Wave Phenomena Physics 15c. Lecture 12 Multi-Dimensional Waves

Similar documents
Wave Phenomena Physics 15c

Wave Phenomena Physics 15c

Summary: Method of Separation of Variables

Waveguide Guide: A and V. Ross L. Spencer

4 The dynamical FRW universe

( ) 2. ( ) is the Fourier transform of! ( x). ( ) ( ) ( ) = Ae i kx"#t ( ) = 1 2" ( )"( x,t) PC 3101 Quantum Mechanics Section 1

The Wave Equation I. MA 436 Kurt Bryan

Conducting Ellipsoid and Circular Disk

Chapter 4 Contravariance, Covariance, and Spacetime Diagrams

Consequently, the temperature must be the same at each point in the cross section at x. Let:

Partial Derivatives. Limits. For a single variable function f (x), the limit lim

Heat flux and total heat

potentials A z, F z TE z Modes We use the e j z z =0 we can simply say that the x dependence of E y (1)

Math 124A October 04, 2011

Waveguides Free Space. Modal Excitation. Daniel S. Weile. Department of Electrical and Computer Engineering University of Delaware

Riemann Sums and Riemann Integrals

Physics 116C Solution of inhomogeneous ordinary differential equations using Green s functions

Riemann Sums and Riemann Integrals

Aike ikx Bike ikx. = 2k. solving for. A = k iκ

Improper Integrals, and Differential Equations

Recitation 3: More Applications of the Derivative

Energy Bands Energy Bands and Band Gap. Phys463.nb Phenomenon

Problems for HW X. C. Gwinn. November 30, 2009

Phys 6321 Final Exam - Solutions May 3, 2013

PHYSICS 116C Homework 4 Solutions

Math 100 Review Sheet

3 Mathematics of the Poisson Equation

We partition C into n small arcs by forming a partition of [a, b] by picking s i as follows: a = s 0 < s 1 < < s n = b.

Test , 8.2, 8.4 (density only), 8.5 (work only), 9.1, 9.2 and 9.3 related test 1 material and material from prior classes

Candidates must show on each answer book the type of calculator used.

Surface Integrals of Vector Fields

Applied Physics Introduction to Vibrations and Waves (with a focus on elastic waves) Course Outline

Jackson 2.26 Homework Problem Solution Dr. Christopher S. Baird University of Massachusetts Lowell

Line and Surface Integrals: An Intuitive Understanding

Best Approximation. Chapter The General Case

Orthogonal functions

13.4 Work done by Constant Forces

Lecture 3. Limits of Functions and Continuity

Name Solutions to Test 3 November 8, 2017

Kinematic Waves. These are waves which result from the conservation equation. t + I = 0. (2)

Section 14.3 Arc Length and Curvature

PHYS 4390: GENERAL RELATIVITY LECTURE 6: TENSOR CALCULUS

The Regulated and Riemann Integrals

MATH 144: Business Calculus Final Review

(uv) = u v + uv, (1) u vdx + b [uv] b a = u vdx + u v dx. (8) u vds =

1 1D heat and wave equations on a finite interval

CHAPTER 4 MULTIPLE INTEGRALS

(4.1) D r v(t) ω(t, v(t))

This final is a three hour open book, open notes exam. Do all four problems.

Math 32B Discussion Session Session 7 Notes August 28, 2018

Linearly Similar Polynomials

CHM Physical Chemistry I Chapter 1 - Supplementary Material

First midterm topics Second midterm topics End of quarter topics. Math 3B Review. Steve. 18 March 2009

Space Curves. Recall the parametric equations of a curve in xy-plane and compare them with parametric equations of a curve in space.

Chapter 0. What is the Lebesgue integral about?

Math 1102: Calculus I (Math/Sci majors) MWF 3pm, Fulton Hall 230 Homework 2 solutions

How do we solve these things, especially when they get complicated? How do we know when a system has a solution, and when is it unique?

Bases for Vector Spaces

Bernoulli Numbers Jeff Morton

Line Integrals. Partitioning the Curve. Estimating the Mass

Massachusetts Institute of Technology Quantum Mechanics I (8.04) Spring 2005 Solutions to Problem Set 6

THREE-DIMENSIONAL KINEMATICS OF RIGID BODIES

MATH34032: Green s Functions, Integral Equations and the Calculus of Variations 1

Point Lattices: Bravais Lattices

The solutions of the single electron Hamiltonian were shown to be Bloch wave of the form: ( ) ( ) ikr

7.1 Integral as Net Change and 7.2 Areas in the Plane Calculus

Quantum Physics I (8.04) Spring 2016 Assignment 8

The Dirac distribution

Functions of Several Variables

( dg. ) 2 dt. + dt. dt j + dh. + dt. r(t) dt. Comparing this equation with the one listed above for the length of see that

In-Class Problems 2 and 3: Projectile Motion Solutions. In-Class Problem 2: Throwing a Stone Down a Hill

Physics 741 Graduate Quantum Mechanics 1 Solutions to Final Exam, Fall 2011

along the vector 5 a) Find the plane s coordinate after 1 hour. b) Find the plane s coordinate after 2 hours. c) Find the plane s coordinate

DEFINITION OF ASSOCIATIVE OR DIRECT PRODUCT AND ROTATION OF VECTORS

Review of Gaussian Quadrature method

HOMEWORK SOLUTIONS MATH 1910 Sections 7.9, 8.1 Fall 2016

Generalizations of the Basic Functional

S56 (5.3) Vectors.notebook January 29, 2016

The Properties of Stars

R. I. Badran Solid State Physics

Chapter 3. Vector Spaces

JUST THE MATHS SLIDES NUMBER INTEGRATION APPLICATIONS 11 (Second moments of an area (A)) A.J.Hobson

Goals: Determine how to calculate the area described by a function. Define the definite integral. Explore the relationship between the definite

Spherical Coordinates

Problem set 1: Solutions Math 207B, Winter 2016

The area under the graph of f and above the x-axis between a and b is denoted by. f(x) dx. π O

l 2 p2 n 4n 2, the total surface area of the

Quantum Mechanics Qualifying Exam - August 2016 Notes and Instructions

Properties of Integrals, Indefinite Integrals. Goals: Definition of the Definite Integral Integral Calculations using Antiderivatives

Math 231E, Lecture 33. Parametric Calculus

1 Which of the following summarises the change in wave characteristics on going from infra-red to ultraviolet in the electromagnetic spectrum?

Notes on length and conformal metrics

Homework Assignment 6 Solution Set

Integrals - Motivation

Riemann is the Mann! (But Lebesgue may besgue to differ.)

12 TRANSFORMING BIVARIATE DENSITY FUNCTIONS

g i fφdx dx = x i i=1 is a Hilbert space. We shall, henceforth, abuse notation and write g i f(x) = f

DEFINITION The inner product of two functions f 1 and f 2 on an interval [a, b] is the number. ( f 1, f 2 ) b DEFINITION 11.1.

7.6 The Use of Definite Integrals in Physics and Engineering

ES.182A Topic 32 Notes Jeremy Orloff

Transcription:

Wve Phenomen Physics 15c Lecture 12 Multi-Dimensionl Wves

Gols For Tody Wves in 2- nd 3-dimensions Extend 1-D wve eqution into 2- nd 3-D Norml mode solutions come esily Plne wves Boundry conditions Rectngulr drum Chldni pltes Sound in rectngulr room

1-Dimensionl Wves We ve studied 1-D wves extensively Non-dispersive wve eqution is Norml modes re Dispersion reltion is t 2 ξ(x,t) = Ae i(kx±ωt ) ω = c w k 2 ξ(x,t) 2 2 ξ(x,t) = c w x 2 True even for dispersive wves Non-dispersive cse Try to extend nturlly to 2-D or 3-D It s esy

1-D to 2-D Let s extend from 1-D to 2-D Simplest wy is to ignore y We just declre tht ξ (x, y, t) is constnt in y Eqution nd solution remins the sme s 1-D 2 ξ(x,y,t) t 2 = c w 2 2 ξ(x,y,t) x 2 ξ(x,t) ξ(x,y,t) e.g. ξ(x,y,t) = ξ 0 e i(kx ωt ) This isn t the whole story We should be ble to send wves in y-direction too Move this wy

Isotropy We my define x-y coordintes s we find convenient Physics should not depend on prticulr direction Tht is, unless the medium hs preferred direction Non-directionl medi re clled isotropic Extend the 1-D wve eqution to mke it isotropic 2 ξ(x,y,t) t 2 2 2 ξ(x,y,t) = c w x 2 Extend the solution s well + 2 ξ(x,y,t) y 2 Substitute into the eqution nd we find the dispersion reltion: ξ(x,y,t) = ξ 0 e i(k x x+k y y ωt ) ω 2 = c w 2 (k x 2 + k y 2 ) Miniml extension

Wvenumber Vector We cn consider (k x, k y ) s 2-D vector Dispersion reltion determines the length of k k = (k x,k y ) Solution cn be written s ω 2 = c w 2 (k x 2 + k y 2 ) = c w 2 (k k) = c w 2 k 2 ξ(x,t) = ξ 0 e i(k x x+k y y ωt ) = ξ 0 e i(k x ωt ) Depends on the dot-product Points on line perpendiculr to k hve sme vlue of k x As t increses, this line moves k points the direction of wve propgtion k x y k x x

Norml Modes We now hve plne-wve solutions trveling in ll directions ξ k (x,t) = e i(k x ωt ) ω = ω(k) = c w k The direction is given by the wvenumber vector k Dispersion reltion determines the length of k For ech ω, there re infinite number of norml modes It s convenient to use k to specify norml mode There is one norml mode for every 2-D vector k Any rbitrry wves cn be expressed by liner combintion of these norml modes To show this, we need to expnd Fourier trnsform

Fourier Trnsform Any function f(x,y) cn be expressed s f (x,y) = Suppose t t = 0, the wve hd form f(x, y) Fourier integrl breks it into They trvel s + + So we know the complete solution F(k x,k y )e i(k x x+k y y ) dk x dk y where the Fourier trnsform F(k x,k y ) is given by 1 + + F(k x,k y ) = f (x,y)e i(kx x+ky y ) dx dy (2π) 2 ξ(x,y,t) = e i(k x x+k y y ωt ) + + e i(k x x+k y y ) F(k x,k y )e i(k x x+k y y ωt ) dk x dk y NB: ω depends on k

Rectngulr Membrne Imgine rectngulr drum Elstic film is stretched over rigid frme Consider smll piece Δx Δy Mss is m = ρδxδy It s pulled from 4 edges by tension L y T Δy T Δx T Δx T Δy Proportionl to the length of the edge L x Forces re blnced in the x-y plne Let s mke the film vibrte in z

Rectngulr Membrne Vibrtion mkes Viewed from the bottom edge, there is force in the z direction F z = T Δy z(x,y,t) +T Δy x T 2 z(x,y,t) ΔxΔy x 2 Sme with the other edges Totl force on this little piece is F z = T 2 z(x,y,t) x 2 z = z(x,y,t) z(x + Δx,y,t) x ΔxΔy +T 2 z(x,y,t) y 2 ΔxΔy T Δy x x + Δx x

Wve Eqution The eqution of motion is ρδxδy 2 z(x,y,t) t 2 = T 2 z(x,y,t) x 2 ΔxΔy +T 2 z(x,y,t) y 2 ΔxΔy 2 z(x,y,t) = T 2 z(x,y,t) t 2 ρ x 2 We lredy know the norml modes + 2 z(x,y,t) y 2 2-D wve eqution! z(x,y,t) = e i(k x ωt ) ω = c w k = T ρ k Remining problem: wht hppens t the edges? The film cn t move there z = 0

Stnding Wves Edge of the film is fixed z(0,y,t) = z(l x,y,t) = z(x,0,t) = z(x,l y,t) = 0 Similr to string with fixed ends ξ(0,t) = ξ(l,t) = 0 Solution ws stnding wves ξ(x,t) = sin nπ L x sin nπc w L Guess: 2-D stnding wves t z(x,y,t) = sin(k x x)sin(k y y)e iωt Let s see where this brings us

Stnding Wves To stisfy the boundry conditions To stisfy the dispersion reltion Frequencies don t come in nice integer rtios Drums don t hve cler pitch Bottom line: z(x,y,t) = sin(k x x)sin(k y y)e iωt sink x L x = 0 sink y L y = 0 k x L x = nπ k y L y = mπ ω = c w π n2 L x 2 + m2 L y 2 ω = c w k 1-D string hd L x ω = c w nπ L z(x,y,t) = sin nπ mπ x sin y e iωt L y

Stnding Wves z(x,y,t) = sin nπ x L x mπ sin y e iωt L y (n,m) = (1,1) Node lines split the film into n m rectngles (n,m) = (3,4) (n,m) = (1,2) (n,m) = (2,2) z = 0 on these lines

Stnding Wves vs. Norml Modes Stnding wves nd norml modes don t look relted z(x,y,t) = sin(k x x)sin(k y y)e iωt z(x,y,t) = e i(k x ωt ) They re in fct. Just not esy to see For 1-D wves, 2 norml modes They move in opposite directions hve sme ω Adding them gives stnding wves For 2-D wves, infinite norml modes hve sme ω They move in ll directions in the x-y plne Try dding 4 of them with mixed signs e i(kx±ωt ) e i(k x x+k y y ωt ) e i( k x x+k y y ωt ) e i(k x x k y y ωt ) + e i( k x x k y y ωt ) = 4 sin(k x x)sin(k y y)e iωt

Chldni Plte Ernst Chldni (1756-1827) Squre plte is held t the center Vibrtion of the plte = 2-D wves Don t worry bout the wve eqution Norml mode solution is s usul Boundry conditions re No force t the edge 1-D nlog is pipe with both ends open Guess the solution: k x = nπ k y = mπ Tht sounds esy enough z(x,y,t) = cos(k x x)cos(k y y)e iωt z(x,y,t) = cos nπ x mπ y cos e iωt

Chldni Plte z(x,y,t) = cos nπ x mπ y cos e iωt Extr condition: fixed in the middle It cn t move, nd cn t hve slope z center = cos nπ 2 z x center = nπ sin nπ 2 cos mπ 2 e iωt = 0 cos mπ 2 e iωt = 0 z = mπ y center cos nπ 2 Obvious solution is cos nπ 2 n nd m must be both odd sin mπ 2 e iωt = 0 = cos mπ 2 = 0

Chldni Plte z(x,y,t) = cos nπ x mπ y cos e iωt Think bout ngulr frequency ω Sme for n m If n m we hve two stnding-wve solutions with the sme frequency Liner combintion is lso stnding wves Suppose n nd m re both even Center is not node If we subtrct (m, n) from (n, m), we find cos nπ x mπ y cos mπ x cos This stisfies ll the conditions! nπ y cos ω = c w π Exmple: (2, 4) e iωt n 2 + m 2

Chldni Ptterns Both n nd m re even z center = z x center = z y center = cos nπ 2 cos mπ 2 nπ sin nπ 2 mπ cos nπ 2 (2, 4) (4, 2) cos mπ 2 cos nπ 2 e iωt = 0 mπ cos 2 + mπ mπ sin 2 cos nπ 2 sin mπ 2 + nπ cos mπ 2 sin nπ 2 e iωt = 0 e iωt = 0

Chldni Ptterns Mke liner combintions from (odd, odd) solutions Both sum nd difference stisfy the constrints (of course) (1, 3) (3, 1) sum 2 solutions for ech (odd, odd) pir 1 solution for ech (even, even) pir All of them hve 4-fold symmetry (= 90 rottion) diff.

3-D Plne Wves Esy to extend wve eqution to 3-D 2 ξ t = c 2 2 ξ 2 w x + 2 ξ 2 y + 2 ξ 2 z 2 = c 2 2 ξ = w x, y, z Norml mode is Dispersion reltion This sounds ll fmilir ξ = e i(k x x+k y y +k z z ωt ) = e i(k x ωt ) ω = c w k

Isotropy nd Reltivity Wve eqution nd the norml mode solutions for n isotropic medium contin only dot-products of vectors.k.. sclr products 2 ξ t 2 = c 2 ( )ξ w ξ = e i(k x ωt ) They re invrint under rottion of coordinte xes For EM wves in vcuum, is Lorentz sclr k x ωt = k x kct It s invrint under Lorentz trnsformtion Form of equtions re constrined by the symmetry of the physicl system

Stnding Wve in Box Imgine rectngulr room with rigid wlls Sound in this room mkes stnding wves ξ(x,y,z,t) = sin(k x x)sin(k y y)sin(k z z)e iωt Boundry conditions k x L x = n x π Dispersion reltion ω = c w π k y L y = n y π n 2 x 2 L x + n 2 y 2 L y + n 2 z 2 L z k z L z = n z π L z L x These frequencies resonte in the room L y Cn we express stnding wves using norml modes? Try it!

Concert Hll Acoustics Stnding wves in room is Bd Thing Only prticulr frequencies exist For ech frequency, there re node plnes You cn t her the frequency if you sit on node plne Rel wlls re not completely rigid Stone wlls (e.g. church) come close Sound bsorbers (soft stuff) my be ttched to the wlls Think of them s termintion resistors for sound Complete bsorption mkes the room sound ded You wnt some echo for musicl enjoyment Concert-hll coustics is combintion of rt nd science Look up Wllce Clement Sbine (1868 1919) nd his work on Fogg Lecture Hll

Royl Festivl Hll, London

1/20 th Acoustic Model http://www.coxt.freeserve.co.uk/

Summry Wves in 2- nd 3-dimensions Wve eqution nd norml modes esily extended 2 ξ t = c 2 2 ξ 2 w x + 2 ξ 2 y + 2 ξ 2 z 2 = c 2 2 ξ ξ = e i(k x x+k y y +k z z ωt ) = e i(k x ωt ) w Norml modes re plne wves Isotropy nd (for EM wves) Lorentz invrince Boundry conditions in 2-D nd 3-D Rectngulr drum, Chldni plte, sound in room Nturl extension of the 1-D problems such s string Next: sphericl wves, shock wves