Physics 217 Practice Final Exam: Solutions

Similar documents
General Physics II. number of field lines/area. for whole surface: for continuous surface is a whole surface

CHAPTER 7 Applications of Integration

Electric Potential. and Equipotentials

This immediately suggests an inverse-square law for a "piece" of current along the line.

School of Electrical and Computer Engineering, Cornell University. ECE 303: Electromagnetic Fields and Waves. Fall 2007

Physics 11b Lecture #11

Physics 604 Problem Set 1 Due Sept 16, 2010

Solutions to Midterm Physics 201

School of Electrical and Computer Engineering, Cornell University. ECE 303: Electromagnetic Fields and Waves. Fall 2007

CHAPTER (6) Biot-Savart law Ampere s Circuital Law Magnetic Field Density Magnetic Flux

DEPARTMENT OF CIVIL AND ENVIRONMENTAL ENGINEERING FLUID MECHANICS III Solutions to Problem Sheet 3

Chapter 28 Sources of Magnetic Field

Physics 218, Spring March 2004

Radial geodesics in Schwarzschild spacetime

Prerna Tower, Road No 2, Contractors Area, Bistupur, Jamshedpur , Tel (0657) ,

Lecture 11: Potential Gradient and Capacitor Review:

1 Using Integration to Find Arc Lengths and Surface Areas

ELECTRO - MAGNETIC INDUCTION

In electrostatics, the electric field E and its sources (charges) are related by Gauss s law: Surface

U>, and is negative. Electric Potential Energy

The Area of a Triangle

AVS fiziks. Institute for NET/JRF, GATE, IIT-JAM, JEST, TIFR and GRE in PHYSICAL SCIENCES

Chapter 25 Electric Potential

ELECTROSTATICS. 4πε0. E dr. The electric field is along the direction where the potential decreases at the maximum rate. 5. Electric Potential Energy:

Electric Field F E. q Q R Q. ˆ 4 r r - - Electric field intensity depends on the medium! origin

Class Summary. be functions and f( D) , we define the composition of f with g, denoted g f by

Collection of Formulas

(A) 6.32 (B) 9.49 (C) (D) (E) 18.97

SPA7010U/SPA7010P: THE GALAXY. Solutions for Coursework 1. Questions distributed on: 25 January 2018.

Fluids & Bernoulli s Equation. Group Problems 9

PX3008 Problem Sheet 1

Homework 3 MAE 118C Problems 2, 5, 7, 10, 14, 15, 18, 23, 30, 31 from Chapter 5, Lamarsh & Baratta. The flux for a point source is:

Illustrating the space-time coordinates of the events associated with the apparent and the actual position of a light source

Course Updates. Reminders: 1) Assignment #8 available. 2) Chapter 28 this week.

8.022 (E&M) Lecture 13. What we learned about magnetism so far

3.1 Magnetic Fields. Oersted and Ampere

Influence of the Magnetic Field in the Solar Interior on the Differential Rotation

Continuous Charge Distributions

Answers to test yourself questions

Mark Scheme (Results) January 2008

( ) ( ) ( ) ( ) ( ) # B x ( ˆ i ) ( ) # B y ( ˆ j ) ( ) # B y ("ˆ ( ) ( ) ( (( ) # ("ˆ ( ) ( ) ( ) # B ˆ z ( k )

Electricity & Magnetism Lecture 6: Electric Potential

10 Statistical Distributions Solutions

Winter 2004 OSU Sources of Magnetic Fields 1 Chapter 32

9.4 The response of equilibrium to temperature (continued)

Optimization. x = 22 corresponds to local maximum by second derivative test

CHAPTER 25 ELECTRIC POTENTIAL

Experiment 1 Electric field and electric potential

Section 35 SHM and Circular Motion

Physics 505 Fall 2005 Midterm Solutions. This midterm is a two hour open book, open notes exam. Do all three problems.

(conservation of momentum)

Physics 1502: Lecture 2 Today s Agenda

( ) D x ( s) if r s (3) ( ) (6) ( r) = d dr D x

Lecture 13 - Linking E, ϕ, and ρ

Today in Physics 122: getting V from E

MATH34032: Green s Functions, Integral Equations and the Calculus of Variations 1. 1 [(y ) 2 + yy + y 2 ] dx,

On the Eötvös effect

Chapter Seven Notes N P U1C7

Friedmannien equations

of Technology: MIT OpenCourseWare). (accessed MM DD, YYYY). License: Creative Commons Attribution- Noncommercial-Share Alike.

MAGNETIC EFFECT OF CURRENT & MAGNETISM

Applications of Definite Integral

Chapter Introduction to Partial Differential Equations

Applications of Definite Integral

Problems set # 3 Physics 169 February 24, 2015

TOPIC: Electrostatics and Magnetostatics (ENEL475) Q.1

Lecture 4. Electric Potential

10 m, so the distance from the Sun to the Moon during a solar eclipse is. The mass of the Sun, Earth, and Moon are = =

Welcome to Physics 272

Quality control. Final exam: 2012/1/12 (Thur), 9:00-12:00 Q1 Q2 Q3 Q4 Q5 YOUR NAME

(a) Counter-Clockwise (b) Clockwise ()N (c) No rotation (d) Not enough information

The Wave Equation I. MA 436 Kurt Bryan

Chapter 2: Electric Field

r a + r b a + ( r b + r c)

1 Introduction. K. Morawetz*, M. Gilbert and A. Trupp Induced Voltage in an Open Wire

ECE Microwave Engineering. Fall Prof. David R. Jackson Dept. of ECE. Notes 8. Waveguides Part 5: Coaxial Cable

Chapter 22 The Electric Field II: Continuous Charge Distributions

A NOTE ON THE POCHHAMMER FREQUENCY EQUATION

Topics for Review for Final Exam in Calculus 16A

Physics 122, Fall September 2012

The Double Integral. The Riemann sum of a function f (x; y) over this partition of [a; b] [c; d] is. f (r j ; t k ) x j y k

Mathematical Reflections, Issue 5, INEQUALITIES ON RATIOS OF RADII OF TANGENT CIRCLES. Y.N. Aliyev

EECE 260 Electrical Circuits Prof. Mark Fowler

1.2. Linear Variable Coefficient Equations. y + b "! = a y + b " Remark: The case b = 0 and a non-constant can be solved with the same idea as above.

CHAPTER 2 ELECTROSTATIC POTENTIAL

Properties and Formulas

CHAPTER 18: ELECTRIC CHARGE AND ELECTRIC FIELD

Two dimensional polar coordinate system in airy stress functions

Chapter 21: Electric Charge and Electric Field

Previously. Extensions to backstepping controller designs. Tracking using backstepping Suppose we consider the general system

MATHEMATICS IV 2 MARKS. 5 2 = e 3, 4

1. Viscosities: μ = ρν. 2. Newton s viscosity law: 3. Infinitesimal surface force df. 4. Moment about the point o, dm

16.1 Permanent magnets

( ) Make-up Tests. From Last Time. Electric Field Flux. o The Electric Field Flux through a bit of area is

University of Illinois at Chicago Department of Physics. Electricity & Magnetism Qualifying Examination

Week 8. Topic 2 Properties of Logarithms

r r E x w, y w, z w, (1) Where c is the speed of light in vacuum.

Module 4: Moral Hazard - Linear Contracts

STD: XI MATHEMATICS Total Marks: 90. I Choose the correct answer: ( 20 x 1 = 20 ) a) x = 1 b) x =2 c) x = 3 d) x = 0

Prof. Anchordoqui Problems set # 12 Physics 169 May 12, 2015

Transcription:

Physis 17 Ptie Finl Em: Solutions Fll This ws the Physis 17 finl em in Fll 199 Twenty-thee students took the em The vege soe ws 11 out of 15 (731%), nd the stndd devition 9 The high nd low soes wee 145 nd 75 If ny of these solutions seems obsue, plese ontt us so we n eplin it bette Poblem 1 (3 points) An infinite ylinde with dius R is hged unifomly, with hge density ρ, eept fo n infinite ylindil hole pllel to the ylinde's is The hole hs dius R nd is tngent to the eteio of the ylinde A shot hunk of the ylinde is shown in the ompnying figue E y Clulte the eleti field eveywhee inside the hole, nd sketh the lines of E on the figue ρ R Supepose now ylinde with hge density ρ on wide ylinde with hge density ρ to ete the hole; then supepose the fields fom these two hge distibutions The field inside unifomly hged infinite ylinde n be omputed by using Guss Lw, with ylindil Gussin sufe (dius s less thn the wie s dius, length ) oil with the wie: R y s s + E d = Qenlosed E πs = π ρπs E = πρs ( ) 4

Then, with E + s the field fom the wide ylinde nd now one, we hve (see figue): E s the field inside the E+ = πρs+, E = πρs, E= E + E = πρ s s = πρryˆ ( ) + + The field is onstnt, nd points stight up Multiply on the ight by 1ε to get the nswe in MKS units b An infinite ylindil wie with dius R ies unifom uent density J, eept inside n infinite ylindil hole pllel to the wie's is The hole hs dius R nd is tngent to the eteio of the wie A shot hunk of the wie is shown in the ompnying figue y B Clulte the mgneti field eveywhee inside the hole, nd sketh J the lines of B on the figue R Supepose now wie with uent density -J on wide ylinde with hge density J to ete the hole; then supepose the fields fom these two uent distibutions The field inside unifomdensity uent n be omputed by using Ampèe s Lw, with iul Ampèen loop (dius s less thn the wie s dius) oil with the wie: B d = Ienlosed πjs B πs= ( Jπs ) B = φˆ Then, with B + s the field fom the wide ylinde nd now one, we hve: B s the field inside the πjs+ πj πj B+ = φˆ+ = s+ ( sinφ+ ˆ + os φ+ yˆ) = ( y+ ˆ + + yˆ), π J B = ( y ˆ + yˆ ) But = = nd y = y + R= y (see oss setion figue in pt ), so + +

3 ( y ( y R) ) B πj ˆ ˆ ˆ ˆ πjr = B + + B = + + = ˆ y y The field is onstnt, nd points hoiontlly, to the left in the figue Reple the 1 with µ to get the nswe in MKS units An infinite ylindil flu tube with dius R ies unifom mgneti field B, pllel to the ylinde's is, eept inside n infinite ylindil hole pllel to the flu tube s is The hole hs dius R nd is tngent to the eteio of the flu tube A shot hunk of the flu tube is shown in the ompnying figue The mgneti field is eo inside the hole nd outside the flu tube, but whee it eists, it is inesing linely with time: B y E R t B( t) = B ˆ t Clulte the eleti field eveywhee inside the hole, nd sketh the lines of E on the figue Supepose now flu tube with mgneti field -B on wide flu tube with mgneti field B to ete the hole; then supepose the fields fom these two flu tubes The field inside unifom mgneti flu tube n be omputed by using Fdy s Lw, with iul Ampèen loop (dius s less thn the flu tube s dius) oil with the flu tube: 1 dφb E d = dt 1 db πsb Bs E πs= πs = E = φˆ dt t t Then, with E + s the field fom the wide flu tube nd now one, we hve: E s the field inside the Bs B E = φˆ = ˆ + yˆ, + + + t t ( y ) B E = ( ( y R) ˆ + yˆ ), t

4 so ( y ( y R) ) E B B ˆ ˆ ˆ ˆ R = E + + E = + + = ˆ t y y t The field is onstnt, nd points hoiontlly, to the ight in the figue Eliminte the fto of 1 to get the nswe in MKS units Poblem (3 points) Clulte the eleti field t point on the is of unifomly-hged iul disk, distne fom the ile's ente The disk hs sufe hge density σ nd dius de Fo two infinitesiml elements the sme distne wy fom the is (s) on opposite sides ( φ nd φ+ π ), the hoiontl omponents of de nel nd the vetil () omponents dd; thus the ontibution to the eleti field fom ing with dius s nd width ds is dq osθ π sds de= ˆ =σ + s + s θ s ds σ Thus + sds du E = ˆπσ = ˆπσ = ˆ πσ u ( + s ) 3 3 u 1 + = πσ 1 ˆ + b The hged iul disk fom pt is set into ottion bout its is, with ngul fequeny ω Clulte the mgneti field B t point on the is distne fom the ente of the disk Agin, the hoiontl omponents nel nd vetil omponents dd, fo uent elements symmetilly pled bout the is, so db ω θ σ

5 ( σω)( π sds) 1 Kd 1 s db = os θ = s + + s Thus πσω sds B= ˆ 3 3 ( + s ) Not mny points would be lost by stopping hee, but we ll ssume we e tying fo pefet soe: πσω udu B= ˆ 3 Integte by pts, with ( ) 3 ( + u) dv = du + u, v = + u : πσω πσω u du B= ˆ uv vdu = ˆ + + u + u + dw πσω + w w + + πσω + ˆ πσω = ˆ + = ˆ + πσω = ˆ + + = + + Multiply on the ight by 1ε in pt, nd eple the 1 with µ in pt b, to get the nswes in MKS units Poblem 3 ( points) Conside the efeene point fo eleti potentil to be t infinity fo both pts of this poblem A onduting sphee with dius is in n infinite vuum Wht is its pitne? Conside it to y hge q; then, fo >,

6 q E= ˆ, qd q CV V = E d = = = C = Multiply on the ight by 1ε fo the MKS nswe b The sme sphee is pled in n infinite, wekly-onduting medium with esistivity ρ Wht is the esistne between the sphee nd infinity? If the ondutivity is smll enough, the eleti field is given simply by the eletostti vlue, so Fo ll But V >, then, π π σ q J = σ E= ˆ 1 I = J d = σq dφ dθsinθ = σq ( π)( ) = 4 πσq = q still, so, sine V lso = IR, R V 1 ρ = = = I σ Divide on the ight by 1ε fo the MKS nswe Poblem 4 (1 points) Clulte the mgneti field inside long solenoid with dius, N tuns pe unit length, nd uent I Use Ampèe s Lw with etngul loop, two sides pllel to the solenoid s is: B d = Ienlosed Bh = INh B= NIˆ,

7 whee I is the uent in eh tun of the solenoid, nd the dietion is long the oil s is in the dietion given by the ight hnd ule Reple the 1 with µ to get the nswe in MKS units b Inside the long solenoid nd pllel to it, thee is shot solenoid with dius b, N b tuns pe unit length, nd length Wht is the mutul indutne of the two solenoids? b It s esiest to wok out the flu in the smll oil fom the field in the lge one: Φ = = Bb BA b NIN b π b (flu theds Nb b NN b = I = MI, so M = NN b b loops) Reple the 1 with µ to get the nswe in MKS units Poblem 5 ( points) An infinite, hged, stight wie (hge pe unit length λ ) lies pllel to the is, nd pllel to two infinite, gounded onduting plnes whih inteset t 9 ngle The hged wie lies distne fom eh plne Clulte the eleti field E t point A, fom eh plne on the sme side s the line hge, nd t point B, fom eh plne but on the side opposite the line hge y A λ 1 λ λ 4 B 3 λ

8 Point B is inside the onduto, so the eleti field is eo thee Fo point A, use the method of imges Thee e thee imges of the line hge in the onduting plne, two with hge pe unit length λ nd one with λ, lbeled -4 in the figue bove The eleti field fo n infinite line hge n be lulted fom Guss Lw, using Gussin ylinde with dius s nd length h: E d = qenlosed λ E πsh= πλh E= s ˆ 4 s So we n supepose the fields fom the fou line hges t point A: E= E + E + E + E 1 3 4 1 1 1 1 3 1 ˆ ˆ ˆ ˆ = λ + y + y 1 1 1 1 1 3 1 1 1 ˆ ˆ ˆ ˆ + y + + y 1 1 1 3 λ 1 3 1 1 1 1 3 1 ˆ = ˆ + + + y 1 1 1 1 1 1 11λ = ( ˆ + yˆ ) 3 Poblem 6 ( points) A sphee with dius R ies polition distne fom the ente P = K, whee K is onstnt nd is the veto Find the sufe nd volume bound hges σb = P( R) ˆ = KR, 1 d ρb = P = ( K ) = 3 K d Chek: the totl bound hge should ome out to eo, nd it does: 4 3 3 3 q = R σb + πr ρb = KR KR = 3 b Clulte the fields E nd D eveywhee

9 Sine the hges e distibuted with spheil symmety, we n use Guss Lw with spheil gussin sufes With one of those dwn outside the sphee > R, we enlose no hge (see pt, bove), so ( ) E d = E =, D = E + P = Fo the inside of the sphee ( R) popotionl to its volume:, Gussin sphee enloses hge E d = qenlosed 4 3 4 3 E = π ρb = π ( 3K) 3 3 E= K = 4 πp, D= E+ P= Note tht we ould hve done the whole poblem with D, beuse thee e no fee hges nd the polition is dil (ie P =, so D= ) Poblem 7 ( points) A iul wfe is mde of vey wekly onduting mteil with esistivity ρ nd dieleti onstnt ε Its dius is nd its thikness is ( ) Highly ondutive, metlli eletodes ove the iul fes Unde the ssumption tht the mteil s ondutivity doesn't ffet the pitne, lulte the esistne nd pitne of the wfe with its eletodes ρ, ε ρ ρ R = = A π εa ε C = = 4, Reple ε by ε to onvet to MKS b Suppose tht the wfe is hged up with bttey with voltge V, nd tht the bttey is disonneted t t = Wite one diffeentil eqution desibing the hge on the eletodes, nd the simil equtions desibing the potentil diffeene V ( t ), nd the eleti field E ( t) within the wfe

1 (Hint: The wfe's esistne nd pitne hve the sme potentil diffeene, nd n theefoe be epesented by two elements in pllel) Kihhoff s ule #, with the loop dwn ountelokwise, gives us Divide this esult though by C nd use q q + IR = ; C dq 1 dq + q = + q= dt RC dt ερ = CV to get dv + V = dt ερ + I dq = q dt + R C V The field is onstnt between the pltes; divide this lst esult by nd use V = E to get de + E = dt ερ Solve the diffeentil eqution to obtin the eleti field between the eletodes s funtion of time de de + E= dt ερ = E ερ E t ln = E ερ Et = Ee () t ερ d In tems of the esistivity nd dieleti onstnt of the mteil, wht is the time onstnt? Comment on the genelity of this esult, onsideing the dependene of the time onstnt on the shpe of the wfe The esult of pt n lso be witten s t τ ερ () = Ee, τ = Et Reple ε by ε to onvet to MKS Note tht the time onstnt doesn t hve ny ftos o vibles in it tht hve to do with the shpe of the wfe; this must dt

11 theefoe be genel esult fo the eltion of n eleti field in medium tht onduts