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Cornell - MATH - 2940
Concept Questions: 11-18-2011MA2940: Linear Algebra for Engineers1) (T/F) If = 0 is an eigenvalue of a square matrix A, then A cannot be a Markov matrix.2) (T/F) If = 0 is an eigenvalue of a square matrix A, then A cannot be a symmetricmatrix.3) (T/F
Cornell - PHYSICS - 2214
Physics 2214Fall 2011Lecture 1UOscillationsA mechanical oscillation is any repetitive motion.Examples of free oscillations i.e., those that occur spontaneously after an object is displaced:Mass on a Spring:Oscillating Beam:Pendulum:Torsion Oscil
Cornell - PHYSICS - 2214
Physics 2214Fall 2011Lecture 2Recap:Stable Equilibrium: For a stable equilibrium point at x = xeq, we need:! (!" ) = 0!"# !"!"!"<0For a system to exhibit oscillations after you displace it, it must have a stable equilibrium point.Simple Harmoni
Cornell - PHYSICS - 2214
Physics 22142010 Robert E. ThorneFall 2011Lecture 3Energy in damped oscillating systemsThe total energy is the sum of the kinetic and potential energies, E = K + U. In a dampedsystem, the energy decays away. In the underdamped case, K and U oscillat
Cornell - PHYSICS - 2214
Physics 22142010 Robert E. ThorneSpring 2010Lecture 4So far weve considered oscillating systems that consist of only one degree of freedom. In otherwords, to completely describe their motion we need only describe the motion of a single point,which r
Cornell - PHYSICS - 2214
Physics 22142010 Robert E. ThorneFall 2011Lecture 5Recap: Ideal Traveling WavesWaves keep their shape as they propagate through a mediumWaves move at a constant speed v that is determined by the medium.The speed v is the same for waves of all shape
Cornell - PHYSICS - 2214
Physics 22142010 Robert E. ThorneFall 2011Lecture 6RecapIdeal Traveling Waves:! ! , ! = ! ! !"! !! !! ! =!!"!"!Waves on a string:!(! , !) = transversedisplacementApply Newtons 2nd law:! = ! sin x + x, t sin x, tAssume slopes !" !" and an
Cornell - PHYSICS - 2214
Physics 22142010 Robert E. ThorneFall 2011Lecture 7RecapStanding Waves:- simple harmonic motion at each point- amplitude of SHM varies with position x, i.e. Am =- phase of SHM is the same for all x- due to interference of waves traveling in oppos
Cornell - PHYSICS - 2214
Physics 22142010 Robert E. ThorneFall 2011Lecture 8RecapSinusoidal drives are unique in the following sense. If we drive a linear system with a sinusoidal(harmonic) drive, the response at each point in the system will also be sinusoidal at the same
Cornell - PHYSICS - 2214
Physics 2214 2010 Robert E. ThorneSpring 2010Lecture 9Wave Interference and Beats"Interference" is a fancy sounding word, used in expressions like "laser interference" and"quantum interference." But what does it mean for two waves to interfere? It j
Cornell - PHYSICS - 2214
Physics 2214Robert E. Thorne 2010Spring 2010Lecture 13Recap: Energy and Power in WavesStrings:1 y 2 t Kinetic energy per unit length:uk =Elastic potential energy per unit length:1 y up = 2 x 22y yx tThese expressions are completely gen
Cornell - PHYSICS - 2214
Physics 2214Robert E. ThorneSpring 2010Lecture 14Recap: Maxwells equations in integral form: E d A = Bd A = 0Qencd E d = dt B BddE = ic + dt Maxwells Equations in Differential FormWe can rewrite Maxwells equations in differential form (i.e.
Cornell - PHYSICS - 2214
Physics 22142010 Robert E. ThorneSpring 2010Lecture 15Recap:Maxwells equations in integral and differential form:Qenc E d A = iE =0 Bd A = 0iB = 0dBdtd B d = I c + dt E E d= E = Bt B = jc + Etwhere =K0 and =Km0.Wave equations in
Cornell - PHYSICS - 2214
Physics 22142010Robert E. ThorneSpring 2010Lecture 18Total internal reflectionWhen a wave is incident from a high index (n1) material onto a low index (n2) material, therefracted wave bends away from the normal. If the incident angle is large enough
Cornell - PHYSICS - 2214
Physics 22142010 Robert E. ThorneSpring 2010Lecture 19EM Wave InterferenceTo interfere two waves, you simply add up their amplitudes at each point in space, and look atthe resulting pattern in space and time. We've already seen examples of wave inte
Cornell - PHYSICS - 2214
Physics 22142010 Robert E. ThorneSpring 2010Lecture 20Recap: InterferenceCoherent sources: have same frequency, wavelength and polarization. Coherence of sourcesensures that the electric fields produced by the sources at a given position P have a fi
Cornell - PHYSICS - 2214
Physics 22142010 Robert E. ThorneSpring 2010Lecture 21DiffractionDiffraction is just another kind of interference phenomenon. In this case, the interfering wavesare often produced by a single source. But now we partially block the path of the waves
Cornell - PHYSICS - 2214
Physics 22142010 Robert E. ThorneSpring 2010Lecture 22Why Quantum Mechanics?Observations/questions ca 1900 not explained by classical mechanics and EM wave theory:Accelerated charges emit radiation (as in an antenna). Charges undergoing circular mot
Cornell - PHYSICS - 2214
Physics 22142010 Robert E. ThorneSpring 2010Lecture 23RecapPhotoelectric effectV0 K max of the photoejected electrons.Observations:- Electrons are emitted when f > fth- The electrons are emitted instantly, with no time delay, as soon as the light
Cornell - PHYSICS - 2214
Physics 22142010 Robert E. ThorneSpring 2010Lecture 24RecapWaves: , f; Energy density; Intensityspread out in spaceshow interference and diffractiontransfer energy and momentum continuously to a particleParticles:Point likediscrete energy E, m
Cornell - PHYSICS - 2214
Survival of concept of Atom Democritus (460 370 BCE) Epicurus (341 270BCE) Titus Lucre&us Carus (99 -55 BCE) Poggio Bracciolini (1380-1459) Survival of concept of At
Cornell - PHYSICS - 2214
TA's Name:_ Section: _Your Name: _Physics 2214 Assignment 1Concepts:complex numberscomplex exponentialsoscillationsrestoring forcessimple harmonic motionforce law for SHMdamped oscillationsdriven oscillations and resonancedecay time and resona
Cornell - PHYSICS - 2214
TA's Name:_ Section: _Your Name: _Physics 214 Assignment 2Concepts:damped oscillationsdriven oscillatons and resonancedamping regimespower in driven oscillationsReading: Lecture Notes for lectures 2 and 3 (on BB); Y&F, Vol. 1, Chapter 13Assignmen
Cornell - PHYSICS - 2214
TA's Name:_ Section: _Your Name: _Physics 2214 Assignment 3Concepts:traveling wavesharmonic traveling waveswaves on a stringsound wavesReading: Y&F, Vol. 1, Chapters 15 and 16Assignment: Due at the beginning of section on Wed., Sept. 21 or Thurs.
Cornell - PHYSICS - 2214
TA's Name:_ Section: _Your Name: _Physics 2214 Assignment 4Concepts:Derivation of the wave equationW aves on stringsSound wavesStanding wavesStanding waves on stringsStanding sound waves in pipesReading: Y&F, Vol. 1, Chapter 16.Assignment: Due
Cornell - PHYSICS - 2214
TA's Name:_ Section: _Your Name: _Physics 2214 Assignment 5Concepts:Energy and Power in wavesReflection and Transmission of wavesElectromagnetic wavesReading: Y&F, Vol. 1, Chapters 15 & 16; Vol. 2, Chapter 21; Lecture notesAssignment: Due in secon
Cornell - PHYSICS - 2214
Physics 2214 Assignment 6Concepts:Electromagnetic WavesRelations between E, B and vReflection and transmission of EM wavesPlane WavesPolarizationReading: Y&F, Vol. 2, Chapter 32 and 33Assignment: Due in section, Wed. or Thurs. of the week of Octob
Cornell - PHYSICS - 2214
Physics 2214 Assignment 7Concepts:EM WavesPolarizationInterferencePower and MomentumLasersPoynting vectorReading: Y&F, Vol. 2, Chapters 32, 33, and 35Assignment: Due in W ednesday or Thursday section the week of Oct. 31.Physics Problems:1. EM W
Cornell - PHYSICS - 2214
Physics 2214 Assignment 8Concepts:Snell's lawConstructive and Destructive InterferencePhotoelectric EffectDiffractionOptical ResolutionReading: Y&F, Vol. 2, Chapters 33, 35, and 36, Vol. 3, Chapter 38Assignment: Due in second section meeting the w
Cornell - PHYSICS - 2214
Physics 2214 Assignment 9Concepts:Photoelectric Effect and PhotonsCompton scatteringDeBroglie wavelength of particlesElectron diffractionW ave functions and interpretationPlane wavesBeatsUncertainty PrincipleSchrdinger EquationReading: Y&F, Vol
Cornell - PHYSICS - 2214
Phys 2214 Homework #1 SolutionsSeptember 1, 20111. z (t) = rei(t+)(a) z (t) = rei(t+) = r[cos(t + ) + i sin(t + )]. Then x(t) =Re[z (t)] = r cos(t + ) and y (t) = Im[z (t)] = r sin(t + ) .(b) Suppose = 0 + i1 . Thenz (t) = rei(t+) = rei(0 +i1 t+) =
Cornell - PHYSICS - 2214
Phys 2214 Homework #2 SolutionsSeptember 9, 20111. Free oscillations(a) For the initial conditions x(0) = A and v (0) = 0, we have thefollowing results:i. Underdamped: x(t) = Aet/A cos(0 t)ii. Overdamped: x(t) = Aet/Aiii. Critically damped: x(t) =
Cornell - PHYSICS - 2214
Phys 2214 Homework #3 SolutionsSeptember 15, 20111. The disturbance travels down the rubber tube with the wave speed,which, for a one-dimensional transverse wave with constant tensionand mass/length, is given byv=.The tension is equal to the weight
Cornell - PHYSICS - 2214
Phys 2214 Homework #4 SolutionsSeptember 30, 20111. For a long, thin rod, the compressions created by a longitudinal wavetraveling along the rod will change the length to a greater extent thanthe diameter. So, we can replace the equation for the bulk
Cornell - PHYSICS - 2214
Phys 2214Assignment #5 Solutions1. Optical standing waves in a laser(a) standing wave frequencies: 1 2 L, so f n n f1 n (b) (i) n nmax nmin [ f 0 f ( f 0 f )] (ii) For n = 1, L c1nc, n = 1,2,3, 2L4L f and n = 6cc 0.075m 7.5cm4 f3. Superpo
Cornell - PHYSICS - 2214
Phys 2214 Homework #6 SolutionsOctober 26, 20111. EM Waves in VacuumGiven Gauss law, E = / 0 , assume = 0, since were in a vacuum.Also, we take the plane wave to be traveling in the +x direction, soE = f (x ct) + g (x ct) + h(x ct) .xyzNote that
Cornell - PHYSICS - 2214
Phys 2214 Homework #7 SolutionsNovember 1, 20111. EM Waves in Conductors.The current density is J = E/, where is the electrical resistivity.Amperes law in dierential form isB =EE+.tIf is small (a good conductor), then the rst term on the right h
Cornell - PHYSICS - 2214
PHYS 2214 Homework #8 Solutions1. Deriving Snells Law.(a) From the gure in the book,d1 d2t = t1 + t2 =+=v1 v2h2 + x21+v1h2 + (l x)22v2.(b) The independent variable here is x, since the others are just parameters. So, we nd the minimum time
Conestoga - EE - 1244
Welcome to 2G03:Problem Solving &Technical CommunicationDr. E. Cranston and Mr. V. Leung2G03 Lecture 1: Introduction (1)Welcome Instructors: Emily Cranston and Vince Leung TAs: Kevin Kan and Sarah Charlong Avenue to Learn Courseware: 2011 updated
Conestoga - EE - 1244
The Writing Process2G03: Problem Solving &Technical CommunicationDr. E. Cranston and Mr. V. Leung2G03 Lecture 2: The Writing Process (1)Presentations: ChE Professors Prof. M. Thompson(Polymers) Prof. C. Filipe(Bioengineering) Prof. T. Adams(Pro
Conestoga - EE - 1244
The Writing Process (Continued)2G03: Problem Solving &Technical CommunicationDr. E. Cranston and Mr. V. Leung2G03 Lecture 3: The Writing Process Continued (1)Housekeeping Emily Cranston: ecranst@mcmaster.ca Vince Leung: leungv@mcmaster.ca Hand in
Conestoga - EE - 1244
The Job Search2G03: Problem Solving &Technical CommunicationDr. E. Cranston and Mr. V. Leung2G03 Lecture 4: The Job Search and Formatting (1)Housekeeping Emily Cranston: ecranst@mcmaster.ca Vince Leung: leungv@mcmaster.ca Hand in assignments in cl
Conestoga - EE - 1244
Boss-Quality Documents,Audience Analysisand Interview SkillsDr. E. Cranston and Mr. V. Leung2G03 Lecture 5: Boss-Quality, Audience Analysis, Interview Skills (1)Housekeeping Emily Cranston: ecranst@mcmaster.ca OFFICE HOURS: Wednesday 1 pm to 3 pm
Conestoga - EE - 1244
Ethics, Paraphrasing and WhatIndustry Expects of YouDr. E. Cranston and Mr. V. Leung2G03 Lecture 6: Ethics, Paraphrasing and What Industry Expects of You (1)Housekeeping Emily Cranston: ecranst@mcmaster.ca OFFICE HOURS: not this week but otherwise
Conestoga - EE - 1244
Awareness inProblem SolvingDr. E. Cranston and Mr. V. Leung2G03 Lecture 7: Awareness in Problem Solving (1)Housekeeping Emily Cranston: ecranst@mcmaster.ca OFFICE HOURS: Wednesdays 1 pm to 3 pm (JHE A412) Vince Leung: leungv@mcmaster.ca Due today
Conestoga - EE - 1244
Problem Solving Strategyand Self-AssessmentDr. E. Cranston and Mr. V. Leung2G03 Lecture 8: Strategy and Self-Assessment (1)Housekeeping Emily Cranston: ecranst@mcmaster.ca OFFICE HOURS: Wednesdays 1 pm to 3 pm (JHE A412) Vince Leung: leungv@mcmast
Conestoga - EE - 1244
Oral Presentation Skills andthe Unique YouMs. S. Charlong, Dr. E. Cranston,and Mr. V. Leung2G03 Lecture 9: Oral Presentations and the Unique You (1)Housekeeping Emily Cranston: ecranst@mcmaster.ca OFFICE HOURS: Wednesdays 1 pm to 3 pm (JHE A412)
Conestoga - EE - 1244
Time and StressManagementDr. E. Cranston and Mr. V. Leung2G03 Lecture 10: Time and Stress Management (1)Housekeeping Emily Cranston: ecranst@mcmaster.ca OFFICE HOURS: Wednesdays 1 pm to 3 pm (JHE A412) Vince Leung: leungv@mcmaster.ca Due today: N
Conestoga - EE - 1244
Analysis and ClassificationDr. E. Cranston and Mr. V. Leung2G03 Lecture 11: Analysis and Classification (1)Housekeeping Emily Cranston: ecranst@mcmaster.ca OFFICE HOURS: Wednesdays 1 pm to 3 pm (JHE A412) Vince Leung: leungv@mcmaster.ca Due today:
Conestoga - EE - 1244
CreativityDr. E. Cranstonand Mr. V. Leung2G03 Lecture 12: Creativity (1)Housekeeping Emily Cranston: ecranst@mcmaster.ca OFFICE HOURS: Dec 7th only: 1 pm to 3 pm (JHE A412) Vince Leung: leungv@mcmaster.ca Due today:Corrected term paper (with abs
Conestoga - EE - 1244
CORRELATIONData arise in pairs(xi, yi),i = 1 , 2, . . . , nResponse y : outcome of experimentExplanatory x: explains outcomeScatterplotPlot observed pairs (xi, yi) in x-y plane1Example: Cancer Mortality in Oregonvs Radioactive ContaminationCoun
Conestoga - EE - 1244
Meaning of r2 - Worked ExampleExamplex = explanatory variable= temperature (degrees Celsius)y = response variable= yield (kg)x181920212223242526272829y76.177.978.178.278.879.779.981.181.281.882.883.51First check that a reg
Conestoga - EE - 1244
PROBABILITYChapter 2.1Deterministic: dx = bx.dtStatistical:observation = true value + error error dierent each time experimentis performed.1Example. Quality control. Sample n,X = proportion defective, p = true defective rate.X = p + errorIn pr
Conestoga - EE - 1244
Conditional ProbabilityProbabilities do not live in a vacuum.They are specied by conditions whichmay change or about which additionalinformation may become available. Consider A, B with P (A), P (B ) given. Suppose have knowledge that B occurred.How
Conestoga - EE - 1244
RANDOM VARIABLESMeasurements and observations are calledrandom variables. Each results from anoutcome of an experiment, so:Denition: Random variable X is realfunction on sample space S.Start with discrete r.v. RX is nite orcountable.1For any real
Conestoga - EE - 1244
Binomial DistributionAssumptions n independent trials trial i has dichotomous outcome (0 or 1, no or yes, failure or success, etc.) denotedby Xi. Called Bernoulli trials. probability of success on anytrial is the same p.1Let Y = # of successes.Y
Conestoga - EE - 1244
Example:- 19 19 square Go board (Japanese boardgame)- throw dart repeatedly and at random- mark square hit111. P (specic square hit) = 19 1= 1193612. How many throws, until highprobability of hitting some squareagain?3. After N throws, what
Conestoga - EE - 1244
Poisson DistributionFlaws occur at random alonglength of oil pipeline. Average per unit length. Y = number ofaws in a randomly selected section of pipeline of length 1. Canwe determine the distribution ofY?Generic situation is incidentshappening o