Physics 505 Fall 2007 Homework Assignment #5 Solutions. Textbook problems: Ch. 3: 3.13, 3.17, 3.26, 3.27

Size: px
Start display at page:

Download "Physics 505 Fall 2007 Homework Assignment #5 Solutions. Textbook problems: Ch. 3: 3.13, 3.17, 3.26, 3.27"

Transcription

1 Physics 55 Fa 7 Homework Assignment #5 Soutions Textook proems: Ch. 3: 3.3, 3.7, 3.6, Sove for the potentia in Proem 3., using the appropriate Green function otained in the text, and verify that the answer otained in this way agrees with the direct soution from the differentia equation. Reca that Proem 3. asks for the potentia etween two concentric spheres of radii a and with > a, where the upper hemisphere of the inner sphere and the ower hemisphere of the outer sphere are maintained at potentia V, and where the other hemispheres are at zero potentia. Since this proem invoves the potentia etween two spheres, we use the Dirichet Green s function G x, x = +,m a + r< a+ r + < r> + r > + Y m ΩY m Ω Because there are no charges etween the spheres, the Green s function soution for the potentia ony invoves the surface integra Φ x = S Φ x G n da Here, we note a sutety in that the oundary surface is actuay disconnected, and incudes oth the inner sphere of radius a and the outer sphere of radius. This means that the potentia may e written as a sum of two contriutions Φ x = r =a Φ x G n a dω r = We now compute the norma derivatives of the Green s function and G r n = G r< =a r = =r =a = a a,m a + r + a Φ x G n dω + r Y m ΩY m Ω G r n = G r> = r = =r = = r a a +,m a + Y m ΩY m Ω r

2 Inserting these expressions into yieds Φ x =,m +,m V a Ω Y m Ω dω V Ω Y m Ω dω a a + a + r + r r a a + + r a Y m Ω Y m Ω This is the genera expression for the soution to the oundary vaue proem where V a Ω is the potentia on the inner sphere and V Ω is the potentia on the outer sphere. For the upper/ower hemispheres proem, we note that azimutha symmetry aows us to restrict the m vaues to m = ony. In this case, the spherica harmonic expansion reduces to a Legendre poynomia expansion Φ x = + V a ζp ζdζ V ζp ζdζ + a + a + r + r a + r a a + r a P cos θ + P cos θ where ζ = cos θ. Since V a = V for ζ > and V = V for ζ <, this aove expression reduces to Φ x = + V N a + a + r a + r + + V N r a a a + r = + V N a + a + r a + r r a + P cos θ + P cos θ a r + P cos θ where N = { = P ζdζ = j+ Γj πj! = j odd

3 If desired, the potentia may e rearranged to read Φ x = + V N a a a + r a + r = V + V j+ 4j Γj a j a j j= 4 πj! a 4j + r P cos θ a j r j + P j cos θ which agrees with the soution to Proem 3. that we have found earier. 3.7 The Dirichet Green function for the unounded space etween the panes at z = and z = L aows discussion of a point charge or a distriution of charge etween parae conducting panes hed at zero potentia. a Using cyindrica coordinates show that one form of the Green function is G x, x = 4 L n= m= e imφ φ sin nπz sin L nπz L nπ nπ I m L ρ < K m L ρ > In cyindrica coordinates, the poar direction φ is periodic with period π. This suggests that the Green s function coud e expanded as a Fourier series in e imφ. Simiary, the oundary conditions G = at z = and z = L motivates the use of a Fourier sine series sinnπz/l in the z coordinate. More precisey, a compete Fourier expansion in φ and z woud give G x, x = gρ, ρ e imφ e im φ nπz n πz sin sin L L m,n,m,n However, it turns out that m and m and n and n do not need to e chosen to e independent. This can e seen from the Green s function equation given here as a differentia equation in x x G x, x = δ 3 x x In cyindrica coordinates, this reads ρ ρ ρ ρ + ρ φ + z Gρ, φ, z; ρ, φ, z = ρ δρ ρ δφ φ δz z 3

4 Using the competeness reations and suggests that we take n= m= e imφ φ = πδφ φ 4 nπz nπz sin sin L L = L δz z G x, x = n= m= gρ, ρ e imφ φ sin nπz nπz sin L L 5 Sustituting this decomposition into 3 gives d ρ dρ ρ d dρ m ρ Making the sustitution nπ L gρ, ρ = 4 Lρ δρ, ρ x = nπρ L converts the homogeneous part of this to a modified Besse equation d dx + x d dx + m x gx, x = 4 Lx δx, x At this stage, the soution ecomes standard. Noting that the modified Besse function I m x ows up as x and the function K m x ows up as x, we are eft with { gx, x AIm x x < x = BK m x x > x where the coefficients A and B are determined y the matching conditions g < = g >, d dx g < = d dx g > + 4 Lx at x = x. This system may e soved to yied A = 4 K m x Lx I mx K m x I m x K mx B = 4 I m x Lx I mx K m x I m x K mx

5 Noting that the modified Besse functions satisfy the Wronskian formua I ν xk νx I νxk ν x = x finay gives { Im xk m x x < x gx, x = 4 L I m x K m x x > x = 4 L I mx < K m x > where x < = minx, x, x > = maxx, x Converting x ack to ρ and sustituting into 5 then gives the desired Dirichet Green s function G x, x = 4 L n= m= e imφ φ sin nπz nπz sin L L I m nπρ< L nπρ> K m L Show that an aternative form of the Green function is G x, x = m= dk e imφ φ J m kρj m kρ sinhkz < sinhkl z > sinhkl This aternative form of the Green s function is derived y expanding in φ and ρ instead of φ and z. For the ρ expansion, we use the integra reation kj ν kρj ν kρ dk = ρ δρ ρ aong with the competeness reation 4 to motivate the decomposition G x, x = m= kdk g k z, z e imφ φ J m kρj m kρ 6 Since the Besse function J m kρ satisfies the Besse equation d dρ + ρ d dρ + k m ρ J m kρ = the sustitution of 6 into the Greens function equation 3 gives d dz k g k z, z = δz z

6 Since g k z, z vanishes at z = and z = L, this is a standard one-dimensiona Green s function proem. Writing { g k z, z A sinhkz z < z = B sinhkl z z > z we find that the matching and jump conditions ecome A sinhkz = B sinhkl z, A coshkz = B coshkl z + k This may e soved to give so that A = k g k z, z = Sustituting this into 6 then yieds G x, x = m= k sinhkl z, B = sinhkz sinhkl k sinhkl k sinhkl sinhkz < sinhkl z > dk e imφ φ J m kρj m kρ sinhkz < sinhkl z > sinhkl 3.6 Consider the Green function appropriate for Neumann oundary conditions for the voume V etween the concentric spherica surfaces defined y r = a and r =, a <. To e ae to use.46 for the potentia, impose the simpe constraint.45. Use an expansion in spherica harmonics of the form G x, x = g r, r P cos γ = where g r, r = r </r + > + f r, r. a Show that for >, the radia Green function has the symmetric form g r, r = r < r> a + rr + + a + r r rr + a+ + + r + r + There are severa approaches to this proem. However, we first consider the Neumann oundary condition.45 G x x n = ndy S

7 For this proem with two oundaries, the surface area S must e the area of oth oundaries ie it is the tota area surrounding the voume. Hence S = a +, and in particuar this is uniform constant in the anges. As a resut, this wi ony contriute to the = term in the expansion of the Green s function. More precisey, we coud write G x x n = ndy g r, r n P cos γ ndy = a + P cos γ Since the Legendre poynomias are orthogona, this impies that g r, r n = ndy a + δ, Noting that the outward norma is either in the ˆr or the ˆr direction for the sphere at a or, respectivey, we end up with two oundary condition equations g r, r r = a a + δ g r, r, r = a + δ, 7 Now that we have written down the oundary conditions for g r, r, we proceed to otain its expicit form. The suggestion of the proem is to write Since g r, r = r < r + > x x = + f r, r r< r> + P cos γ we see that the first term in g r, r is designed to give the singuar source deta function. The remaining term F x, x = f r, r P cos γ then soves the homogeneous equation x F x, x =. But we know how to sove Lapace s equation in spherica coordinates, and the resut is that the radia function must e of the form f r, r = A r + B r + Note that we are taking the Green s function equation to act on the x variae, where x may e thought of as a parameter constant giving the ocation of the deta function source. We thus have g r, r = r < r + > + A r + B r + 8

8 A that remains is to use the oundary conditions 7 to sove for A and B. For the inside sphere at a, we have whie for the outside sphere we have a r + + A a + B a + = δ, a r + + A + B + = δ, a + For we rewrite these equations as a + + A a + = + /r + + B + r which may e soved to give A = B + + a + r = + a + Inserting this into 8 yieds g r, r = r < r + > + r + a + = r < r> a + rr + + = + a + = + + a + r< a + /r + + a + + r a/r / a + + / + a/r + a r + a r < r > a + r + < + r a + r r + a + r rr + a+ + r + + a + r < r > r < r + > r > a + r > + r< + r r + which is vaid for. Note that in the ast few ines we have een ae to rewrite the Green s function in terms of a product of ur < and vr > where u and v satisfies Neumann oundary conditions at r = a and r =, respectivey. r + >

9 This is reated to another possie method of soving this proem. Using the Legendre identity = + P cos γ = δφ φ δcos θ cos θ the Green s function equation may e reduced to the one-dimensiona proem d d dr r + g dr r, r = + δr r Using the genera method for the Sturm-Liouvie proem, the Green s function is given y g r, r = + A u r < v r > where ur and vr sove the homogeneous equation and the constant A is fixed y the Wronskian, W u, v = A /r. For the oundary conditions 7 are homogeneous u r r =a = v r r = = It is easy to see that these are satisfied y ur = r + Computing the Wronskian gives which aows us to identify a + + r + vr = r r + u v u v = + a+ + + r A = a + This gives the resut of the ast ine of. Show that for = g r, r = a r > a + r + fr where fr is aritrary. Show expicity in.46 that answers for the potentia Φ x are independent of fr. The = case invoves a non-homogeneous oundary condition. Hence the resut of wi not work. Of course, we can sti work out the one-dimensiona deta

10 function proem with matching and jump conditions at r = r. However it is more direct to return to 9 and and to simpy sove those conditions for =. Both 9 and resut in a B = a + whie eaving A competey undetermined. Finay, since r is thought of as a parameter, this indicates that A = fr can e an aritrary function of r. The = Green s function is given y 8 g r, r = r > a a + r + fr Incidentay, we note that without the inhomogeneous Neumann oundary condition term /S there wi e no soution to the system 9 and for = uness is taken to. This demonstrates the inconsistency of simpy setting G/ n = for the Neumann Green s function. Note that, y setting fr = a /a + r we otain a symmetrica Green s function g r, r = a r > a + r + r On the other hand, the choice of fr is unphysica. This arises ecause, for the Neumann Green s function, the fr contriution to the potentia is given y Φ x = ρ x fr d 3 x + Φ x ɛ V S n fr da = fr ρ x d 3 x ɛ E x dâ ɛ V S = fr q enc ɛ E x dâ = ɛ y Gauss aw. It is important not to mix up r and r in this derivation. 3.7 Appy the Neumann Green function of Proem 3.6 to the situation in which the norma eectric fied is E r = E cos θ at the outer surface r = and is E r = on the inner surface r = a. a Show that the eectrostatic potentia inside the voume V is r cos θ Φ x = E p 3 + a3 r 3 where p = a/. Find the components of the eectric fied cos θ E r r, θ = E p 3 a3 sin θ r 3, E θ r, θ = E p 3 S + a3 r 3

11 Since there is no charge etween the spheres, the soution to e oundary vaue proem is given y Φ x = Φ x S n G x, x da = E r Ω G x, x dω r = = E G x, x cos θ dω By writing = E r = = P cos γ = r = + g r, r P cos γ cos θ dω m Y m ΩY m Ω and noting that cos θ = /3Y Ω, we end up with the expansion Φ x = E 3,m g r, Y m Ω + = E g r, Y Ω 3 3 = E cos θ g r, 3 Y m Ω Y Ω dω where we have used orthogonaity of the spherica harmonics. Inserting = into then gives Φ x = E cos θ r 3 3 a 3 + a3 3 r = E r cos θ a/ 3 + a3 r 3 3 This is the potentia for a constant eectric fied comined with an eectric dipoe. Defining p = a/, the components of the eectric fied are E r = Φ r = E cos θ p 3 a3 r 3, E θ = Φ r θ = E sin θ p 3 + a3 r 3 Note that the oundary conditions E r r=a = and E r r= = E cos θ are oviousy satisfied. On the other hand, the parae component of the fied, E θ, is non-vanishing on oth surfaces except at the poes. Physicay, this indicates that these surfaces are not conductors. Cacuate the Cartesian or cyindrica components of the fied, E z ad E ρ, and make a sketch or computer pot of the ines of eectric force for a typica case of p =.5.

12 Rewriting 3 as Φ x = E p 3 z + a3 z r 3 = E p 3 z + a 3 z ρ + z 3/ we otain E z = Φ z = E p 3 + a3 3ẑ r 3 E ρ = Φ ρ = E p 3 3a3 ẑ ˆρ r 3 where ˆρ = ρ/r, ẑ = z/r, and r = ρ + z. As indicated aove, this corresponds to a constant eectric fied comined with an eectric dipoe. For E >, a sketch of the eectric fied ines ooks ike This sketch indicates that the radia component of the eectric fied vanishes at the surface of the inner sphere.

Physics 505 Fall Homework Assignment #4 Solutions

Physics 505 Fall Homework Assignment #4 Solutions Physics 505 Fa 2005 Homework Assignment #4 Soutions Textbook probems: Ch. 3: 3.4, 3.6, 3.9, 3.0 3.4 The surface of a hoow conducting sphere of inner radius a is divided into an even number of equa segments

More information

Legendre Polynomials - Lecture 8

Legendre Polynomials - Lecture 8 Legendre Poynomias - Lecture 8 Introduction In spherica coordinates the separation of variabes for the function of the poar ange resuts in Legendre s equation when the soution is independent of the azimutha

More information

Jackson 4.10 Homework Problem Solution Dr. Christopher S. Baird University of Massachusetts Lowell

Jackson 4.10 Homework Problem Solution Dr. Christopher S. Baird University of Massachusetts Lowell Jackson 4.10 Homework Probem Soution Dr. Christopher S. Baird University of Massachusetts Lowe PROBLEM: Two concentric conducting spheres of inner and outer radii a and b, respectivey, carry charges ±.

More information

Separation of Variables and a Spherical Shell with Surface Charge

Separation of Variables and a Spherical Shell with Surface Charge Separation of Variabes and a Spherica She with Surface Charge In cass we worked out the eectrostatic potentia due to a spherica she of radius R with a surface charge density σθ = σ cos θ. This cacuation

More information

$, (2.1) n="# #. (2.2)

$, (2.1) n=# #. (2.2) Chapter. Eectrostatic II Notes: Most of the materia presented in this chapter is taken from Jackson, Chap.,, and 4, and Di Bartoo, Chap... Mathematica Considerations.. The Fourier series and the Fourier

More information

Notes: Most of the material presented in this chapter is taken from Jackson, Chap. 2, 3, and 4, and Di Bartolo, Chap. 2. 2π nx i a. ( ) = G n.

Notes: Most of the material presented in this chapter is taken from Jackson, Chap. 2, 3, and 4, and Di Bartolo, Chap. 2. 2π nx i a. ( ) = G n. Chapter. Eectrostatic II Notes: Most of the materia presented in this chapter is taken from Jackson, Chap.,, and 4, and Di Bartoo, Chap... Mathematica Considerations.. The Fourier series and the Fourier

More information

PHYS 110B - HW #1 Fall 2005, Solutions by David Pace Equations referenced as Eq. # are from Griffiths Problem statements are paraphrased

PHYS 110B - HW #1 Fall 2005, Solutions by David Pace Equations referenced as Eq. # are from Griffiths Problem statements are paraphrased PHYS 110B - HW #1 Fa 2005, Soutions by David Pace Equations referenced as Eq. # are from Griffiths Probem statements are paraphrased [1.] Probem 6.8 from Griffiths A ong cyinder has radius R and a magnetization

More information

MATH 172: MOTIVATION FOR FOURIER SERIES: SEPARATION OF VARIABLES

MATH 172: MOTIVATION FOR FOURIER SERIES: SEPARATION OF VARIABLES MATH 172: MOTIVATION FOR FOURIER SERIES: SEPARATION OF VARIABLES Separation of variabes is a method to sove certain PDEs which have a warped product structure. First, on R n, a inear PDE of order m is

More information

Lecture 8 February 18, 2010

Lecture 8 February 18, 2010 Sources of Eectromagnetic Fieds Lecture 8 February 18, 2010 We now start to discuss radiation in free space. We wi reorder the materia of Chapter 9, bringing sections 6 7 up front. We wi aso cover some

More information

Physics 506 Winter 2006 Homework Assignment #6 Solutions

Physics 506 Winter 2006 Homework Assignment #6 Solutions Physics 506 Winter 006 Homework Assignment #6 Soutions Textbook probems: Ch. 10: 10., 10.3, 10.7, 10.10 10. Eectromagnetic radiation with eiptic poarization, described (in the notation of Section 7. by

More information

Physics 116C Helmholtz s and Laplace s Equations in Spherical Polar Coordinates: Spherical Harmonics and Spherical Bessel Functions

Physics 116C Helmholtz s and Laplace s Equations in Spherical Polar Coordinates: Spherical Harmonics and Spherical Bessel Functions Physics 116C Hemhotz s an Lapace s Equations in Spherica Poar Coorinates: Spherica Harmonics an Spherica Besse Functions Peter Young Date: October 28, 2013) I. HELMHOLTZ S EQUATION As iscusse in cass,

More information

Math 124B January 31, 2012

Math 124B January 31, 2012 Math 124B January 31, 212 Viktor Grigoryan 7 Inhomogeneous boundary vaue probems Having studied the theory of Fourier series, with which we successfuy soved boundary vaue probems for the homogeneous heat

More information

221B Lecture Notes Notes on Spherical Bessel Functions

221B Lecture Notes Notes on Spherical Bessel Functions Definitions B Lecture Notes Notes on Spherica Besse Functions We woud ike to sove the free Schrödinger equation [ h d r R(r) = h k R(r). () m r dr r m R(r) is the radia wave function ψ( x) = R(r)Y m (θ,

More information

Section 6: Magnetostatics

Section 6: Magnetostatics agnetic fieds in matter Section 6: agnetostatics In the previous sections we assumed that the current density J is a known function of coordinates. In the presence of matter this is not aways true. The

More information

Gauss Law. 2. Gauss s Law: connects charge and field 3. Applications of Gauss s Law

Gauss Law. 2. Gauss s Law: connects charge and field 3. Applications of Gauss s Law Gauss Law 1. Review on 1) Couomb s Law (charge and force) 2) Eectric Fied (fied and force) 2. Gauss s Law: connects charge and fied 3. Appications of Gauss s Law Couomb s Law and Eectric Fied Couomb s

More information

Physics 235 Chapter 8. Chapter 8 Central-Force Motion

Physics 235 Chapter 8. Chapter 8 Central-Force Motion Physics 35 Chapter 8 Chapter 8 Centra-Force Motion In this Chapter we wi use the theory we have discussed in Chapter 6 and 7 and appy it to very important probems in physics, in which we study the motion

More information

11.1 One-dimensional Helmholtz Equation

11.1 One-dimensional Helmholtz Equation Chapter Green s Functions. One-dimensiona Hemhotz Equation Suppose we have a string driven by an externa force, periodic with frequency ω. The differentia equation here f is some prescribed function) 2

More information

Higher dimensional PDEs and multidimensional eigenvalue problems

Higher dimensional PDEs and multidimensional eigenvalue problems Higher dimensiona PEs and mutidimensiona eigenvaue probems 1 Probems with three independent variabes Consider the prototypica equations u t = u (iffusion) u tt = u (W ave) u zz = u (Lapace) where u = u

More information

Assignment 7 Due Tuessday, March 29, 2016

Assignment 7 Due Tuessday, March 29, 2016 Math 45 / AMCS 55 Dr. DeTurck Assignment 7 Due Tuessday, March 9, 6 Topics for this week Convergence of Fourier series; Lapace s equation and harmonic functions: basic properties, compuations on rectanges

More information

LECTURE NOTES 9 TRACELESS SYMMETRIC TENSOR APPROACH TO LEGENDRE POLYNOMIALS AND SPHERICAL HARMONICS

LECTURE NOTES 9 TRACELESS SYMMETRIC TENSOR APPROACH TO LEGENDRE POLYNOMIALS AND SPHERICAL HARMONICS MASSACHUSETTS INSTITUTE OF TECHNOLOGY Physics Department Physics 8.07: Eectromagnetism II October 7, 202 Prof. Aan Guth LECTURE NOTES 9 TRACELESS SYMMETRIC TENSOR APPROACH TO LEGENDRE POLYNOMIALS AND SPHERICAL

More information

Radiation Fields. Lecture 12

Radiation Fields. Lecture 12 Radiation Fieds Lecture 12 1 Mutipoe expansion Separate Maxwe s equations into two sets of equations, each set separatey invoving either the eectric or the magnetic fied. After remova of the time dependence

More information

LECTURE NOTES 8 THE TRACELESS SYMMETRIC TENSOR EXPANSION AND STANDARD SPHERICAL HARMONICS

LECTURE NOTES 8 THE TRACELESS SYMMETRIC TENSOR EXPANSION AND STANDARD SPHERICAL HARMONICS MASSACHUSETTS INSTITUTE OF TECHNOLOGY Physics Department Physics 8.07: Eectromagnetism II October, 202 Prof. Aan Guth LECTURE NOTES 8 THE TRACELESS SYMMETRIC TENSOR EXPANSION AND STANDARD SPHERICAL HARMONICS

More information

4 1-D Boundary Value Problems Heat Equation

4 1-D Boundary Value Problems Heat Equation 4 -D Boundary Vaue Probems Heat Equation The main purpose of this chapter is to study boundary vaue probems for the heat equation on a finite rod a x b. u t (x, t = ku xx (x, t, a < x < b, t > u(x, = ϕ(x

More information

SEMINAR 2. PENDULUMS. V = mgl cos θ. (2) L = T V = 1 2 ml2 θ2 + mgl cos θ, (3) d dt ml2 θ2 + mgl sin θ = 0, (4) θ + g l

SEMINAR 2. PENDULUMS. V = mgl cos θ. (2) L = T V = 1 2 ml2 θ2 + mgl cos θ, (3) d dt ml2 θ2 + mgl sin θ = 0, (4) θ + g l Probem 7. Simpe Penduum SEMINAR. PENDULUMS A simpe penduum means a mass m suspended by a string weightess rigid rod of ength so that it can swing in a pane. The y-axis is directed down, x-axis is directed

More information

Lecture 17 - The Secrets we have Swept Under the Rug

Lecture 17 - The Secrets we have Swept Under the Rug Lecture 17 - The Secrets we have Swept Under the Rug Today s ectures examines some of the uirky features of eectrostatics that we have negected up unti this point A Puzze... Let s go back to the basics

More information

In Coulomb gauge, the vector potential is then given by

In Coulomb gauge, the vector potential is then given by Physics 505 Fa 007 Homework Assignment #8 Soutions Textbook probems: Ch. 5: 5.13, 5.14, 5.15, 5.16 5.13 A sphere of raius a carries a uniform surface-charge istribution σ. The sphere is rotate about a

More information

Cluster modelling. Collisions. Stellar Dynamics & Structure of Galaxies handout #2. Just as a self-gravitating collection of objects.

Cluster modelling. Collisions. Stellar Dynamics & Structure of Galaxies handout #2. Just as a self-gravitating collection of objects. Stear Dynamics & Structure of Gaaxies handout # Custer modeing Just as a sef-gravitating coection of objects. Coisions Do we have to worry about coisions? Gobuar custers ook densest, so obtain a rough

More information

Week 6 Lectures, Math 6451, Tanveer

Week 6 Lectures, Math 6451, Tanveer Fourier Series Week 6 Lectures, Math 645, Tanveer In the context of separation of variabe to find soutions of PDEs, we encountered or and in other cases f(x = f(x = a 0 + f(x = a 0 + b n sin nπx { a n

More information

David Eigen. MA112 Final Paper. May 10, 2002

David Eigen. MA112 Final Paper. May 10, 2002 David Eigen MA112 Fina Paper May 1, 22 The Schrodinger equation describes the position of an eectron as a wave. The wave function Ψ(t, x is interpreted as a probabiity density for the position of the eectron.

More information

14 Separation of Variables Method

14 Separation of Variables Method 14 Separation of Variabes Method Consider, for exampe, the Dirichet probem u t = Du xx < x u(x, ) = f(x) < x < u(, t) = = u(, t) t > Let u(x, t) = T (t)φ(x); now substitute into the equation: dt

More information

6 Wave Equation on an Interval: Separation of Variables

6 Wave Equation on an Interval: Separation of Variables 6 Wave Equation on an Interva: Separation of Variabes 6.1 Dirichet Boundary Conditions Ref: Strauss, Chapter 4 We now use the separation of variabes technique to study the wave equation on a finite interva.

More information

Physics 566: Quantum Optics Quantization of the Electromagnetic Field

Physics 566: Quantum Optics Quantization of the Electromagnetic Field Physics 566: Quantum Optics Quantization of the Eectromagnetic Fied Maxwe's Equations and Gauge invariance In ecture we earned how to quantize a one dimensiona scaar fied corresponding to vibrations on

More information

Gauss s law - plane symmetry

Gauss s law - plane symmetry Gauss s aw - pane symmetry Submitted by: I.D. 3923262 Find the eectric fied aong the z-axis of an infinite uniformey charged pane at the x y pane (charge density σ) with a hoe at the origin of a radius

More information

Week 5 Lectures, Math 6451, Tanveer

Week 5 Lectures, Math 6451, Tanveer Week 5 Lectures, Math 651, Tanveer 1 Separation of variabe method The method of separation of variabe is a suitabe technique for determining soutions to inear PDEs, usuay with constant coefficients, when

More information

2M2. Fourier Series Prof Bill Lionheart

2M2. Fourier Series Prof Bill Lionheart M. Fourier Series Prof Bi Lionheart 1. The Fourier series of the periodic function f(x) with period has the form f(x) = a 0 + ( a n cos πnx + b n sin πnx ). Here the rea numbers a n, b n are caed the Fourier

More information

More Scattering: the Partial Wave Expansion

More Scattering: the Partial Wave Expansion More Scattering: the Partia Wave Expansion Michae Fower /7/8 Pane Waves and Partia Waves We are considering the soution to Schrödinger s equation for scattering of an incoming pane wave in the z-direction

More information

Math 124B January 17, 2012

Math 124B January 17, 2012 Math 124B January 17, 212 Viktor Grigoryan 3 Fu Fourier series We saw in previous ectures how the Dirichet and Neumann boundary conditions ead to respectivey sine and cosine Fourier series of the initia

More information

FFTs in Graphics and Vision. Spherical Convolution and Axial Symmetry Detection

FFTs in Graphics and Vision. Spherical Convolution and Axial Symmetry Detection FFTs in Graphics and Vision Spherica Convoution and Axia Symmetry Detection Outine Math Review Symmetry Genera Convoution Spherica Convoution Axia Symmetry Detection Math Review Symmetry: Given a unitary

More information

Lecture Notes for Math 251: ODE and PDE. Lecture 32: 10.2 Fourier Series

Lecture Notes for Math 251: ODE and PDE. Lecture 32: 10.2 Fourier Series Lecture Notes for Math 251: ODE and PDE. Lecture 32: 1.2 Fourier Series Shawn D. Ryan Spring 212 Last Time: We studied the heat equation and the method of Separation of Variabes. We then used Separation

More information

Chapter 4: Electrostatic Fields in Matter

Chapter 4: Electrostatic Fields in Matter Chapter 4: Eectrostatic Fieds in Matter 4. Poarization 4. The Fied of a Poarized Oject 4.3 The Eectric Dispacement 4.4 Sef-Consistance of Eectric Fied and Poarization; Linear Dieectrics 4. Poarization

More information

arxiv: v1 [hep-th] 10 Dec 2018

arxiv: v1 [hep-th] 10 Dec 2018 Casimir energy of an open string with ange-dependent boundary condition A. Jahan 1 and I. Brevik 2 1 Research Institute for Astronomy and Astrophysics of Maragha (RIAAM, Maragha, Iran 2 Department of Energy

More information

9. EXERCISES ON THE FINITE-ELEMENT METHOD

9. EXERCISES ON THE FINITE-ELEMENT METHOD 9. EXERCISES O THE FIITE-ELEMET METHOD Exercise Thickness: t=; Pane strain proem (ν 0): Surface oad Voume oad; 4 p f ( x, ) ( x ) 0 E D 0 0 0 ( ) 4 p F( xy, ) Interna constrain: rigid rod etween D and

More information

Quantum Mechanical Models of Vibration and Rotation of Molecules Chapter 18

Quantum Mechanical Models of Vibration and Rotation of Molecules Chapter 18 Quantum Mechanica Modes of Vibration and Rotation of Moecues Chapter 18 Moecuar Energy Transationa Vibrationa Rotationa Eectronic Moecuar Motions Vibrations of Moecues: Mode approximates moecues to atoms

More information

Course 2BA1, Section 11: Periodic Functions and Fourier Series

Course 2BA1, Section 11: Periodic Functions and Fourier Series Course BA, 8 9 Section : Periodic Functions and Fourier Series David R. Wikins Copyright c David R. Wikins 9 Contents Periodic Functions and Fourier Series 74. Fourier Series of Even and Odd Functions...........

More information

12.2. Maxima and Minima. Introduction. Prerequisites. Learning Outcomes

12.2. Maxima and Minima. Introduction. Prerequisites. Learning Outcomes Maima and Minima 1. Introduction In this Section we anayse curves in the oca neighbourhood of a stationary point and, from this anaysis, deduce necessary conditions satisfied by oca maima and oca minima.

More information

CS229 Lecture notes. Andrew Ng

CS229 Lecture notes. Andrew Ng CS229 Lecture notes Andrew Ng Part IX The EM agorithm In the previous set of notes, we taked about the EM agorithm as appied to fitting a mixture of Gaussians. In this set of notes, we give a broader view

More information

Module 22: Simple Harmonic Oscillation and Torque

Module 22: Simple Harmonic Oscillation and Torque Modue : Simpe Harmonic Osciation and Torque.1 Introduction We have aready used Newton s Second Law or Conservation of Energy to anayze systems ike the boc-spring system that osciate. We sha now use torque

More information

Supporting Information for Suppressing Klein tunneling in graphene using a one-dimensional array of localized scatterers

Supporting Information for Suppressing Klein tunneling in graphene using a one-dimensional array of localized scatterers Supporting Information for Suppressing Kein tunneing in graphene using a one-dimensiona array of ocaized scatterers Jamie D Was, and Danie Hadad Department of Chemistry, University of Miami, Cora Gabes,

More information

MAT 167: Advanced Linear Algebra

MAT 167: Advanced Linear Algebra < Proem 1 (15 pts) MAT 167: Advanced Linear Agera Fina Exam Soutions (a) (5 pts) State the definition of a unitary matrix and expain the difference etween an orthogona matrix and an unitary matrix. Soution:

More information

C. Fourier Sine Series Overview

C. Fourier Sine Series Overview 12 PHILIP D. LOEWEN C. Fourier Sine Series Overview Let some constant > be given. The symboic form of the FSS Eigenvaue probem combines an ordinary differentia equation (ODE) on the interva (, ) with a

More information

HYDROGEN ATOM SELECTION RULES TRANSITION RATES

HYDROGEN ATOM SELECTION RULES TRANSITION RATES DOING PHYSICS WITH MATLAB QUANTUM PHYSICS Ian Cooper Schoo of Physics, University of Sydney ian.cooper@sydney.edu.au HYDROGEN ATOM SELECTION RULES TRANSITION RATES DOWNLOAD DIRECTORY FOR MATLAB SCRIPTS

More information

MATH 131P: PRACTICE FINAL SOLUTIONS DECEMBER 12, 2012

MATH 131P: PRACTICE FINAL SOLUTIONS DECEMBER 12, 2012 MATH 3P: PRACTICE FINAL SOLUTIONS DECEMBER, This is a closed ook, closed notes, no calculators/computers exam. There are 6 prolems. Write your solutions to Prolems -3 in lue ook #, and your solutions to

More information

Jackson 3.3 Homework Problem Solution Dr. Christopher S. Baird University of Massachusetts Lowell

Jackson 3.3 Homework Problem Solution Dr. Christopher S. Baird University of Massachusetts Lowell Jackson 3.3 Homewok Pobem Soution D. Chistophe S. Baid Univesity of Massachusetts Lowe POBLEM: A thin, fat, conducting, cicua disc of adius is ocated in the x-y pane with its cente at the oigin, and is

More information

Lecture Notes for Math 251: ODE and PDE. Lecture 34: 10.7 Wave Equation and Vibrations of an Elastic String

Lecture Notes for Math 251: ODE and PDE. Lecture 34: 10.7 Wave Equation and Vibrations of an Elastic String ecture Notes for Math 251: ODE and PDE. ecture 3: 1.7 Wave Equation and Vibrations of an Eastic String Shawn D. Ryan Spring 212 ast Time: We studied other Heat Equation probems with various other boundary

More information

Wave Equation Dirichlet Boundary Conditions

Wave Equation Dirichlet Boundary Conditions Wave Equation Dirichet Boundary Conditions u tt x, t = c u xx x, t, < x 1 u, t =, u, t = ux, = fx u t x, = gx Look for simpe soutions in the form ux, t = XxT t Substituting into 13 and dividing

More information

1 Heat Equation Dirichlet Boundary Conditions

1 Heat Equation Dirichlet Boundary Conditions Chapter 3 Heat Exampes in Rectanges Heat Equation Dirichet Boundary Conditions u t (x, t) = ku xx (x, t), < x (.) u(, t) =, u(, t) = u(x, ) = f(x). Separate Variabes Look for simpe soutions in the

More information

THE NUMERICAL EVALUATION OF THE LEVITATION FORCE IN A HYDROSTATIC BEARING WITH ALTERNATING POLES

THE NUMERICAL EVALUATION OF THE LEVITATION FORCE IN A HYDROSTATIC BEARING WITH ALTERNATING POLES THE NUMERICAL EVALUATION OF THE LEVITATION FORCE IN A HYDROSTATIC BEARING WITH ALTERNATING POLES MARIAN GRECONICI Key words: Magnetic iquid, Magnetic fied, 3D-FEM, Levitation, Force, Bearing. The magnetic

More information

Strauss PDEs 2e: Section Exercise 2 Page 1 of 12. For problem (1), complete the calculation of the series in case j(t) = 0 and h(t) = e t.

Strauss PDEs 2e: Section Exercise 2 Page 1 of 12. For problem (1), complete the calculation of the series in case j(t) = 0 and h(t) = e t. Strauss PDEs e: Section 5.6 - Exercise Page 1 of 1 Exercise For probem (1, compete the cacuation of the series in case j(t = and h(t = e t. Soution With j(t = and h(t = e t, probem (1 on page 147 becomes

More information

Math 220B - Summer 2003 Homework 1 Solutions

Math 220B - Summer 2003 Homework 1 Solutions Math 0B - Summer 003 Homework Soutions Consider the eigenvaue probem { X = λx 0 < x < X satisfies symmetric BCs x = 0, Suppose f(x)f (x) x=b x=a 0 for a rea-vaued functions f(x) which satisfy the boundary

More information

Chemical Kinetics Part 2. Chapter 16

Chemical Kinetics Part 2. Chapter 16 Chemica Kinetics Part 2 Chapter 16 Integrated Rate Laws The rate aw we have discussed thus far is the differentia rate aw. Let us consider the very simpe reaction: a A à products The differentia rate reates

More information

Applied Nuclear Physics (Fall 2006) Lecture 7 (10/2/06) Overview of Cross Section Calculation

Applied Nuclear Physics (Fall 2006) Lecture 7 (10/2/06) Overview of Cross Section Calculation 22.101 Appied Nucear Physics (Fa 2006) Lecture 7 (10/2/06) Overview of Cross Section Cacuation References P. Roman, Advanced Quantum Theory (Addison-Wesey, Reading, 1965), Chap 3. A. Foderaro, The Eements

More information

Solution Set Seven. 1 Goldstein Components of Torque Along Principal Axes Components of Torque Along Cartesian Axes...

Solution Set Seven. 1 Goldstein Components of Torque Along Principal Axes Components of Torque Along Cartesian Axes... : Soution Set Seven Northwestern University, Cassica Mechanics Cassica Mechanics, Third Ed.- Godstein November 8, 25 Contents Godstein 5.8. 2. Components of Torque Aong Principa Axes.......................

More information

PhysicsAndMathsTutor.com

PhysicsAndMathsTutor.com . Two points A and B ie on a smooth horizonta tabe with AB = a. One end of a ight eastic spring, of natura ength a and moduus of easticity mg, is attached to A. The other end of the spring is attached

More information

Fourier Series. 10 (D3.9) Find the Cesàro sum of the series. 11 (D3.9) Let a and b be real numbers. Under what conditions does a series of the form

Fourier Series. 10 (D3.9) Find the Cesàro sum of the series. 11 (D3.9) Let a and b be real numbers. Under what conditions does a series of the form Exercises Fourier Anaysis MMG70, Autumn 007 The exercises are taken from: Version: Monday October, 007 DXY Section XY of H F Davis, Fourier Series and orthogona functions EÖ Some exercises from earier

More information

Bohr s atomic model. 1 Ze 2 = mv2. n 2 Z

Bohr s atomic model. 1 Ze 2 = mv2. n 2 Z Bohr s atomic mode Another interesting success of the so-caed od quantum theory is expaining atomic spectra of hydrogen and hydrogen-ike atoms. The eectromagnetic radiation emitted by free atoms is concentrated

More information

4 Separation of Variables

4 Separation of Variables 4 Separation of Variabes In this chapter we describe a cassica technique for constructing forma soutions to inear boundary vaue probems. The soution of three cassica (paraboic, hyperboic and eiptic) PDE

More information

ANISOTROPIES OF THE MICROWAVE BACKGROUND

ANISOTROPIES OF THE MICROWAVE BACKGROUND ANISOTROPIES OF THE MICROWAVE BACKGROUND The Universe just before recombination is a very tighty couped fuid, due to the arge eectromagnetic Thomson cross section. Photons scatter off charged partices

More information

Dual Integral Equations and Singular Integral. Equations for Helmholtz Equation

Dual Integral Equations and Singular Integral. Equations for Helmholtz Equation Int.. Contemp. Math. Sciences, Vo. 4, 9, no. 34, 1695-1699 Dua Integra Equations and Singuar Integra Equations for Hemhotz Equation Naser A. Hoshan Department of Mathematics TafiaTechnica University P.O.

More information

An approximate method for solving the inverse scattering problem with fixed-energy data

An approximate method for solving the inverse scattering problem with fixed-energy data J. Inv. I-Posed Probems, Vo. 7, No. 6, pp. 561 571 (1999) c VSP 1999 An approximate method for soving the inverse scattering probem with fixed-energy data A. G. Ramm and W. Scheid Received May 12, 1999

More information

Chemical Kinetics Part 2

Chemical Kinetics Part 2 Integrated Rate Laws Chemica Kinetics Part 2 The rate aw we have discussed thus far is the differentia rate aw. Let us consider the very simpe reaction: a A à products The differentia rate reates the rate

More information

Physics 505 Fall 2005 Homework Assignment #8 Solutions

Physics 505 Fall 2005 Homework Assignment #8 Solutions Physics 55 Fall 5 Homework Assignment #8 Solutions Textbook problems: Ch. 5: 5., 5.4, 5.7, 5.9 5. A circular current loop of radius a carrying a current I lies in the x-y plane with its center at the origin.

More information

Electromagnetism Spring 2018, NYU

Electromagnetism Spring 2018, NYU Eectromagnetism Spring 08, NYU March 6, 08 Time-dependent fieds We now consider the two phenomena missing from the static fied case: Faraday s Law of induction and Maxwe s dispacement current. Faraday

More information

MA 201: Partial Differential Equations Lecture - 10

MA 201: Partial Differential Equations Lecture - 10 MA 201: Partia Differentia Equations Lecture - 10 Separation of Variabes, One dimensiona Wave Equation Initia Boundary Vaue Probem (IBVP) Reca: A physica probem governed by a PDE may contain both boundary

More information

CONCHOID OF NICOMEDES AND LIMACON OF PASCAL AS ELECTRODE OF STATIC FIELD AND AS WAVEGUIDE OF HIGH FREQUENCY WAVE

CONCHOID OF NICOMEDES AND LIMACON OF PASCAL AS ELECTRODE OF STATIC FIELD AND AS WAVEGUIDE OF HIGH FREQUENCY WAVE Progress In Eectromagnetics Research, PIER 30, 73 84, 001 CONCHOID OF NICOMEDES AND LIMACON OF PASCAL AS ELECTRODE OF STATIC FIELD AND AS WAVEGUIDE OF HIGH FREQUENCY WAVE W. Lin and Z. Yu University of

More information

APPENDIX C FLEXING OF LENGTH BARS

APPENDIX C FLEXING OF LENGTH BARS Fexing of ength bars 83 APPENDIX C FLEXING OF LENGTH BARS C.1 FLEXING OF A LENGTH BAR DUE TO ITS OWN WEIGHT Any object ying in a horizonta pane wi sag under its own weight uness it is infinitey stiff or

More information

Why Doesn t a Steady Current Loop Radiate?

Why Doesn t a Steady Current Loop Radiate? Why Doesn t a Steady Current Loop Radiate? Probem Kirk T. McDonad Joseph Henry Laboratories, Princeton University, Princeton, NJ 8544 December, 2; updated March 22, 26 A steady current in a circuar oop

More information

Chapter 5. Wave equation. 5.1 Physical derivation

Chapter 5. Wave equation. 5.1 Physical derivation Chapter 5 Wave equation In this chapter, we discuss the wave equation u tt a 2 u = f, (5.1) where a > is a constant. We wi discover that soutions of the wave equation behave in a different way comparing

More information

Term Test AER301F. Dynamics. 5 November The value of each question is indicated in the table opposite.

Term Test AER301F. Dynamics. 5 November The value of each question is indicated in the table opposite. U N I V E R S I T Y O F T O R O N T O Facuty of Appied Science and Engineering Term Test AER31F Dynamics 5 November 212 Student Name: Last Name First Names Student Number: Instructions: 1. Attempt a questions.

More information

Homework #04 Answers and Hints (MATH4052 Partial Differential Equations)

Homework #04 Answers and Hints (MATH4052 Partial Differential Equations) Homework #4 Answers and Hints (MATH452 Partia Differentia Equations) Probem 1 (Page 89, Q2) Consider a meta rod ( < x < ), insuated aong its sides but not at its ends, which is initiay at temperature =

More information

Lecture Note 3: Stationary Iterative Methods

Lecture Note 3: Stationary Iterative Methods MATH 5330: Computationa Methods of Linear Agebra Lecture Note 3: Stationary Iterative Methods Xianyi Zeng Department of Mathematica Sciences, UTEP Stationary Iterative Methods The Gaussian eimination (or

More information

arxiv: v1 [math.ca] 6 Mar 2017

arxiv: v1 [math.ca] 6 Mar 2017 Indefinite Integras of Spherica Besse Functions MIT-CTP/487 arxiv:703.0648v [math.ca] 6 Mar 07 Joyon K. Boomfied,, Stephen H. P. Face,, and Zander Moss, Center for Theoretica Physics, Laboratory for Nucear

More information

Theoretical Cosmology

Theoretical Cosmology Theoretica Cosmoogy Ruth Durrer, Roy Maartens, Costas Skordis Geneva, Capetown, Nottingham Benasque, February 16 2011 Ruth Durrer (Université de Genève) Theoretica Cosmoogy Benasque 2011 1 / 14 Theoretica

More information

APPENDIX B. Some special functions in low-frequency seismology. 2l +1 x j l (B.2) j l = j l 1 l +1 x j l (B.3) j l = l x j l j l+1

APPENDIX B. Some special functions in low-frequency seismology. 2l +1 x j l (B.2) j l = j l 1 l +1 x j l (B.3) j l = l x j l j l+1 APPENDIX B Soe specia functions in ow-frequency seisoogy 1. Spherica Besse functions The functions j and y are usefu in constructing ode soutions in hoogeneous spheres (fig B1). They satisfy d 2 j dr 2

More information

Solutions to Laplace s Equation in Cylindrical Coordinates and Numerical solutions. ρ + (1/ρ) 2 V

Solutions to Laplace s Equation in Cylindrical Coordinates and Numerical solutions. ρ + (1/ρ) 2 V Solutions to Laplace s Equation in Cylindrical Coordinates and Numerical solutions Lecture 8 1 Introduction Solutions to Laplace s equation can be obtained using separation of variables in Cartesian and

More information

1.2 Partial Wave Analysis

1.2 Partial Wave Analysis February, 205 Lecture X.2 Partia Wave Anaysis We have described scattering in terms of an incoming pane wave, a momentum eigenet, and and outgoing spherica wave, aso with definite momentum. We now consider

More information

ESCI 340 Physical Meteorology Radiation Lesson 5 Terrestrial Radiation and Radiation Balance Dr. DeCaria

ESCI 340 Physical Meteorology Radiation Lesson 5 Terrestrial Radiation and Radiation Balance Dr. DeCaria ECI 30 Physica Meteoroogy Radiation Lesson 5 errestria Radiation and Radiation Baance Dr. DeCaria References: Atmospheric cience: An Introductory urvey, Waace and Hobbs An Introduction to Atmospheric Radiation,

More information

Agenda Administrative Matters Atomic Physics Molecules

Agenda Administrative Matters Atomic Physics Molecules Fromm Institute for Lifeong Learning University of San Francisco Modern Physics for Frommies IV The Universe - Sma to Large Lecture 3 Agenda Administrative Matters Atomic Physics Moecues Administrative

More information

Volume 13, MAIN ARTICLES

Volume 13, MAIN ARTICLES Voume 13, 2009 1 MAIN ARTICLES THE BASIC BVPs OF THE THEORY OF ELASTIC BINARY MIXTURES FOR A HALF-PLANE WITH CURVILINEAR CUTS Bitsadze L. I. Vekua Institute of Appied Mathematics of Iv. Javakhishvii Tbiisi

More information

Introduction to LMTO method

Introduction to LMTO method 1 Introduction to MTO method 24 February 2011; V172 P.Ravindran, FME-course on Ab initio Modeing of soar ce Materias 24 February 2011 Introduction to MTO method Ab initio Eectronic Structure Cacuations

More information

c 2007 Society for Industrial and Applied Mathematics

c 2007 Society for Industrial and Applied Mathematics SIAM REVIEW Vo. 49,No. 1,pp. 111 1 c 7 Society for Industria and Appied Mathematics Domino Waves C. J. Efthimiou M. D. Johnson Abstract. Motivated by a proposa of Daykin [Probem 71-19*, SIAM Rev., 13 (1971),

More information

1D Heat Propagation Problems

1D Heat Propagation Problems Chapter 1 1D Heat Propagation Probems If the ambient space of the heat conduction has ony one dimension, the Fourier equation reduces to the foowing for an homogeneous body cρ T t = T λ 2 + Q, 1.1) x2

More information

1. Measurements and error calculus

1. Measurements and error calculus EV 1 Measurements and error cacuus 11 Introduction The goa of this aboratory course is to introduce the notions of carrying out an experiment, acquiring and writing up the data, and finay anayzing the

More information

THE THREE POINT STEINER PROBLEM ON THE FLAT TORUS: THE MINIMAL LUNE CASE

THE THREE POINT STEINER PROBLEM ON THE FLAT TORUS: THE MINIMAL LUNE CASE THE THREE POINT STEINER PROBLEM ON THE FLAT TORUS: THE MINIMAL LUNE CASE KATIE L. MAY AND MELISSA A. MITCHELL Abstract. We show how to identify the minima path network connecting three fixed points on

More information

First-Order Corrections to Gutzwiller s Trace Formula for Systems with Discrete Symmetries

First-Order Corrections to Gutzwiller s Trace Formula for Systems with Discrete Symmetries c 26 Noninear Phenomena in Compex Systems First-Order Corrections to Gutzwier s Trace Formua for Systems with Discrete Symmetries Hoger Cartarius, Jörg Main, and Günter Wunner Institut für Theoretische

More information

Extraction of Astrophysical Cross Sections in the Trojan-Horse Method

Extraction of Astrophysical Cross Sections in the Trojan-Horse Method Few-Body Systems 29, 75±93 (2000) Extraction of Astrophysica Cross Sections in the Trojan-Horse Method S. Type and H. H. Woter Sektion Physik, Universitat Munchen, Am Couomwa 1, D-85748 Garching, Germany

More information

b n n=1 a n cos nx (3) n=1

b n n=1 a n cos nx (3) n=1 Fourier Anaysis The Fourier series First some terminoogy: a function f(x) is periodic if f(x ) = f(x) for a x for some, if is the smaest such number, it is caed the period of f(x). It is even if f( x)

More information

Elements of Kinetic Theory

Elements of Kinetic Theory Eements of Kinetic Theory Statistica mechanics Genera description computation of macroscopic quantities Equiibrium: Detaied Baance/ Equipartition Fuctuations Diffusion Mean free path Brownian motion Diffusion

More information

Physics 127c: Statistical Mechanics. Fermi Liquid Theory: Collective Modes. Boltzmann Equation. The quasiparticle energy including interactions

Physics 127c: Statistical Mechanics. Fermi Liquid Theory: Collective Modes. Boltzmann Equation. The quasiparticle energy including interactions Physics 27c: Statistica Mechanics Fermi Liquid Theory: Coective Modes Botzmann Equation The quasipartice energy incuding interactions ε p,σ = ε p + f(p, p ; σ, σ )δn p,σ, () p,σ with ε p ε F + v F (p p

More information

1.1 a.) Suppose we have a conductor and place some charge density within it. For a surface S inside the conductor enclose the charge density!

1.1 a.) Suppose we have a conductor and place some charge density within it. For a surface S inside the conductor enclose the charge density! 1.1 a. uppose we have a conductor and place some charge density within it. # Q = d 3 x x V ( For a surface inside the conductor enclose the charge density E d a = 1 d 3 x $ %( x$ # V This will cause an

More information

MA 201: Partial Differential Equations Lecture - 11

MA 201: Partial Differential Equations Lecture - 11 MA 201: Partia Differentia Equations Lecture - 11 Heat Equation Heat conduction in a thin rod The IBVP under consideration consists of: The governing equation: u t = αu xx, (1) where α is the therma diffusivity.

More information