . The ratio is 4 0 Gm2 q2 = = 4(8.851012 C2 /Nm2 )(6.671011 Nm2 /kg2 )(9.111031 kg)2 , (1.601019 C)2 2.41043 .
Gravitational effects would be swamped by electrostatic effects at any separation. (b) The ratio is 4 0 Gm2 q2 = = 4(8.851012 C2 /Nm2 )(6.671011 Nm2 /kg2 )(1.671027 kg)2 , (1.601019 C)2 8.11037 .
E522 (a) Q = 938.27 MeV  0.511 MeV) = 937.76 MeV. (b) Q = 938.27 MeV  135 MeV) = 803 MeV. E523 The gravitational force from the lead sphere is 4Gme R Gme M = . R2 3 Setting this equal to the electrostatic force from the proton and solving for R, R= or 3(1.61019 C)2 16 2 (8.851012 F/m)(6.671011 Nm2 /kg2 )(11350 kg/m3 )(9.111031 kg)(5.291011 m)2 which means R = 2.851028 m. E524 Each takes half the energy of the pion, so = (1240 MeV fm) = 18.4 fm. (135 MeV)/2 16 2 3e2 2, 0 Gme a0
E525
The energy of one of the pions will be E= (pc)2 + (mc2 )2 = (358.3 MeV)2 + (140 MeV)2 = 385 MeV.
There are two of these pions, so the rest mass energy of the 0 is 770 MeV. E526 E = mc2 , so = (1.5106 eV)/(20 eV) = 7.5104 . The speed is given by v = c 1  1/ 2 c  c/2 2 , where the approximation is true for large . Then v = c/2(7.5104 )2 = 2.7102 m/s. 326
E527 d = ct = hc/2E. Then d= (1240 MeV fm) = 2.16103 fm. 2(91200 MeV)
E528 (a) Electromagnetic. (b) Weak, since neutrinos are present. (c) Strong. (d) Weak, since strangeness changes. E529 (a) Baryon number is conserved by having two "p" on one side and a "p" and a 0 on the other. Charge will only be conserved if the particle x is positive. Strangeness will only be conserved if x is strange. Since it can't be a baryon it must be a meson. Then x is K + . (b) Baryon number on the left is 0, so x must be an antibaryon. Charge on the left is zero, so x must be neutral because "n" is neutral. Strangeness is everywhere zero, so the particle must be n. (c) There is one baryon on the left and one on the right, so x has baryon number 0. The charge on the left adds to zero, so x is neutral. The strangeness of x must also be 0, so it must be a 0 . E5210 neutral. neutron possible There are two positive on the left, and two on the right. The antineutron must then be The baryon number on the right is one, that on the left would be two, unless the antihas a baryon number of minus one. There is no strangeness on the right or left, except the antineutron, so it must also have strangeness zero.
E5211 (a) Annihilation reactions are electromagnetic, and this involves s. s (b) This is neither weak nor electromagnetic, so it must be strong. (c) This is strangeness changing, so it is weak. (d) Strangeness is conserved, so this is neither weak nor electromagnetic, so it must be strong. E5212 (a) K0 e+ + e , (b) K0 + + 0 , (c) K0 + + + +  , (d) K0 + + 0 + 0 , E5213 (a) 0 p + + . (b) n p + e+ + e . (c) + + + + . (d) K  + . E5214 E5215 From top to bottom, they are ++ , + , 0 , + , 0 , 0 ,  ,  ,  , and  . E5216 (a) This is not possible. (b) uuu works. E5217 A strangeness of +1 corresponds to the existence of an antiquark, which has a charge s of +1/3. The only quarks that can combine with this antiquark to form a meson will have charges of 1/3 or +2/3. It is only possible to have a net charge of 0 or +1. The reverse is true for strangeness 1.
327
E5218 Put bars over everything. For the antiproton, uudZ, for the antineutron, udd. quarks u c d c s c c c c u cd c s Q 0 1 1 0 0 1 1 S 0 0 1 0 0 0 1 C 1 1 1 0 1 1 1 particle D0 D D s c D0 D+ D+ s
E5219 We'll construct a table:
E5220 (a) Write the quark content out then cancel out the parts which are the same on both sides: dds udd + d, u so the fundamental process is s u + d + u. (b) Write the quark content out then cancel out the parts which are the same on both sides: d ud + d, s u so the fundamental process is u + d + u. s (c) Write the quark content out then cancel out the parts which are the same on both sides: ud + uud uus + u, s so the fundamental process is d + d s + . s (d) Write the quark content out then cancel out the parts which are the same on both sides: + udd uud + d, u so the fundamental process is u + u. E5221 The slope is (7000 km/s) = 70 km/s Mpc. (100 Mpc) E5222 c = Hd, so d = (3105 km/s)/(72 km/s Mpc) = 4300 Mpc. E5223 The question should read "What is the..." The speed of the galaxy is v = Hd = (72 km/s Mpc)(240 Mpc) = 1.72107 m/s. The red shift of this would then be = (656.3nm) 1  (1.72107 m/s)2 /(3108 m/s)2 = 695 nm. 1  (1.72107 m/s)/(3108 m/s) 328
E5224 We can approximate the red shift as = 0 /(1  u/c), so u=c 1 The distance is d = v/H = (0.02)(3108 m/s)/(72 km/s Mpc) = 83 Mpc. E5225 The minimum energy required to produce the pairs is through the collision of two 140 MeV photons. This corresponds to a temperature of T = (140 MeV)/(8.62105 eV/K) = 1.621012 K. This temperature existed at a time t= (1.51010 s1/2 K)2 = 86 s. (1.621012 K)2 0 (590 nm) (602 nm)
=c 1
= 0.02c.
E5226 (a) 0.002 m. (b) f = (3108 m/s)/(0.002 m) = 1.51011 Hz. (c) E = (1240 eV nm)/(2106 nm) = 6.2104 eV. E5227 (a) Use Eq. 523: t= (1.51010 sK)2 = 91012 s. (5000 K)2
That's about 280,000 years. (b) kT = (8.62105 eV/K)(5000 K) = 0.43 eV. (c) The ratio is (109 )(0.43 eV) = 0.457. (940106 eV) P521 The total energy of the pion is 135 + 80 = 215 MeV. The gamma factor of relativity is = E/mc2 = (215 MeV)/(135 MeV) = 1.59, so the velocity parameter is = 1  1/ 2 = 0.777. The lifetime of the pion as measured in the laboratory is t = (8.41017 s)(1.59) = 1.341016 s, so the distance traveled is d = vt = (0.777)(3.00108 m/s)(1.341016 s) = 31 nm.
329
P522
(a) E = K + mc2 and pc = pc =
E 2  (mc2 )2 , so
(2200 MeV + 1777 MeV)2  (1777 MeV)2 = 3558 MeV.
That's the same as p= . (b) qvB = mv 2 /r, so p/qB = r. Then r= P523 (1.901018 kg m/s) = 9.9 m. (1.61019 C)(1.2 T) (3558106 eV) (1.61019 J/eV) = 1.901018 kg m/s (3108 m/s)
(a) Apply the results of Exercise 451: E= (1240 MeV fm) = (4.281010 MeV/K)T. (2898 m K)T
(b) T = 2(0.511 MeV)/(4.281010 MeV/K) = 2.39109 K. P524 (a) Since = 0 we have = 0 or z= Now invert, z(1  ) + 1  = 1  2, (z + 1)2 (1  )2 = 1  2 , (z 2 + 2z + 1)(1  2 + 2 ) = 1  2 , 2 2 (z + 2z + 2)  2(z 2 + 2z + 1) + (z 2 + 2z) = 0. Solve this quadratic for , and = (b) Using the result, = (c) The distance is d = v/H = (0.934)(3108 m/s)/(72 km/s Mpc) = 3893 Mpc. (4.43)2 + 2(4.43) = 0.934. (4.43)2 + 2(4.43) + 2 z2 z 2 + 2z . + 2z + 2 1  2 +  1 . 1 1  2  1, 1 1  2 , 1
330
P525
(a) Using Eq. 4819, E = kT ln
n1 . n2
Here n1 = 0.23 while n2 = 1  0.23, then E = (8.62105 eV/K)(2.7 K) ln(0.23/0.77) = 2.8104 eV. (b) Apply the results of Exercise 451: = P526 (1240 eV nm) = 4.4 mm. (2.8104 eV)
(a) Unlimited expansion means that v Hr, so we are interested in v = Hr. Then Hr H 2 r3 3H 2 /8G = 2GM/r, = 2G(4r3 /3), = .
(b) Evaluating, 3[72103 m/s (3.0841022 m)]2 (6.021023 /mol) = 5.9/m3 . (0.001 kg/mol) 8(6.671011 N m2 /kg2 ) P527 (a) The force on a particle in a spherical distribution of matter depends only on the matter contained in a sphere of radius smaller than the distance to the center of the spherical distribution. And then we can treat all that relevant matter as being concentrated at the center. If M is the total mass, then r3 M = M 3, R is the fraction of matter contained in the sphere of radius r < R. The force on a star of mass m a distance r from the center is F = GmM /r2 = GmM r/R3 . This force is the source of the centripetal force, so the velocity is v = ar = F r/m = r GM/R3 . The time required to make a revolution is then T = 2r = 2 v R3 /GM .
Note that this means that the system rotates as if it were a solid body! (b) If, instead, all of the mass were concentrated at the center, then the centripetal force would be F = GmM/r2 , so v= and the period would be T = 2r = 2 v r3 /GM . ar = F r/m = GM/r,
331
P528 We will need to integrate Eq. 456 from 0 to min , divide this by I(T ), and set it equal to z = 0.2109 . Unfortunately, we need to know T to perform the integration. Writing what we do know and then letting x = hc/kT , z = = =
m 2c2 h d 15c2 h3 , 5 k4 T 4 5 hc/kT  1 2 e 0 15c2 h3 2k 4 T 4 xm x3 dx , x 2 5 k 4 T 4 h3 c2 e 1 15 x3 dx . 4 xm ex  1
The result is a small number, so we expect that xm is fairly large. We can then ignore the 1 in the denominator and then write z 4 /15 = x3 ex dx
xm
which easily integrates to z 4 /15 xm 3 exm . The solution is x 30, so T = (2.2106 eV) = 8.5108 K. (8.62105 eV/K)(30)
332
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