Waveguides and resonant cavities

Similar documents
Waveguides and resonant cavities

ELASTIC WAVE PROPAGATION IN A CONTINUOUS MEDIUM

Section 8.3 Polar Form of Complex Numbers

Lectures - Week 4 Matrix norms, Conditioning, Vector Spaces, Linear Independence, Spanning sets and Basis, Null space and Range of a Matrix

16 Reflection and transmission, TE mode

CONDUCTORS AND INSULATORS

Frequency dependence of the permittivity

The Feynman path integral

8.022 (E&M) Lecture 4

Week3, Chapter 4. Position and Displacement. Motion in Two Dimensions. Instantaneous Velocity. Average Velocity

Advanced Circuits Topics - Part 1 by Dr. Colton (Fall 2017)

The equation of motion of a dynamical system is given by a set of differential equations. That is (1)

PHYS 705: Classical Mechanics. Newtonian Mechanics

PHYS 1101 Practice problem set 12, Chapter 32: 21, 22, 24, 57, 61, 83 Chapter 33: 7, 12, 32, 38, 44, 49, 76

1 Matrix representations of canonical matrices

Difference Equations

Implicit Integration Henyey Method

PHY2049 Exam 2 solutions Fall 2016 Solution:

The Geometry of Logit and Probit

APPENDIX A Some Linear Algebra

Physics 443, Solutions to PS 7

Canonical transformations

ECE 107: Electromagnetism

PES 1120 Spring 2014, Spendier Lecture 6/Page 1

Lecture 6/7 (February 10/12, 2014) DIRAC EQUATION. The non-relativistic Schrödinger equation was obtained by noting that the Hamiltonian 2

Lecture 12: Discrete Laplacian

n α j x j = 0 j=1 has a nontrivial solution. Here A is the n k matrix whose jth column is the vector for all t j=0

Δ x. u(x,t) Fig. Schematic view of elastic bar undergoing axial motions

Module 3 LOSSY IMAGE COMPRESSION SYSTEMS. Version 2 ECE IIT, Kharagpur

Boundaries, Near-field Optics

THE CHINESE REMAINDER THEOREM. We should thank the Chinese for their wonderful remainder theorem. Glenn Stevens

3.1 Expectation of Functions of Several Random Variables. )' be a k-dimensional discrete or continuous random vector, with joint PMF p (, E X E X1 E X

Salmon: Lectures on partial differential equations. Consider the general linear, second-order PDE in the form. ,x 2

THEOREMS OF QUANTUM MECHANICS

Field and Wave Electromagnetic. Chapter.4

PHYS 705: Classical Mechanics. Calculus of Variations II

Affine transformations and convexity

First day August 1, Problems and Solutions

Classical Mechanics Virtual Work & d Alembert s Principle

Chapter 5. Solution of System of Linear Equations. Module No. 6. Solution of Inconsistent and Ill Conditioned Systems

14 Lagrange Multipliers

V. Electrostatics. Lecture 25: Diffuse double layer structure

Physics 114 Exam 3 Spring Name:

Homework 4. 1 Electromagnetic surface waves (55 pts.) Nano Optics, Fall Semester 2015 Photonics Laboratory, ETH Zürich

Δ x. u(x,t) Fig. Schematic view of elastic bar undergoing axial motions

Rate of Absorption and Stimulated Emission

Robert Eisberg Second edition CH 09 Multielectron atoms ground states and x-ray excitations

CHAPTER 13. Exercises. E13.1 The emitter current is given by the Shockley equation:

Chapter 4 The Wave Equation

More metrics on cartesian products

Lecture Note 3. Eshelby s Inclusion II

princeton univ. F 17 cos 521: Advanced Algorithm Design Lecture 7: LP Duality Lecturer: Matt Weinberg

3 Basic boundary value problems for analytic function in the upper half plane

Chapter Newton s Method

The optimal delay of the second test is therefore approximately 210 hours earlier than =2.

The KMO Method for Solving Non-homogenous, m th Order Differential Equations

A particle in a state of uniform motion remain in that state of motion unless acted upon by external force.

College of Computer & Information Science Fall 2009 Northeastern University 20 October 2009

CHAPTER 14 GENERAL PERTURBATION THEORY

DECOUPLING THEORY HW2

12. The Hamilton-Jacobi Equation Michael Fowler

Electricity and Magnetism - Physics 121 Lecture 10 - Sources of Magnetic Fields (Currents) Y&F Chapter 28, Sec. 1-7

Note: Please use the actual date you accessed this material in your citation.

763622S ADVANCED QUANTUM MECHANICS Solution Set 1 Spring c n a n. c n 2 = 1.

Inner Product. Euclidean Space. Orthonormal Basis. Orthogonal

8.6 The Complex Number System

ON A DETERMINATION OF THE INITIAL FUNCTIONS FROM THE OBSERVED VALUES OF THE BOUNDARY FUNCTIONS FOR THE SECOND-ORDER HYPERBOLIC EQUATION

2.3 Nilpotent endomorphisms

Supplement: Proofs and Technical Details for The Solution Path of the Generalized Lasso

20. Mon, Oct. 13 What we have done so far corresponds roughly to Chapters 2 & 3 of Lee. Now we turn to Chapter 4. The first idea is connectedness.

Problem 1: To prove that under the assumptions at hand, the group velocity of an EM wave is less than c, I am going to show that

ACTM State Calculus Competition Saturday April 30, 2011

CHAPTER II THEORETICAL BACKGROUND

Georgia Tech PHYS 6124 Mathematical Methods of Physics I

Foundations of Arithmetic

Physics 5153 Classical Mechanics. D Alembert s Principle and The Lagrangian-1

Open Systems: Chemical Potential and Partial Molar Quantities Chemical Potential

Section 3.6 Complex Zeros

A how to guide to second quantization method.

Modelli Clamfim Equazione del Calore Lezione ottobre 2014

Uniqueness of Weak Solutions to the 3D Ginzburg- Landau Model for Superconductivity

(2mn, m 2 n 2, m 2 + n 2 )

MMA and GCMMA two methods for nonlinear optimization

Formulas for the Determinant

ˆ (0.10 m) E ( N m /C ) 36 ˆj ( j C m)

Lecture 13 APPROXIMATION OF SECOMD ORDER DERIVATIVES

Please review the following statement: I certify that I have not given unauthorized aid nor have I received aid in the completion of this exam.

Problem Set 9 Solutions

Linear, affine, and convex sets and hulls In the sequel, unless otherwise specified, X will denote a real vector space.

Complete subgraphs in multipartite graphs

MAGNETISM MAGNETIC DIPOLES

Fundamental loop-current method using virtual voltage sources technique for special cases

Maximizing the number of nonnegative subsets

Asymptotics of the Solution of a Boundary Value. Problem for One-Characteristic Differential. Equation Degenerating into a Parabolic Equation

Dynamic Programming. Preview. Dynamic Programming. Dynamic Programming. Dynamic Programming (Example: Fibonacci Sequence)

MAE140 - Linear Circuits - Winter 16 Final, March 16, 2016

Introduction to Antennas & Arrays

Random Walks on Digraphs

Physics 4B. A positive value is obtained, so the current is counterclockwise around the circuit.

find (x): given element x, return the canonical element of the set containing x;

Transcription:

Wavegudes and resonant cavtes February 8, 014 Essentally, a wavegude s a conductng tube of unform cross-secton and a cavty s a wavegude wth end caps. The dmensons of the gude or cavty are chosen to transmt, hold or amplfy partcular forms of electromagnetc wave. We wll consder the case of a hollow tube extended n the z drecton, wth arbtrary but constant crosssectonal shape n the xy-plane. We consder possble wave solutons matchng these boundary condtons. 1 Wave equatons As we have shown, the Maxwell equatons, gve rse to wave equatons, B E + B t D H D t E B We assume that the electrc and magnetc felds have spatal and tme dependence of the form E E x, y e ±kz ωt B B x, y e ±kz ωt for waves travelng n the ±z drecton. Unlke our plane wave solutons, however, the felds must satsfy boundary condtons n the x and y drectons, along the sdes of the wavegude. Separatng the del operator nto longtudnal z and transverse parts, the d Alembertan becomes t + ˆk, µɛ t + µɛ t + t + Substtutng the assumed tme and z-dependence nto the wave equatons gves 0 t µɛ t + E t µɛ ω + k E 1

and, wth the correspondng result for B, 0 t + µɛω k E 0 t + µɛω k B General soluton: Separatng transverse and longtudnal components We can smplfy the problem by separatng the transverse, E t, and longtudnal, ˆkE z, parts, then treatng E z and B z as sources for the transverse parts. We can use the z-component of wave equaton together wth the boundary condtons to solve for the sources, E z, B z. Defnng t + ˆk E E t + ˆkE z ˆk E ˆk and smlarly for B, the source-free Maxwell equatons become t B t ± kb z t E t ± ke z t + ˆk E t + ˆkE z ω B t + ˆkB z t + ˆk B t + ˆkB z + ɛµω E t + ˆkE z The frst two equatons have the form we are after, t B t kb z t ke z and we turn out attenton to the curl equatons. The curl terms expand as t + ˆk E t + ˆkE z t E t + t ˆkE z + ˆk E t + ˆk ˆk E z t E t + î ˆk E z x + ĵ ˆk E z y + ˆk E t t E t ĵ E z x + î E z y + ˆk E t and smlarly for the magnetc terms. Thus t E t ĵ E z x + î E z y ± ˆk ke t ω B t + ˆkB z t B t ĵ B z x + î B z y ± ˆk kb t + εµω E t + ˆkE z

Notng that t E t les n the z-drecton, we separate the transverse and longtudnal parts of each equaton, ĵ E z x + î E z y ± ˆk ke t ωb t t E t ωb zˆk ĵ B z x + î B z y ± ˆk kb t + ɛµω 0 t B t + ɛµωe zˆk We can stll smplfy the frst and thrd. Snce they are transverse, we lose no nformaton by takng the cross product wth ˆk. For the frst ths becomes 0 ˆk ĵ E z x + î E z y ± ˆk ke t ωb t î E z x + ĵ E z y ± ˆk ˆk ke t ωˆk B t and smlarly for the thrd. t E z ± ke t ωˆk B t 0 t E z ± ke t + ωˆk B t 3 General soluton: Separatng E t and B t In the resultng par of equatons, ±ke t + ωˆk B t t E z ±kb t ɛµωˆk t B z the transverse E t and B t are stll coupled. To separate them, solve the second for B t, and substtute nto the frst, B t ± 1 t B z + ɛµωˆk E t k ±ke t + ωˆk B t t E z ±ke t + ωˆk ± 1 t B z + ɛµωˆk t E z k ±ke t ± ω k ˆk t B z + ɛµωˆk t E z ±ke t ± ɛµ ω k ˆk ˆk Et t E z ω k ˆk t B z ± k ɛµ ω t E z ω k k ˆk t B z ± k ɛµω t E z ω k k ˆk t B z and therefore, ɛµω k ±k t E z ωˆk t B z 3

Substtutng ths back nto the expresson for B t, B t ± 1 t B z + ɛµωˆk E t k ± 1 ɛµω t B z k ɛµω k ˆk ±k t E z ωˆk t B z ± 1 ɛµω t B z k ɛµω k ±kˆk t E z + ω t B z 1 ɛµω k ɛµω k kˆk ɛµω t E z ɛµω k ω tb z ± t B z ɛµω ɛµω k ɛµω k kˆk t E z ± ɛµω k ω 1 t B z ɛµω k ɛµωˆk t E z ± k t B z and we have solved for the transverse felds n terms of the longtudnal ones: B t ɛµω k ±k t E z ωˆk t B z ɛµω k ɛµωˆk t E z ± k t B z To have a complete soluton, we must check the remanng Maxwell equatons, The dvergence equatons become t Usng the reduced form of the wave equaton, t B t kb z t ke z t ωb zˆk t B t ɛµωe zˆk ɛµω k ±k t t E z ω t ˆk t B z 0 t + µɛω k E together wth t ˆk t B z t ε 3k t B z,k t 1 t B z t t 1B z the rght sde smplfes, t ±k k ɛµω k µɛω E z ke z as requred. 4

For the curl, t ɛµω k t ±k t E z ωˆk t B z ω ɛµω k t ˆk t B z Sortng out the double curl, [ ] t ˆk t B z t ˆk t B z ] ε jk t j [ˆk t B z k j,k ε jk t j εk3m t mb z j,k,m ε jk ε 3mk t j t mb z j,k,m δ 3 δ jm δ m δ j3 t j t mb z j,m δ 3 t j t jb z t 3 t B z j ˆk t B z The second term vanshes because t has no z component. Therefore, usng the wave equaton agan, t ω ɛµω k ˆk t B z ω ɛµω k ˆk k µɛω B z ωb zˆk The correspondng dvergence and curl of B t are left as exercses for the reader. 4 Characterstcs of solutons Our general method of soluton s now to solve 0 t + µɛω k E z 0 t + µɛω k B z wth the approprate boundary condtons, then use these solutons to solve B t ɛµω k ±k t E z ωˆk t B z ɛµω k ɛµωˆk t E z ± k t B z for the transverse parts. We consder three specal cases, dependng on one or both of E z and B z vanshng: 1. If both E z and B z vansh, then both the electrc and magnetc felds are purely transverse. These solutons are called TEM waves Transverse Electrc and Magnetc. 5

. If E z vanshes, then the electrc feld s purely transverse. These solutons are called TE waves Transverse Electrc. 3. If B z vanshes, then the magnetc feld s purely transverse. These solutons are called TM waves Transverse Magnetc. Generc waves are a combnaton of all three. Ths method sketched above works for TE and TM waves see below, but n the case where E z B z we have ɛµω k and ths soluton fals. We treat ths specal TEM case frst, then use the technque to dscusss TE and TM waves. 4.1 Transverse electromagnetc waves: TEM Transverse electromagnetc waves n a wavegude are those wth no z-component to the felds, E z B z In ths case, our orgnal equatons have zero source, t B T EM t E T EM t E T EM t B T EM so that the transverse electrc and magnetc felds satsfy the Laplace equaton of electrostatcs n - dmensons. Ths means that our general soluton above cannot be used because µɛω k. Instead, the relevant soluton to the -dmensonal Laplace equaton s determned purely by ts boundary condtons. Snce a closed conductor allows no feld nsde, TEM waves cannot exst nsde a completely enclosed, perfectly conductng cavty. We also have Combnng these last two equatons, ±ke T EM + ωˆk B T EM ±kb T EM ɛµωˆk E T EM k E T EM + ɛµω ˆk ˆk ET EM k ɛµω E T EM we see that we must have and the magnetc feld satsfes k k 0 ɛµω B T EM ± ɛµˆk E T EM TEM waves are the domnant mode n a coaxal cable: nner and outer cylndrcal conductors held at opposte potental lead to a radal electrc feld, whle opposte currents on the conductors lead to an azmuthal magnetc feld. These are transverse to the drecton along the cable, so waves propagate along the cable between the conductors. 6

4. Transverse electrc, TE, modes and transverse magnetc, TM, modes 4..1 Boundary condtons Modes drven by nonzero E z and/or B z fall nto two categores. To see why, consder a perfectly conductng boundary. For a perfectly conductng wavegude, we fnd the boundary condtons usng the assumpton that free charges move nstantly to produce whatever surface charge densty, Σ, and surface current densty, K, are requred to make the electrc and magnetc felds vansh nsde the conductor. The full boundary condtons are therefore n D Σ n H K n E n B There can therefore be no tangental component of the electrc feld at the surface, and no normal component of the magnetc feld. For the longtudnal electrc feld, the boundary condton s n ˆk E z so that E z at the boundary. For the boundary condton on B z we start wth our separaton of the Maxwell equatons nto longtudnal and transverse components, where we found kb t ɛµωˆk t B z Consder the normal component of ths equaton, kn B t ɛµωn ˆk Et n t B z k n B t ɛµωˆk E t n B z n The left sde of ths equaton vanshes by the boundary condtons, so we must have B z n at the surface as well. Therefore, we seek solutons to the -dmensonal wave equatons wth boundary condtons 0 t + µɛω k E z 0 t + µɛω k B z E z S B z n S Snce each of these components also satsfes the orgnal wave equaton, 0 t + µɛω k E z 0 t + µɛω k B z 7

we have well-defned egenvalue problems for E z and B z. Snce the transverse drecton s a bounded regon, we expect a dscrete set of egenvalues. Because the boundary condtons are dfferent but the equatons the same, unqueness guarantees that the spectrum of allowed values wll be dfferent for E z and B z. Ths means that at a gven resonant frequency, n general only one or the other source feld wll be excted. Ths dvdes the solutons nto two types, 1. TE waves: The electrc feld s transverse,.e., E z everywhere whle B z satsfes the boundary condton Bz n S.. TM waves: The magnetc feld s transverse so that B z everywhere whle E z satsfes the boundary condton E z S. A general soluton for the feld n a wavegude or cavty s a superposton of TE, TM and TEM waves. 4.. The transverse felds Frst, we smplfy our solutons for transverse felds n the TE and TM cases. For TM waves, we set B z. Then B t Takng the curl of the transverse electrc feld, so that ˆk For TE waves, E z we get a smlar result, B t so substtutng the second equaton nto the frst, so takng the cross product wth ˆk, ±k ɛµω k te z ɛµω ˆk t ɛµω k E z ±k ɛµω k ˆk t E z ± k ɛµω B t ± k ɛω H t H t ± ɛω k ˆk E t ω ˆk ɛµω k t B z ±k ɛµω k tb z ω ˆk ɛµω k t B z ω ˆk ɛµω k ɛµω k B t ±k ω ±k ˆk B t ˆk ω k ˆk ˆk B t ± ω k B t 8

so that H t ± k µω ˆk E t Both of these relatonshps, for TM and TE waves, have the form where, usng k 0 εµω, Z { k The quantty Z s called the wave mpedence. Ths gves solutons of the form: H t ± 1 Z ˆk E t ɛω k µ k 0 ɛ T M modes µω k k0 µ k ɛ T E modes k ± ɛµω k te z H t ± 1 Z ˆk E t wth Z k k 0 µ ɛ for TM and ω ˆk ɛµω k t B z H t ± 1 Z ˆk E t wth Z k0 k µ ɛ for TE. 4..3 The egenvalue problem We want to fnd solutons for TE and TM modes. These wll dffer from the TEM mode due to the presence of ether nonzero E z or nonzero B z, whch provde the source for the transverse felds. Denote ether of these source felds by ψ, { Ez T M modes ψ T E modes and defne B z γ µɛω k Then the reduced wave equaton for ψ becomes an egenvalue problem, wth boundary condtons t ψ γ ψ ψ S T M ψ n T E S Snce these boundary condtons are perodc, the wave equaton wll have a dscrete spectrum of allowed values for the constant, γ γ λ. These correspond to dscrete values of the wavelength, or equvalently, wave number k, gven by k λ µεω γ λ 9

The Laplacan wll have wave modes rather than exponental modes only for γ > 0. Ths leads to a cutoff frequency, ω λ, Expressng k λ n terms of frequency, we have µɛω > γλ ω ω λ γ λ µɛ k λ µɛω γλ µɛ ω γ λ µε µɛ ω ωλ so the wave vector becomes magnary, leadng to attenuaton, for frequences lower than ω λ. Now consder a fxed frequency, as we allow ω λ to range over the possble egenvalues. There s some maxmum allowed cutoff frequency, correspondng to some mnmum value of k λ and therefore some maxmum wavelength that can propagate at that frequency. As a result, only a fnte number of possble wavelengths can propagate. It s possble to choose the dmensons of the wavegude so that at the desred frequency or frequency range, only a sngle wavelength can propagate. Once we have solved for ψ, we can fnd the transverse felds from the expressons above. 4.3 Example: TE modes n a rectangular wavegude Suppose we have TE modes n a rectangular wavegude. Let the cross-secton of the gude run from x to x a, and from y to y b. Then, wth γ H z,we solve wth boundary condton 0 t + γ ψ x + y + γ ψ ψ n T E S The boundary condton n each drecton may be satsfed at the orgn by a cosne, so we have ψ H 0 cos αx cos βy and fttng the boundary condtons at x a and at y b requres α mπ a egenfunctons are ψ mn H 0 cos mπx nπy cos a b wth egenvalues The cutoff frequency follows from γ mn π m a + n b and β nπ b. Therefore, the ω mn γ mn µε π m 1/ µε a + n b 10

for the varous modes. If we want to desgn a wavegude wth only one allowed mode, we want the lowest values for m, n. If a > b, the smallest value of ω mn occurs for n and m 1, For ths mode, we have the felds, ω 10 and therefore, for waves movng n the +z drecton, π a µɛ H z ψ 10 H 0 cos πx a B t + k γ tb z ka µ π t H 0 cos πx a kaµ π H 0 sn πx a e kz ωt From the mpedence equaton, so crossng wth ˆk H t + k µω ˆk E t µω k ˆk H t µω ka k π H 0 sn πx e kz ωt ĵ a ωaµ π H 0 sn πx a ekz ωt ĵ 11