Chapter 11. Maxwell's Equations in Special Relativity. 1

Similar documents
(a) We desribe physics as a sequence of events labelled by their space time coordinates: x µ = (x 0, x 1, x 2 x 3 ) = (c t, x) (12.

Examples of Tensors. February 3, 2013

ELECTRODYNAMICS: PHYS 30441

Vector Field Theory (E&M)

TENSOR FORM OF SPECIAL RELATIVITY

The Procedure of Finding the Stress-Energy. Tensor and Equations of Vector Field of Any Form

Particle-wave symmetry in Quantum Mechanics And Special Relativity Theory

Four-dimensional equation of motion for viscous compressible substance with regard to the acceleration field, pressure field and dissipation field

11.1 The Special Theory of Relativity

The homopolar generator: an analytical example

Volume Charge Density in Most General Lorentz Transformation

The Dirac Equation in a Gravitational Field

Chapter 26 Lecture Notes

Spinning Charged Bodies and the Linearized Kerr Metric. Abstract

Name Solutions to Test 1 September 23, 2016

Generation of EM waves

The Hamiltonian in Covariant Theory of Gravitation

Lagrangian Formulation of the Combined-Field Form of the Maxwell Equations

Dynamics of the Electromagnetic Fields

Relativistic Dynamics

ELECTROMAGNETIC WAVES WITH NONLINEAR DISPERSION LAW. P. М. Меdnis

Dirac s equation We construct relativistically covariant equation that takes into account also the spin. The kinetic energy operator is

The concept of the general force vector field

Electrodynamics in Uniformly Rotating Frames as Viewed from an Inertial Frame

Advanced Computational Fluid Dynamics AA215A Lecture 4

Green s function for the wave equation

1 sin 2 r = 1 n 2 sin 2 i

1 The beginnings of relativity

n n=1 (air) n 1 sin 2 r =

Hamiltonian with z as the Independent Variable

1 Summary of Electrostatics

Final Review. A Puzzle... Special Relativity. Direction of the Force. Moving at the Speed of Light

Hidden Momentum in a Spinning Sphere

Relativity in Classical Physics

The concept of the general force vector field

PHY 396 T: SUSY Solutions for problem set #12.

An Elucidation of the Symmetry of Length Contraction Predicted by the Special Theory of Relativity

QUANTUM MECHANICS II PHYS 517. Solutions to Problem Set # 1

arxiv: v1 [physics.gen-ph] 5 Jan 2018

Theory of Dynamic Gravitational. Electromagnetism

Virtual Work for Frames. Virtual Work for Frames. Virtual Work for Frames. Virtual Work for Frames. Virtual Work for Frames. Virtual Work for Frames

CHAPTER 26 The Special Theory of Relativity

[Khalid, 5(3): March 2018] ISSN DOI /zenodo Impact Factor

New Chapter 3 The Universal Constants

In this case it might be instructive to present all three components of the current density:

F = F x x + F y. y + F z

Physics 6C. Special Relativity. Prepared by Vince Zaccone For Campus Learning Assistance Services at UCSB

A EUCLIDEAN ALTERNATIVE TO MINKOWSKI SPACETIME DIAGRAM.

HOW TO FACTOR. Next you reason that if it factors, then the factorization will look something like,

The gravitational phenomena without the curved spacetime

The First Principle of Thermodynamics under Relativistic Conditions and Temperature

The Electromagnetic Radiation and Gravity

High Energy Astrophysics

Einstein s Three Mistakes in Special Relativity Revealed. Copyright Joseph A. Rybczyk

Classical Field Theory

An Effective Photon Momentum in a Dielectric Medium: A Relativistic Approach. Abstract

ELECTROMAGNETIC NORMAL MODES AND DISPERSION FORCES.

Properties of Quarks

Application of Bi-Quaternions in Physics

Chapter 35. Special Theory of Relativity (1905)

Modes are solutions, of Maxwell s equation applied to a specific device.

Simple Considerations on the Cosmological Redshift

Electromagnetic radiation

Classical Trajectories in Rindler Space and Restricted Structure of Phase Space with PT-Symmetric Hamiltonian. Abstract

Chapter Outline The Relativity of Time and Time Dilation The Relativistic Addition of Velocities Relativistic Energy and E= mc 2

Module 5: Red Recedes, Blue Approaches. UNC-TFA H.S. Astronomy Collaboration, Copyright 2012

arxiv:gr-qc/ v7 14 Dec 2003

Transverse momentum as a source of gravitoelectromagnetism

Electromagnetic Theory Prof. Ruiz, UNC Asheville, doctorphys on YouTube Chapter B Notes. Special Relativity. B1. The Rotation Matrix

Time Domain Method of Moments

Velocity Addition in Space/Time David Barwacz 4/23/

Lecture 15 (Nov. 1, 2017)

ECE507 - Plasma Physics and Applications

arxiv: v1 [physics.class-ph] 12 Mar 2012

CS420/ S-04 Intro to 3D Math 1

SURFACE WAVES OF NON-RAYLEIGH TYPE

International Journal of Thermodynamics, Vol. 18, No. 1, P (2015). Sergey G.

arxiv:physics/ v1 [physics.class-ph] 8 Aug 2003

GUIDELINES FOR A SPACE PROPULSION DEVICE BASED ON HEIM'S QUANTUM THEORY

Institut für Grenzgebiete der Wissenschaft (IGW), Leopold - Franzens Universität Innsbruck, Innsbruck, Austria

The Unified Geometrical Theory of Fields and Particles

8.022 (E&M) Lecture 11

Green s function for the wave equation

Aharonov-Bohm effect. Dan Solomon.

Fig 1: Variables in constant (1+1)D acceleration. speed of time. p-velocity & c-time. velocities (e.g. v/c) & times (e.g.

Towards an Absolute Cosmic Distance Gauge by using Redshift Spectra from Light Fatigue.

Motion through a velocity selector analyzed using a galilean transformation

Q2. [40 points] Bishop-Hill Model: Calculation of Taylor Factors for Multiple Slip

The Special Theory of Relativity

). In accordance with the Lorentz transformations for the space-time coordinates of the same event, the space coordinates become

We wrote down the Boltzmann equation for photons last time; it is:

Lecture 3 - Lorentz Transformations

Vector Analysis in Three Dimensions

The Hanging Chain. John McCuan. January 19, 2006

Intro to Nuclear and Particle Physics (5110)

4. (12) Write out an equation for Poynting s theorem in differential form. Explain in words what each term means physically.

arxiv:physics/ v4 [physics.gen-ph] 9 Oct 2006

Let s move to Bound States

INTRODUCTION TO QUANTUM MECHANICS

Physics 523, General Relativity Homework 4 Due Wednesday, 25 th October 2006

Transcription:

Vetor Spaes in Phsis 8/6/15 Chapter 11. Mawell's Equations in Speial Relativit. 1 In Chapter 6a we saw that the eletromagneti fields E and B an be onsidered as omponents of a spae-time four-tensor. This tensor, the Mawell field tensor F, transforms under relativisti "boosts" with the same oordinate-transformation matri used to arr out the Lorent transformation on the spae-time vetor. Sine then we have introdued vetor differential alulus, entered around the gradient operator. This operator, operating on the fields E and B and the potentials and A, an be used to epress the four Mawell equations, giving a omplete theor of the eletromagneti field. In this hapter we will start to put these equations into "ovariant form," epressed in terms equall valid in an Lorent frame. In Chapter 6a we introdued the position four-vetor, t the eletromagneti-field four-tensor, 1 1 1 E E E 1 E B B F, 1 E B B 1 E B B and the Lorent transformation matri, 1 1 whih is used in the "usual tensor wa" to transform vetor and tensor indies from one rest frame to another. Contration of indies must alwas be between a upper and a lower inde, with the metri tensor One ma note fators of 1/ whih were not present in the form of the field-strength tensor introdued in Chapter 6a. This is a pesk issue of unit sstems. The form given here gives the orret onstants in the SI sstem of units. 11-1

Vetor Spaes in Phsis 8/6/15 1 1 g g 1 1 used to raise or lower indies. Upper indies are referred to as "ontravariant" indies, and lower indies, as "ovariant" indies, referring to details of tensor analsis whih we hope to avoid disussing here. More Four-Vetors Let's just see some other ombinations of a salar and a three-vetor whih form fourvetors. E p four-momentum p, p E p p p p p four-urrent, A four-potential: A, A A A A A A 1 t 1 four-gradient:, t Note the ool salar invariants formed b ontrating ertain of these vetors with themselves. 11 -

Vetor Spaes in Phsis 8/6/15 t p p E p m 4 1 t The proper-time interval, invariant under Lorent trans. A partile's invariant mass-squared. The wave-equation operator, or the d'alembertian. Here we are interested in seeing what important relations of eletromagnetism an be epressed simpl in ovariant language. Here is an interesting ontration to form a foursalar: Conservation of harge. t Remember? Positive divergene of requires a derease in the harge densit. Now let's show where Mawell's equations ome from. Sine the divergene of the eletri field equals the harge, probabl the divergene of the field-strength tensor equals the four-vetor ombination of harge and urrent. 1 1 1 E E E 1 E B B F t 1 E B B 1 E B B E E E t E B B This gives a stak of four equations, t E B B t E B B t 11-3

Vetor Spaes in Phsis 8/6/15 1 E E B B t E B B t E B B t Or, in old Earth-bound three-vetor notation, E E B t Here we have the two most ompliated of Mawell's equations, the soure equation. And ou might notie that the famous "displaement-urrent" term, invented b Mawell to make the wave-equation work, has appeared as b magi: E displaement t. Well, that is about as muh eitement as most people an bear. But if ou are good for more - - - nobod reall likes the url. Let's set the four-url of the field-strength tensor equal to ero. This will of ourse involve the four-dimensional version of the Levi-Civita totall anti-smmetri tensor, 1, an even permutation of 13 1, an odd permutation of 13 otherwise Then F The top line gives and the net three lines give B B B 1 3 3 E E B 3 1 E B E 1 B E E B 11-4

Vetor Spaes in Phsis 8/6/15 B E t These omplete Mawell's equations. Good enough for one da. 1 http://www.ph.duke.edu/~rgb/class/ph319/ph319/node135.html 11-5