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Course: MATH Cal I- Cal, Spring 2008
School: TN Tech
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Calculus Stewart ET 5e 0534393217;16. Vector Calculus; 16.9 The Divergence Theorem 1. The vectors that end near P are longer than the vectors that start near P , so the net flow is inward 1 1 near P and divF(P ) is negative. The vectors that end near P are shorter than the vectors that start 1 2 1 2 near P , so the net flow is outward near P and divF(P ) is positive. 2 2 2. (a) The vectors that end near P are...

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Calculus Stewart ET 5e 0534393217;16. Vector Calculus; 16.9 The Divergence Theorem 1. The vectors that end near P are longer than the vectors that start near P , so the net flow is inward 1 1 near P and divF(P ) is negative. The vectors that end near P are shorter than the vectors that start 1 2 1 2 near P , so the net flow is outward near P and divF(P ) is positive. 2 2 2. (a) The vectors that end near P are shorter than the vectors that start near P , so the net flow is 1 1 outward and P is a source. The vectors that end near P are longer than the vectors that start near P , 1 2 2 so the net flow is inward and P is a sink. 2 (b) F(x, y)= x, y 1 2 divF= 2 F=1+2y . The y value at P is positive, so divF=1+2y is positive, 1 2 thus P is a source. At P , y< 1 , so divF=1+2y is negative, and P is a sink. 1 1 1 3. divF=3+x+2x=3+3x , so E div FdV = 0 0 0 (3x+3)dxdydz= 9 (notice the triple integral is three 2 times the volume of the cube plus three times x ). To compute S F dS on S : n=i, F=3 i+y j+2z k, and 1 S 1 F dS= S 1 3dS=3; S : F=3x i+x j+2xz k, n= j and 2 S 2 F dS= S 2 xdS= 1 ; 2 S : F=3x i+xy j+2x k, n=k and 3 S 3 F dS= S 3 2xdS=1; S : F=0, 4 S 4 F dS=0; S : F=3x i+2x k, n= j and 5 S 5 F dS= S 5 0dS=0; 9 . 2 S : F=3x i+xy j, n= k and 6 S 6 F dS= S 6 0dS=0. Thus S F dS= 4. divF=2x+x+1=3x+1 so 1 Stewart Calculus ET 5e 0534393217;16. Vector Calculus; 16.9 The Divergence Theorem 2 2 4 r 0 2 2 div FdV = E E 22 (3x+1)dV = 0 0 (3rcos +1)rdzdr d = 0 0 2 0 r(3rcos +1)(4 r )d dr 2 =2 =0 2 = r(4 r ) 3rsin + 2 dr 1 4 r 4 2 0 =2 0 (4r r )dr=2 3 2r =2 (8 4)=8 On S : The surface is z=4 x y ,x +y 1 2 2 2 2 4 , with upward orientation, and F=x i+xy j+(4 x y ) k. 2 2 2 Then F dS = S 1 [ (x )( 2x) (xy)( 2y)+(4 x y )]dA D 2 2 2 2 2 2 2 2 2 2 2 = D 2 2x(x +y )+4 (x +y ) dA= 0 0 (2rcos 2 0 r +4 r )rdr d = 0 2 5 2 1 4 r cos +2r r 5 4 64 sin +4 5 2 0 r=2 r=0 d = 64 cos +4 d 5 = =8 2 On S : The surface is z=0 with downward orientation, so F=x i+xy j, n= k and 2 F ndS= S 2 0dS=0. S 2 Thus 2 Stewart Calculus ET 5e 0534393217;16. Vector Calculus; 16.9 The Divergence Theorem F dS= S S 1 F dS+ S 2 F dS=8 . 5. div F=x+y+z , so 2 1 1 2 1 div FdV = E 0 0 0 2 (rcos +rsin +z)rdzdr d = 0 0 r cos +r sin + 2 2 1 r dr d 2 = 0 1 1 1 1 cos + sin + 3 3 4 2 d = 1 (2 )= 4 2 3 1 2 1 Let S be the top of the cylinder, S the bottom, and S the vertical edge. On S , z=1 , n=k , and F=xyi+y j+x k, so S 1 F dS= S 1 F ndS= S 1 xdS= 0 0 (rcos )rdr d = sin 2 0 1 3 r 3 1 0 =0 . On S , 2 z=0, n= k, and F=xyi so S 2 F dS= S z 2 0dS=0. S is given by r( , z)=cos i+sin 3 j+z k , 0 2 , 0 F dS = z 1. Then r 2 1 r =cos i+sin (cos 2 j and 2 F (r D 2 2 r )dA= z 0 0 sin +zsin )dzd 1 sin 2 2 2 0 S 3 = 0 cos 1 2 sin + sin 2 2 = 2 . d = 1 1 3 cos + 3 4 = 2 Thus S F dS=0+0+ 6. div F=1+1+1=3, so E div FdV = E 3dV =3 (volume of ball) =3 4 3 =4 . To find S F dS we use spherical coordinates. S is the unit sphere, represented by r( , )=sin cos i+sin sin j+cos k , 0 ,0 2 . Then r r =sin 2 cos i+sin 2 sin 2 j+sin cos k (see Example 17.6.10 [ET 16.6.10]) and k. Thus F(r( , ))=sin F dS = S D cos i+sin r )dA= sin j+cos 3 F (r (sin 0 0 cos 2 +sin 3 sin 2 +sin cos 2 )d d 3 Stewart Calculus ET 5e 0534393217;16. Vector Calculus; 16.9 The Divergence Theorem 2 = 0 d 0 x sin d =(2 )(2)=4 7. div F= Theorem, x (e sin y)+ y (e cos y)+ 1 1 2 x z (yz )=e sin y e sin y+2yz=2yz , so by the Divergence 1 0 1 0 1 0 2 x x F dS = S E div FdV = 1 0 2yzdzdydx=2 dx ydy zdz 1 2 z 2 2 0 = 2 x 1 y 2 0 0 0 2 1 0 3 =2 4 3 3 3 3 8. div F= F dS = S x (x z )+ 2 3 y (2xyz )+ 1 2 3 z 3 (xz )=2xz +2xz +4xz =8xz , so by the Divergence Theorem, 1 1 2 2 3 3 3 div FdV = E 8xz dzdydx=8 xdx dy z dz 1 2 3 = 8 2 1 2 x 2 2 1 1 y 2 2 1 4 z 4 3 3 =0 9. div F=3y +0+3z , so using cylindrical coordinates with y=rcos F dS = S E 2 , z=rsin , x=x we have (3y +3z )dV = 1 0 2 2 2 1 2 (3r cos 0 0 1 2 2 +3r sin 9 2 2 2 )rdxdr d = 3 d 0 r dr dx=3(2 ) 1 3 2 1 4 (3)= 10. div F=3x y 2x y x y=0, so S 2 2 2 F dS= E 0dV =0. 11. div F=ysin z+0 ysin z=0, so by the Divergence Theorem, S F dS= E 0dV =0. 12. divF=2xy+2xy+2xy=6xy, so F dS = S E 6xydV 4 Stewart Calculus ET 5e 0534393217;16. Vector Calculus; 16.9 The Divergence Theorem 1 2 2y 2 x 2y 1 2 2y = 0 0 1 2 2y 0 6xydzdxdy= 0 2 2 0 6xy(2 x 2y)dxdy 1 0 = 0 1 0 0 (12xy 2 6x y 12xy )dxdy= 3 6x y 2x y 6x y 1 0 2 3 2 2 x=2 2y x=0 dy = y(2 2y) dy= 2 2 2 8 5 4 3 2 y +6y 8y +4y 5 = 2 5 13. div F=y +0+x =x +y so F dS = S 2 E 2 0 3 2 (x +y )dV = 0 0 r 3 5 2 2 2 2 4 2 r rdzdr d = 0 0 4 2 2 2 r (4 r )dr d 32 3 3 2 = d 0 (4r r )dr=2 r 1 6 r 6 2 0 = 14. div F=4x +4xy so F dS = S 2 E 1 4x(x +y )dV = 0 0 0 2 2 2 1 rcos +2 (4r cos )rdzdr d 2 0 3 = 0 0 (4r cos 2 2 5 2 +8r cos )dr d = 3 4 2 8 2 cos + cos 3 5 d = 2 3 15. div F=12x z+12y z+12z so F dS = S E 2 12z(x +y +z )dV = sin 0 2 2 2 2 R 12( cos 0 0 0 R 5 0 )( ) sin 1 2 sin 2 2 2 d d d 1 6 6 R 0 =12 d 0 cos d d =12(2 ) 0 =0 16. F dS = S E /2 3(x +y +1)dV = 0 0 1 2 2 2 /2 2 3( sin d =2 2 2 +1) 93 5 2 sin d d d 1 3 + cos 3 /2 =2 0 93 3 sin +7sin 5 cos 7cos 0 = 194 5 5 Stewart Calculus ET 5e 0534393217;16. Vector Calculus; 16.9 The Divergence Theorem 17. S F dS= E 3 x dV = 1 1 0 2 1 1 2 x 4 y 4 3 x dzdydx= 2 341 60 2+ 81 sin 20 1 3 3 18. By the Divergence Theorem, the flux of F across the surface of the cube is /2 /2 /2 F dS= S 0 0 0 cos xcos y+3sin ycos ycos z+5sin zcos zcos x dzdydx= 2 2 2 2 2 4 4 6 19 64 2 . 19. For S we have n= k , so F n=F ( k)= x z y = y (since z=0 on S ). So if D is the unit disk, 1 1 we get S 1 F dS= S 1 F ndS= D ( y )dA= 0 0 2 2 1 r (sin 2 2 2 )rdr d = 1 4 . Now since S is closed, we can 2 use the Divergence Theorem. Since divF= use spherical coordinates to get S 2 x E (z x)+ y 2 0 1 3 2 2 2 2 2 y +tan z + (x z+y )=z +y +x , we 3 z /2 1 0 0 2 2 F dS= 1 4 div FdV = 13 . 20 sin d d d = 2 . Finally 5 F dS= S S 2 F dS S 1 F dS= 2 5 = 20. As in the hint to Exercise 19, we create a closed surface S =S S , where S is the part of the 2 1 paraboloid x +y +z=2 that lies above the plane z=1 , and S is the disk x +y =1 on the plane z=1 1 2 2 2 2 oriented downward, and we then apply the Divergence Theorem. Since the disk S is oriented 1 downward, its unit normal vector is n= k and F ( k)= z= 1 on S . So 1 F dS= S 1 F ndS= S 1 ( 1)dS= A(S )= S 1 1 . Let E be the region bounded by S . Then 2 6 Stewart Calculus ET 5e 0534393217;16. Vector Calculus; 16.9 The Divergence Theorem 12 2 r S 2 12 0 0 F dS = 2 div FdV = E E 1dV = 0 0 1 rdzd dr= (r r )d dr 3 =(2 ) 1 = 4 2 F dS= S S 2 Thus the flux of F across S is F dS S 1 F dS= 2 ( )= 3 . 2 2 2 21. Since for x | x| 3 = x i+y j+z k (x +y +z ) y 2 2 2 3/2 and x x 2 y x | x| (x +y +z ) 2 3 2 2 2 3/2 2 2 and (x +y +z ) z (x +y +z ) 2 2 3/2 2 2 2 2 3/2 = (x +y +z ) 3x (x +y +z ) 2 2 2 5/2 2 2 with similar expressions z 2 2 , we have div = 3(x +y +z ) 3(x +y +z ) (x +y +z ) 2 2 2 5/2 =0 , except at (0, 0, 0) where it is undefined. 22. We first need to find F so that S F ndS= S (2x+2y+z )dS, so F n=2x+2y+z . 2 2 But for S, n= 2 x i+y j+z k x +y +z 2 2 2 =x i+y j+z k. Thus F=2 i+2 j+z k and divF=1. If 2 B={(x, y, z)| x +y +z 2 2 1}, then S (2x+2y+z )dS= B dV =V (B)= 4 3 4 (1) = . 3 3 23. S a ndS= E div adV =0 since div a=0. 24. 1 3 F dS= S 1 3 div FdV = E 1 3 3dV =V (E) E 25. S curl F dS= E div(curl F)dV =0 by Theorem 17.5.11 [ET 16.5.11]. 26. 7 Stewart Calculus ET 5e 0534393217;16. Vector Calculus; 16.9 The Divergence Theorem D f dS= S n S ( f n)dS= E div( f )dV = E 2 f dV 27. S (f g) ndS= E div( f g)dV = E (f 2 g+ g f )dV by Exercise 17.5.25 [ET 16.5.25]. 28. S (f g g g f= f f ) ndS= E (f (f S 2 g+ g g g f ) (g f ) ndS= 2 f+ g (f E 2 f ) dV [by Exercise 27]. g g 2 But g, so that f )dV. 29. If c=c i+c j+c k is an arbitrary constant vector, we define F= f c= fc i+ fc j+ fc k . Then 1 2 3 1 2 3 divF=div f c= F ndS= S f f f c+ c+ c= x 1 y 2 z 3 f c and the Divergence Theorem says S F dS= E div FdV f cdV. In particular, if c=i then E S f i ndS= E f idV fn dS= S 2 E fn dS= S 1 E f dV (where n=n i+n j+n k ). Similarly, if c= j we have 1 2 3 x fn dS= S 3 E f dV, y and c=k gives f ndS = S S f dV. Then z fn dS S 2 fn dS 1 i+ i+ j+ S fn dS 3 k f dV z k = E f dV x E f dV y j+ E = E f f f i+ j+ k dV = x y z f dV E as desired. 30. By Exercise 29, S pndS= E pdV, so 8 Stewart Calculus ET 5e 0534393217;16. Vector Calculus; 16.9 The Divergence Theorem F= S pndS= E pdV = E ( gz)dV = E ( g k)dV = g E dV k= gV (E) k density g= gV (E), thus F= W k as desired. But the weight of the displaced liquid is volume 9
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18.1. Solve: We can use the ideal-gas law in the form pV = NkBT to determine the Loschmidt number (N/V):1.013 10 5 Pa N p = 2.69 10 25 m -3 = = V kB T (1.38 10 -23 J K )(273 K )()18.2. Solve: Nitrogen is a diatomic molecule, so r 1.0 10-1
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21.1. Model: The principle of superposition comes into play whenever the waves overlap.Visualize:The graph at t = 1 s differs from the graph at t = 0 s in that the left wave has moved to the right by 1 m and the right wave has moved to the left by
Stevens - PEP - 111
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23.1. Model: Light rays travel in straight lines.Solve: (a) The time ist=x 1.0 m = = 3.33 10 -9 s = 3.33 ns c 3 10 8 m / s(b) The refractive indices for water, glass, and zircon are 1.33, 1.50, and 1.96, respectively. In a time of 3.33 ns, l
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Stevens - PEP - 111
2.1.Solve:Model: The car is represented by the particle model as a dot. (a) Time t (s) Position x (m) 0 1200 1 975 2 825 3 750 4 700 5 650 6 600 7 500 8 300 9 0(b)2.2. Solve:Diagram (a) (b) (c)Position Negative Negative PositiveVelocity
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6.1. Model: We will assume motion under constant-acceleration kinematics in a plane.Visualize:Instead of working with the components of position, velocity, and acceleration in the x and y directions, we will use the kinematic equations in vector f
Stevens - PEP - 111
7.1. Solve: (a) From t = 0 s to t = 1 s the particle rotates clockwise from the angular position +4 rad to -2 rad. Therefore, = -2 - ( +4 ) = -6 rad in one sec, or = -6 rad s . From t = 1 s to t = 2 s, = 0 rad/s. From t = 2 s to t = 4 s the partic
Stevens - PEP - 111
8.1. Visualize:Solve: Figure (i) shows a weightlifter (WL) holding a heavy barbell (BB) across his shoulders. He is standing on a rough surface (S) that is a part of the earth (E). We distinguish between the surface (S), which exerts a contact forc
Stevens - PEP - 111
Solve: (a) The momentum p = mv = (1500 kg)(10 m /s) = 1.5 10 4 kg m /s . (b) The momentum p = mv = (0.2 kg)( 40 m /s) = 8.0 kg m /s .9.1. Model: Model the car and the baseball as particles.9.2. Model: Model the bicycle and its rider as a particl
Stevens - PEP - 111
10.1. Model: We will use the particle model for the bullet (B) and the bowling ball (BB).Visualize:Solve:For the bullet,KB =For the bowling ball,1 1 2 mB vB = (0.01 kg)(500 m /s) 2 = 1250 J 2 2 1 1 2 mBB vBB = (10 kg)(10 m / s) 2 = 500 J 2
Stevens - PEP - 111
11.1. Visualize:r Please refer to Figure Ex11.1. rSolve: (b) (c)(a) A B = AB cos = ( 4)(5)cos 40 = 15.3. r r C D = CD cos = (2)( 4)cos120 = -4.0. r r E F = EF cos = (3)( 4)cos 90 = 0.11.2. Visualize:r Please refer to Figure Ex11.2. rSolve
Stevens - PEP - 111
12.1.Solve: (b)Model: Model the sun (s), the earth (e), and the moon (m) as spherical. (a)Fs on e =Gms me (6.67 10 -11 N m 2 / kg 2 )(1.99 10 30 kg)(5.98 10 24 kg) = 3.53 10 22 N = (1.50 1011 m ) 2 rs2 e -Fm on e =GMm Me (6.67 10 -1
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13.1. Model: The crankshaft is a rotating rigid body.Solve: The crankshaft at t = 0 s has an angular velocity of 250 rad/s. It gradually slows down to 50 rad/s in 2 s, maintains a constant angular velocity for 2 s until t = 4 s, and then speeds up
FSU - CLA - 2123
Classics 2123: The Roman Way Lecture 3. The Early History of Rome and Roman Republican Government Readings: BHR 15-41; Shelton 2-4, 7-8, 251-3, 255-259, 262, 264-5Spring 2008Early History of Rome Regal period: dimly known, mostly through legends;
FSU - CLA - 2123
Classics 2123: The Roman Way Lecture 4. Roman Family LifeSpring 2008Readings: BHR 129-31; Shelton nos. 15, 17-23, 25-27, 30-37, 44-45, 50, 54-56, 59-61, 63-67, 72, 75, 119-120, 124-5I. Definition of the family - familia - power of the father (p
FSU - CLA - 2123
Classics 2123: The Roman Way Lecture 4. Roman Family LifeSpring 2008Readings: BHR 129-31; Shelton nos. 15, 17-23, 25-27, 30-37, 44-45, 50, 54-56, 59-61, 63-67, 72, 75, 119-120, 124-5I. Definition of the family - familia - power of the father (p
FSU - CLA - 2123
Classics 2123: The Roman Way Lecture 6. Internal Disorders; Roman Slavery Readings: BHR 82-92; Shelton 207-209, 219, 227-229, 317-318Spring 2008I. Establishment of Roman provincial government Provincia: sphere of action of a magistrate with imper
UMiami - ACC - 212
Chapter 10Standard CostingAccounting 21210 - 1Learning Objective 1 Describe standard costing and indicate why standard costing is important.Accounting 212 10 - 2Why is Standard Costing Used?A standard is a preestablished benchmark for des
FSU - CLA - 2123
Classics 2123: The Roman Way Outline for Lecture 7. Roman Religion Readings: BHR 41-44; Shelton nos. 402-419, 423-428Spring 2008Problems Studying Ancient Religious Systems - time and culture (modern politics separated from religion) - vocabulary