ELECTRODYNAMICS: PHYS 30441
|
|
- Maximilian Lang
- 5 years ago
- Views:
Transcription
1 . Relativisti Eletromagnetism. Eletromagneti Field Tensor How do E and B fields transform under a LT? They annot be 4-vetors, but what are they? We again re-write the fields in terms of the salar and vetor potentials, A E and B= A = φ. The six equations are written in terms of = and A. t x Firstly, the E-field is given by: Ei A A A A = = = = x x i i φ = ; sine A,A and x i ( x, x ), x ( x, x i E A A i i = = i The B-field is obtained F i ) A A A A B = = = F Similarly, B A A A A = = = F and A A A A B = = = F Collating terms we have: E / E / E / A A E/ B B F = = A A = = F x E / B B E / B B E i and B i are the six elements of the antisymmetri 4x4 matrix F. This matrix is referred to as the eletromagneti field tensor. As it transforms a tensor of rank under a LT: A A F =ΛΛ F, with F = = A A Exerises:. Show that F is a rank Lorentz tensor.. Show that Maxwells nd (M) and rd (M) equations may be expressed as: λ λ λ F + F + F =, and Maxwells st (M) and 4th (M4) by: F = ρ (M).E = ε (M).B = (M) xe = B t (M4) xh = J +ε E t J Eletrodynamis PHYS 44, Relativisti Eletromagnetism Part, R.M. Jones, University of Manhester --
2 In Q we onsider F : A A F = A A = in frame O. Also we know that ontravariant vetors transform as: Firstly we know, A =Λ A and A =Λ A Hene: F A A A A x = =Λ Λ Also, as x =Λ x and we also found earlier x = ( Λ ) x x = Λ x. Thus it is lear that = Λ and = Λ F A A A A =ΛΛ ΛΛ =ΛΛ =ΛΛF x x Thus, F is a Lorentz rank tensor.. In Q. taking F λ + λ F + F λ = with =, =, λ = : B E E B F + F + F = + = + E t, N.b. =, and =,. t t t z with =, =, λ = : x = ( t,x,x,x ) = ( t,r ) B E E B and x = ( t, x, x, x) = ( t, r) F + F + F = + = + E = t, t with =, =, λ = : B E E B F + F + F = E t + = + = x x t x B Collating all three omponents gives Faraday s law or (M): E = t Now for =, =, λ = : B B B F + F + F = = This we reognize as B= or (M). y. Eletrodynamis PHYS 44, Relativisti Eletromagnetism Part, R.M. Jones, University of Manhester --
3 In the seond part of Q F = J stands for 4 equations one for eah value of. For example, for = the first equation reads: F F F F F = E E E = J + + = = ρ E E E ρ ρ + + = ρ = = or E ε ε -.ie. Gauss s law or (M). For = we obtain: F F F F F = E B B E + = + = = x z y B J J x t y z t x gives Ampere s law or (M4): E B= J+ t making a similar expansion for =, Eletrodynamis PHYS 44, Relativisti Eletromagnetism Part, R.M. Jones, University of Manhester --
4 . Lorentz Transform of E and B Fields: Consider the speifi LT orresponding to a boost along the x = x axis. In this ase F transforms as: F =Λ Λ F or in matrix form F = ΛFΛ Thus, evaluating these equations expliitly will give the requisite transformation of E and B fields: F γ γ E / E / E / γ γ E/ B B γ γ γ γ E / B B E / B B = γe γe E E γe γe B B γe γb γ E+γB B γ E +γ B E B B γ γ E γ E B γ E +B E γ B E γ B + E F = γ E B γ B E B γ E + B γ B + E B Also: F E / E / E / = E/ B B E / B B E / B B Eletrodynamis PHYS 44, Relativisti Eletromagnetism Part, R.M. Jones, University of Manhester -4-
5 Thus omparing terms: E = E B = B E =γ( E B ) B =γ B + E E =γ ( E+ B ) B =γb E E =γ E+ γ E x+γ B z B y ( ) ˆ ( ˆ ) ˆ ( ) ( v.e ) v vxb γ v ( γ) ( ) E =γ E+ v.e v+γvxb v ( γ) B B ( v.b ) γ =γ + v vxe v Eletrodynamis PHYS 44, Relativisti Eletromagnetism Part, R.M. Jones, University of Manhester -5-
6 Lienard-Wiehert Eletri Field From A Diret Lorentz Transform We investigate a harge q, initially at rest in the moving frame O. We seek the fields in frame O. Eletri field from a harge q in uniform motion along ˆx. At t = t = both the stationary frame O and the moving frame O overlap. Within O the eletri field follows from Coulombs law: q E = r and B=. 4πε r Also, at time t = from the perspetive of O the fields are given by: E = E B = B = E = E =γ( ) =γ + = =γ E E B B B E E E E = γe E =γ ( E + B ) B =γb E= Thus, Charge q situated at the origin of the moving frame. Initially, at t= both frames oinide. q E = E, γe, γ E = x, γy, γz, and using x= γ x-ut = γx, at t= and y=y, z=z t ( ) ( ) ( ) 4πε r q qγ = γ ( x,y,z) = r. 4πε r 4πε r Note, the eletri field lines point to the present position. Finally, let us write the position vetor in O in terms of variables in O: r = x + y + z =γ x + y + z =γ θ+ θ=γ θ+ θ r os r sin r [os ( )sin ] =γ θ r[ sin ]. γ Eletrodynamis PHYS 44, Relativisti Eletromagnetism Part, R.M. Jones, University of Manhester -6-
7 Collating all terms we obtain: qγr E = = 4 πε γ r sin θ 4 πε r sin θ ( ) q ( ) r ( ) / / This is of ourse no more than the Lienard-Wiehert formula for the E-field of a uniformly moving point harge! We note that the field lines emanate from the present position of the harge and not the retarded position. For a partile at rest the field is isotropi. However, for relativisti veloities along the diretion of motion (θ =, π) the field is redued by a fator of γ - relative to the isotropi ase. Transverse to the diretion of motion (θ = π/) the field is enhaned by a fator of γ. This ompression of the lines of fore in the transverse diretion an be viewed as a onsequene of the FitzGerald- Lorentz ontration. E-field of a harge at rest (γ = ) E-field of a harge in uniform motion (γ = ) Eletrodynamis PHYS 44, Relativisti Eletromagnetism Part, R.M. Jones, University of Manhester -7-
8 Minkowski Fore and Lorentz Fore Covariane How does this relate to the Lorentz fore? We seek a ovariant representation. E dt Reall: U = ( U, U) = ( γ, γ ), p =, pand =γ N.b. Here, E is the partile energy. The Lorentz Fore: = q ( E + v B ), N.b. Here, E is the eletri field. We will adhere to this representation. dt in terms of the momentum 4-vetor beomes the Minkowski fore: = qγ E+ B = q γ E+γ B = U E+ U B q ( ) ( ) ( ) The spatial part of is The time omponent is the rate of hange of energy: =qu.e If the fore and energy hange equations are Lorentz ovariant, the right hand side of the rate of hange of 4-momentum equation must also form the omponents of a 4-vetor They involve harge (learly invariant from frame to frame), 4-veloity and e.m. fields. Eletrodynamis PHYS 44, Relativisti Eletromagnetism Part, R.M. Jones, University of Manhester -8-
9 Let us propose the following ovariant representation: du = m = qf U Writing this out in matrix form, eah omponent is readily identified. E / E / E / γ E/ B B γv γ γ = q E / B B v E / B B v Thus, the zero omponent: E E E q = qγ v + v + v = γe.v And as p denotes the energy of the partile, this learly represents a statement that the rate of hange of energy (or power) is equal to the fore multiplied by partile veloity. We now turn our attention to the spatial omponents. The first omponent (x) is: E = qγ + Bγv Bγv ( ) = qγ E + v B B v Dividing both sides by γ, and with = dt/γ, we reognise this as the first omponent (x) of the Lorentz fore equation. Similarly, for the other omponents (as an exerise, prove the remaining omponents yourself!). Eletrodynamis PHYS 44, Relativisti Eletromagnetism Part, R.M. Jones, University of Manhester -9-
Generation of EM waves
Generation of EM waves Susan Lea Spring 015 1 The Green s funtion In Lorentz gauge, we obtained the wave equation: A 4π J 1 The orresponding Green s funtion for the problem satisfies the simpler differential
More informationTENSOR FORM OF SPECIAL RELATIVITY
TENSOR FORM OF SPECIAL RELATIVITY We begin by realling that the fundamental priniple of Speial Relativity is that all physial laws must look the same to all inertial observers. This is easiest done by
More informationExamples of Tensors. February 3, 2013
Examples of Tensors February 3, 2013 We will develop a number of tensors as we progress, but there are a few that we an desribe immediately. We look at two ases: (1) the spaetime tensor desription of eletromagnetism,
More informationChapter 11. Maxwell's Equations in Special Relativity. 1
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
More informationGreen s function for the wave equation
Green s funtion for the wave equation Non-relativisti ase January 2019 1 The wave equations In the Lorentz Gauge, the wave equations for the potentials are (Notes 1 eqns 43 and 44): 1 2 A 2 2 2 A = µ 0
More information(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.
2 Relativity Postulates (a) All inertial observers have the same equations of motion and the same physial laws. Relativity explains how to translate the measurements and events aording to one inertial
More informationGreen s function for the wave equation
Green s funtion for the wave equation Non relativisti ase 1 The wave equations In the Lorentz Gauge, the wave equations for the potentials in Lorentz Gauge Gaussian units are: r 2 A 1 2 A 2 t = 4π 2 j
More informationVelocity Addition in Space/Time David Barwacz 4/23/
Veloity Addition in Spae/Time 003 David arwaz 4/3/003 daveb@triton.net http://members.triton.net/daveb Abstrat Using the spae/time geometry developed in the previous paper ( Non-orthogonal Spae- Time geometry,
More informationThe homopolar generator: an analytical example
The homopolar generator: an analytial example Hendrik van Hees August 7, 214 1 Introdution It is surprising that the homopolar generator, invented in one of Faraday s ingenious experiments in 1831, still
More information4. (12) Write out an equation for Poynting s theorem in differential form. Explain in words what each term means physically.
Eletrodynamis I Exam 3 - Part A - Closed Book KSU 205/2/8 Name Eletrodynami Sore = 24 / 24 points Instrutions: Use SI units. Where appropriate, define all variables or symbols you use, in words. Try to
More informationVector Field Theory (E&M)
Physis 4 Leture 2 Vetor Field Theory (E&M) Leture 2 Physis 4 Classial Mehanis II Otober 22nd, 2007 We now move from first-order salar field Lagrange densities to the equivalent form for a vetor field.
More informationFour-dimensional equation of motion for viscous compressible substance with regard to the acceleration field, pressure field and dissipation field
Four-dimensional equation of motion for visous ompressible substane with regard to the aeleration field, pressure field and dissipation field Sergey G. Fedosin PO box 6488, Sviazeva str. -79, Perm, Russia
More informationSpinning Charged Bodies and the Linearized Kerr Metric. Abstract
Spinning Charged Bodies and the Linearized Kerr Metri J. Franklin Department of Physis, Reed College, Portland, OR 97202, USA. Abstrat The physis of the Kerr metri of general relativity (GR) an be understood
More informationarxiv: v1 [physics.class-ph] 12 Mar 2012
Relativisti Dynamis of a Charged Partile in an Eletrosalar Field D.V. Podgainy 1, O.A. Zaimidoroga 2 arxiv:1203.2490v1 [physis.lass-ph] 12 Mar 2012 Joint Institute for Nulear Researh 141980, Dubna, Russia
More informationThe Lorenz Transform
The Lorenz Transform Flameno Chuk Keyser Part I The Einstein/Bergmann deriation of the Lorentz Transform I follow the deriation of the Lorentz Transform, following Peter S Bergmann in Introdution to the
More informationName Solutions to Test 1 September 23, 2016
Name Solutions to Test 1 September 3, 016 This test onsists of three parts. Please note that in parts II and III, you an skip one question of those offered. Possibly useful formulas: F qequb x xvt E Evpx
More informationThe Electromagnetic Radiation and Gravity
International Journal of Theoretial and Mathematial Physis 016, 6(3): 93-98 DOI: 10.593/j.ijtmp.0160603.01 The Eletromagneti Radiation and Gravity Bratianu Daniel Str. Teiului Nr. 16, Ploiesti, Romania
More informationHidden Momentum in a Spinning Sphere
Hidden Momentum in a Spinning Sphere 1 Problem Kirk T. MDonald Joseph Henry Laboratories, Prineton University, Prineton, NJ 8544 (August 16, 212; updated June 3, 217 A spinning sphere at rest has zero
More informationRelativity in Classical Physics
Relativity in Classial Physis Main Points Introdution Galilean (Newtonian) Relativity Relativity & Eletromagnetism Mihelson-Morley Experiment Introdution The theory of relativity deals with the study of
More informationAdvanced Computational Fluid Dynamics AA215A Lecture 4
Advaned Computational Fluid Dynamis AA5A Leture 4 Antony Jameson Winter Quarter,, Stanford, CA Abstrat Leture 4 overs analysis of the equations of gas dynamis Contents Analysis of the equations of gas
More informationWe consider the nonrelativistic regime so no pair production or annihilation.the hamiltonian for interaction of fields and sources is 1 (p
.. RADIATIVE TRANSITIONS Marh 3, 5 Leture XXIV Quantization of the E-M field. Radiative transitions We onsider the nonrelativisti regime so no pair prodution or annihilation.the hamiltonian for interation
More informationThe Corpuscular Structure of Matter, the Interaction of Material Particles, and Quantum Phenomena as a Consequence of Selfvariations.
The Corpusular Struture of Matter, the Interation of Material Partiles, and Quantum Phenomena as a Consequene of Selfvariations. Emmanuil Manousos APM Institute for the Advanement of Physis and Mathematis,
More information1 sin 2 r = 1 n 2 sin 2 i
Physis 505 Fall 005 Homework Assignment #11 Solutions Textbook problems: Ch. 7: 7.3, 7.5, 7.8, 7.16 7.3 Two plane semi-infinite slabs of the same uniform, isotropi, nonpermeable, lossless dieletri with
More informationAn Effective Photon Momentum in a Dielectric Medium: A Relativistic Approach. Abstract
An Effetive Photon Momentum in a Dieletri Medium: A Relativisti Approah Bradley W. Carroll, Farhang Amiri, and J. Ronald Galli Department of Physis, Weber State University, Ogden, UT 84408 Dated: August
More information[Khalid, 5(3): March 2018] ISSN DOI /zenodo Impact Factor
GLOBAL JOURNAL OF ENGINEERING SCIENCE AND RESEARCHES LORENZ TRANSFORMATION FOR FREE SPACE AND FIELDS USING MAXWELL S EQUATIONS AND NEWTON'S LAWS Nuha Abdelrahman Khalid*, Mubarak Dirar Abdallah, Zoalnoon
More informationThe concept of the general force vector field
The onept of the general fore vetor field Sergey G. Fedosin PO box 61488, Sviazeva str. 22-79, Perm, Russia E-mail: intelli@list.ru A hypothesis is suggested that the lassial eletromagneti and gravitational
More informationClass 3: Electromagnetism
Class 3: Electromagnetism In this class we will apply index notation to the familiar field of electromagnetism, and discuss its deep connection with relativity Class 3: Electromagnetism At the end of this
More informationA EUCLIDEAN ALTERNATIVE TO MINKOWSKI SPACETIME DIAGRAM.
A EUCLIDEAN ALTERNATIVE TO MINKOWSKI SPACETIME DIAGRAM. S. Kanagaraj Eulidean Relativity s.kana.raj@gmail.om (1 August 009) Abstrat By re-interpreting the speial relativity (SR) postulates based on Eulidean
More informationSURFACE WAVES OF NON-RAYLEIGH TYPE
SURFACE WAVES OF NON-RAYLEIGH TYPE by SERGEY V. KUZNETSOV Institute for Problems in Mehanis Prosp. Vernadskogo, 0, Mosow, 75 Russia e-mail: sv@kuznetsov.msk.ru Abstrat. Existene of surfae waves of non-rayleigh
More informationFinal Review. A Puzzle... Special Relativity. Direction of the Force. Moving at the Speed of Light
Final Review A Puzzle... Diretion of the Fore A point harge q is loated a fixed height h above an infinite horizontal onduting plane. Another point harge q is loated a height z (with z > h) above the plane.
More informationChapter 26 Lecture Notes
Chapter 26 Leture Notes Physis 2424 - Strauss Formulas: t = t0 1 v L = L0 1 v m = m0 1 v E = m 0 2 + KE = m 2 KE = m 2 -m 0 2 mv 0 p= mv = 1 v E 2 = p 2 2 + m 2 0 4 v + u u = 2 1 + vu There were two revolutions
More informationF = c where ^ı is a unit vector along the ray. The normal component is. Iν cos 2 θ. d dadt. dp normal (θ,φ) = dpcos θ = df ν
INTRODUCTION So far, the only information we have been able to get about the universe beyond the solar system is from the eletromagneti radiation that reahes us (and a few osmi rays). So doing Astrophysis
More informationPhys 561 Classical Electrodynamics. Midterm
Phys 56 Classial Eletrodynamis Midterm Taner Akgün Department of Astronomy and Spae Sienes Cornell University Otober 3, Problem An eletri dipole of dipole moment p, fixed in diretion, is loated at a position
More informationENERGY AND MOMENTUM IN ELECTROMAGNETIC WAVES
MISN-0-211 z ENERGY AND MOMENTUM IN ELECTROMAGNETIC WAVES y È B` x ENERGY AND MOMENTUM IN ELECTROMAGNETIC WAVES by J. S. Kovas and P. Signell Mihigan State University 1. Desription................................................
More informationModule II: Relativity and Electrodynamics
Module II: Relativity and Electrodynamics Lecture 2: Lorentz transformations of observables Amol Dighe TIFR, Mumbai Outline Length, time, velocity, acceleration Transformations of electric and magnetic
More informationAharonov-Bohm effect. Dan Solomon.
Aharonov-Bohm effet. Dan Solomon. In the figure the magneti field is onfined to a solenoid of radius r 0 and is direted in the z- diretion, out of the paper. The solenoid is surrounded by a barrier that
More informationTowards an Absolute Cosmic Distance Gauge by using Redshift Spectra from Light Fatigue.
Towards an Absolute Cosmi Distane Gauge by using Redshift Spetra from Light Fatigue. Desribed by using the Maxwell Analogy for Gravitation. T. De Mees - thierrydemees @ pandora.be Abstrat Light is an eletromagneti
More informationDerivation of Non-Einsteinian Relativistic Equations from Momentum Conservation Law
Asian Journal of Applied Siene and Engineering, Volue, No 1/13 ISSN 35-915X(p); 37-9584(e) Derivation of Non-Einsteinian Relativisti Equations fro Moentu Conservation Law M.O.G. Talukder Varendra University,
More informationELECTROMAGNETIC WAVES WITH NONLINEAR DISPERSION LAW. P. М. Меdnis
ELECTROMAGNETIC WAVES WITH NONLINEAR DISPERSION LAW P. М. Меdnis Novosibirs State Pedagogial University, Chair of the General and Theoretial Physis, Russia, 636, Novosibirs,Viljujsy, 8 e-mail: pmednis@inbox.ru
More informationPhysics 523, General Relativity Homework 4 Due Wednesday, 25 th October 2006
Physis 523, General Relativity Homework 4 Due Wednesday, 25 th Otober 2006 Jaob Lewis Bourjaily Problem Reall that the worldline of a ontinuously aelerated observer in flat spae relative to some inertial
More informationLagrangian Formulation of the Combined-Field Form of the Maxwell Equations
Physis Notes Note 9 Marh 009 Lagrangian Formulation of the Combined-Field Form of the Maxwell Equations Carl E. Baum University of New Mexio Department of Eletrial and Computer Engineering Albuquerque
More informationDynamics of the Electromagnetic Fields
Chapter 3 Dynamis of the Eletromagneti Fields 3.1 Maxwell Displaement Current In the early 1860s (during the Amerian ivil war!) eletriity inluding indution was well established experimentally. A big row
More informationTime Domain Method of Moments
Time Domain Method of Moments Massahusetts Institute of Tehnology 6.635 leture notes 1 Introdution The Method of Moments (MoM) introdued in the previous leture is widely used for solving integral equations
More information1 Summary of Electrostatics
1 Summary of Eletrostatis Classial eletrodynamis is a theory of eletri and magneti fields aused by marosopi distributions of eletri harges and urrents. In these letures, we reapitulate the basi onepts
More informationA proposed experiment for measuring the speed of propagation of the Coulomb force.
A proposed experiment for measuring the speed of propagation of the Coulomb fore. January 29, 2009 1 Introdution The eletri field at a time t due to an eletrial harge moving with veloity v is given, using
More informationThe Unified Geometrical Theory of Fields and Particles
Applied Mathematis, 014, 5, 347-351 Published Online February 014 (http://www.sirp.org/journal/am) http://dx.doi.org/10.436/am.014.53036 The Unified Geometrial Theory of Fields and Partiles Amagh Nduka
More informationAddition of velocities. Taking differentials of the Lorentz transformation, relative velocities may be calculated:
Addition of veloities Taking differentials of the Lorentz transformation, relative veloities may be allated: So that defining veloities as: x dx/dt, y dy/dt, x dx /dt, et. it is easily shown that: With
More informationRadiation processes and mechanisms in astrophysics 3. R Subrahmanyan Notes on ATA lectures at UWA, Perth 22 May 2009
Radiation proesses and mehanisms in astrophysis R Subrahmanyan Notes on ATA letures at UWA, Perth May 009 Synhrotron radiation - 1 Synhrotron radiation emerges from eletrons moving with relativisti speeds
More informationELECTROMAGNETIC NORMAL MODES AND DISPERSION FORCES.
ELECTROMAGNETIC NORMAL MODES AND DISPERSION FORCES. All systems with interation of some type have normal modes. One may desribe them as solutions in absene of soures; they are exitations of the system
More information). In accordance with the Lorentz transformations for the space-time coordinates of the same event, the space coordinates become
Relativity and quantum mehanis: Jorgensen 1 revisited 1. Introdution Bernhard Rothenstein, Politehnia University of Timisoara, Physis Department, Timisoara, Romania. brothenstein@gmail.om Abstrat. We first
More informationHamiltonian with z as the Independent Variable
Hamiltonian with z as the Independent Variable 1 Problem Kirk T. MDonald Joseph Henry Laboratories, Prineton University, Prineton, NJ 08544 Marh 19, 2011; updated June 19, 2015) Dedue the form of the Hamiltonian
More informationElectromagnetic radiation
5584 5585 8 Eletromagneti radiation 5586 5587 5588 5589 8. Solution of Maxwell equations with external urrent The eletromagneti field generated by an external (expliitly given) four-urrent J µ (x) is given
More informationThe Thomas Precession Factor in Spin-Orbit Interaction
p. The Thomas Preession Fator in Spin-Orbit Interation Herbert Kroemer * Department of Eletrial and Computer Engineering, Uniersity of California, Santa Barbara, CA 9306 The origin of the Thomas fator
More informationTHE TWIN PARADOX A RELATIVISTIC DOMAIN RESOLUTION
THE TWIN PARADOX A RELATIVISTIC DOMAIN RESOLUTION Peter G.Bass P.G.Bass www.relativitydomains.om January 0 ABSTRACT This short paper shows that the so alled "Twin Paradox" of Speial Relativity, is in fat
More informationThe concept of the general force vector field
OALib Journal, Vol. 3, P. 1-15 (16). http://dx.doi.org/1.436/oalib.11459 The onept of the general fore vetor field Sergey G. Fedosin PO box 61488, Sviazeva str. -79, Perm, Russia E-mail: intelli@list.ru
More informationF = F x x + F y. y + F z
ECTION 6: etor Calulus MATH20411 You met vetors in the first year. etor alulus is essentially alulus on vetors. We will need to differentiate vetors and perform integrals involving vetors. In partiular,
More informationELECTROMAGNETIC WAVES
ELECTROMAGNETIC WAVES Now we will study eletromagneti waves in vauum or inside a medium, a dieletri. (A metalli system an also be represented as a dieletri but is more ompliated due to damping or attenuation
More informationIn this case it might be instructive to present all three components of the current density:
Momentum, on the other hand, presents us with a me ompliated ase sine we have to deal with a vetial quantity. The problem is simplified if we treat eah of the omponents of the vet independently. s you
More informationn n=1 (air) n 1 sin 2 r =
Physis 55 Fall 7 Homework Assignment #11 Solutions Textbook problems: Ch. 7: 7.3, 7.4, 7.6, 7.8 7.3 Two plane semi-infinite slabs of the same uniform, isotropi, nonpermeable, lossless dieletri with index
More informationBrazilian Journal of Physics, vol. 29, no. 3, September, Classical and Quantum Mechanics of a Charged Particle
Brazilian Journal of Physis, vol. 9, no. 3, September, 1999 51 Classial and Quantum Mehanis of a Charged Partile in Osillating Eletri and Magneti Fields V.L.B. de Jesus, A.P. Guimar~aes, and I.S. Oliveira
More informationPhysics for Scientists & Engineers 2
Review Maxwell s Equations Physis for Sientists & Engineers 2 Spring Semester 2005 Leture 32 Name Equation Desription Gauss Law for Eletri E d A = q en Fields " 0 Gauss Law for Magneti Fields Faraday s
More informationPhysics; Watching the Game From the Outside
Physis; Wathing the Game From the Outside Roald C. Maximo Feb It is a good thing to have two ways of looking at a subjet, and also admit that there are two ways of looking at it. James Clerk Maxwell, on
More informationRelativity fundamentals explained well (I hope) Walter F. Smith, Haverford College
Relativity fundamentals explained well (I hope) Walter F. Smith, Haverford College 3-14-06 1 Propagation of waves through a medium As you ll reall from last semester, when the speed of sound is measured
More informationApplication of Bi-Quaternions in Physics
Appliation of Bi-Quaternions in Physis André Waser * First issued: 9.7. Last update: 6.5.7 This paper introdues a new bi-quaternion notation and applies this notation to eletrodynamis. A set of extended
More informationAnnouncements. Lecture 5 Chapter. 2 Special Relativity. The Doppler Effect
Announements HW1: Ch.-0, 6, 36, 41, 46, 50, 51, 55, 58, 63, 65 *** Lab start-u meeting with TA yesterday; useful? *** Lab manual is osted on the ourse web *** Physis Colloquium (Today 3:40m anelled ***
More informationBäcklund Transformations: Some Old and New Perspectives
Bäklund Transformations: Some Old and New Perspetives C. J. Papahristou *, A. N. Magoulas ** * Department of Physial Sienes, Helleni Naval Aademy, Piraeus 18539, Greee E-mail: papahristou@snd.edu.gr **
More informationEINSTEIN FIELD EQUATIONS OBTAINED ONLY WITH GAUSS CURVATURE AND ZOOM UNIVERSE MODEL CHARACTERISTICS
EINSTEIN FIELD EQUATIONS OBTAINED ONLY WITH GAUSS CURVATURE AND ZOOM UNIVERSE MODEL CHARACTERISTICS Sergio Garia Chimeno Abstrat Demonstration how to obtain the Einstein Field Equations without using the
More informationPY Modern Physics
PY 351 - Modern Physis Assignment 6 - Otober 19, 2017. Due in lass on Otober 26, 2017. Assignment 6: Do all six problems. After a base of 4 points (to make the maximum sore equal to 100), eah orret solution
More informationCherenkov Radiation. Bradley J. Wogsland August 30, 2006
Cherenkov Radiation Bradley J. Wogsland August 3, 26 Contents 1 Cherenkov Radiation 1 1.1 Cherenkov History Introdution................... 1 1.2 Frank-Tamm Theory......................... 2 1.3 Dispertion...............................
More informationRelativistic Dynamics
Chapter 7 Relativisti Dynamis 7.1 General Priniples of Dynamis 7.2 Relativisti Ation As stated in Setion A.2, all of dynamis is derived from the priniple of least ation. Thus it is our hore to find a suitable
More informationIntro to Nuclear and Particle Physics (5110)
Intro to Nulear and Partile Physis (5110) Marh 7, 009 Relativisti Kinematis 3/7/009 1 Relativisti Kinematis Review! Wherever you studied this before, look at it again, e.g. Tipler (Modern Physis), Hyperphysis
More informationProcessi di Radiazione e MHD
Proessi di Radiazione e MHD 0. Overview of elestial bodies and sky at various frequenies 1. Definition of main astrophysial observables. Radiative transfer 3. Blak body radiation 4. basi theory of radiation
More informationTheory of Dynamic Gravitational. Electromagnetism
Adv. Studies Theor. Phys., Vol. 6, 0, no. 7, 339-354 Theory of Dynami Gravitational Eletromagnetism Shubhen Biswas G.P.S.H.Shool, P.O.Alaipur, Pin.-7445(W.B), India shubhen3@gmail.om Abstrat The hange
More informationSimple Considerations on the Cosmological Redshift
Apeiron, Vol. 5, No. 3, July 8 35 Simple Considerations on the Cosmologial Redshift José Franiso Garía Juliá C/ Dr. Maro Mereniano, 65, 5. 465 Valenia (Spain) E-mail: jose.garia@dival.es Generally, the
More informationProperties of Quarks
PHY04 Partile Physis 9 Dr C N Booth Properties of Quarks In the earlier part of this ourse, we have disussed three families of leptons but prinipally onentrated on one doublet of quarks, the u and d. We
More informationModes are solutions, of Maxwell s equation applied to a specific device.
Mirowave Integrated Ciruits Prof. Jayanta Mukherjee Department of Eletrial Engineering Indian Institute of Tehnology, Bombay Mod 01, Le 06 Mirowave omponents Welome to another module of this NPTEL mok
More information( ) which is a direct consequence of the relativistic postulate. Its proof does not involve light signals. [8]
The Speed of Light under the Generalized Transformations, Inertial Transformations, Everyday Clok Synhronization and the Lorentz- Einstein Transformations Bernhard Rothenstein Abstrat. Starting with Edwards
More information22.54 Neutron Interactions and Applications (Spring 2004) Chapter 6 (2/24/04) Energy Transfer Kernel F(E E')
22.54 Neutron Interations and Appliations (Spring 2004) Chapter 6 (2/24/04) Energy Transfer Kernel F(E E') Referenes -- J. R. Lamarsh, Introdution to Nulear Reator Theory (Addison-Wesley, Reading, 1966),
More informationarxiv:physics/ v1 [physics.class-ph] 8 Aug 2003
arxiv:physis/0308036v1 [physis.lass-ph] 8 Aug 003 On the meaning of Lorentz ovariane Lszl E. Szab Theoretial Physis Researh Group of the Hungarian Aademy of Sienes Department of History and Philosophy
More informationElectromagnetic radiation of the travelling spin wave propagating in an antiferromagnetic plate. Exact solution.
arxiv:physis/99536v1 [physis.lass-ph] 15 May 1999 Eletromagneti radiation of the travelling spin wave propagating in an antiferromagneti plate. Exat solution. A.A.Zhmudsky November 19, 16 Abstrat The exat
More informationNew Potential of the. Positron-Emission Tomography
International Journal of Modern Physis and Appliation 6; 3(: 39- http://www.aasit.org/journal/ijmpa ISSN: 375-387 New Potential of the Positron-Emission Tomography Andrey N. olobuev, Eugene S. Petrov,
More informationQUANTUM MECHANICS II PHYS 517. Solutions to Problem Set # 1
QUANTUM MECHANICS II PHYS 57 Solutions to Problem Set #. The hamiltonian for a lassial harmoni osillator an be written in many different forms, suh as use ω = k/m H = p m + kx H = P + Q hω a. Find a anonial
More informationOn refinement of certain laws of classical electrodynamics
On refinement of ertain laws of lassial eletrodynamis http://fmnauka.narod.ru/works.html F. F. Mende Abstrat mende_fedor@mail.ru In the ontemporary lassial eletrodynamis exists many unresolved problems.
More informationarxiv:physics/ v1 14 May 2002
arxiv:physis/0205041 v1 14 May 2002 REPLY TO CRITICISM OF NECESSITY OF SIMULTANEOUS CO-EXISTENCE OF INSTANTANEOUS AND RETARDED INTERACTIONS IN CLASSICAL ELECTRODYNAMICS by J.D.Jakson ANDREW E. CHUBYKALO
More informationarxiv:gr-qc/ v7 14 Dec 2003
Propagation of light in non-inertial referene frames Vesselin Petkov Siene College, Conordia University 1455 De Maisonneuve Boulevard West Montreal, Quebe, Canada H3G 1M8 vpetkov@alor.onordia.a arxiv:gr-q/9909081v7
More information2. The Energy Principle in Open Channel Flows
. The Energy Priniple in Open Channel Flows. Basi Energy Equation In the one-dimensional analysis of steady open-hannel flow, the energy equation in the form of Bernoulli equation is used. Aording to this
More information1. RELATIVISTIC KINEMATICS
1. RELATIVISTIC KINEMATICS The one truth of whih the human mind an be ertain indeed, this is the meaning of onsiousness itself is the reognition of its own existene. That we may be seure in this truth
More informationarxiv: v1 [physics.gen-ph] 5 Jan 2018
The Real Quaternion Relativity Viktor Ariel arxiv:1801.03393v1 [physis.gen-ph] 5 Jan 2018 In this work, we use real quaternions and the basi onept of the final speed of light in an attempt to enhane the
More informationWe wrote down the Boltzmann equation for photons last time; it is:
1 Objetives In this leture we will take the photon multipole equations derived last time, and onvert them into Fourier-multipole spae. This will be onvenient for linear perturbation theory, sine eah Fourier
More informationDirac s equation We construct relativistically covariant equation that takes into account also the spin. The kinetic energy operator is
Dira s equation We onstrut relativistially ovariant equation that takes into aount also the spin The kineti energy operator is H KE p Previously we derived for Pauli spin matries the relation so we an
More informationGravitomagnetic Effects in the Kerr-Newman Spacetime
Advaned Studies in Theoretial Physis Vol. 10, 2016, no. 2, 81-87 HIKARI Ltd, www.m-hikari.om http://dx.doi.org/10.12988/astp.2016.512114 Gravitomagneti Effets in the Kerr-Newman Spaetime A. Barros Centro
More informationEinstein s Three Mistakes in Special Relativity Revealed. Copyright Joseph A. Rybczyk
Einstein s Three Mistakes in Speial Relativity Revealed Copyright Joseph A. Rybzyk Abstrat When the evidene supported priniples of eletromagneti propagation are properly applied, the derived theory is
More informationThe Special Theory of Relativity
The Speial Theory of Relatiity Galilean Newtonian Relatiity Galileo Galilei Isaa Newton Definition of an inertial referene frame: One in whih Newton s first law is alid. onstant if F0 Earth is rotating
More informationTHE REFRACTION OF LIGHT IN STATIONARY AND MOVING REFRACTIVE MEDIA
HDRONIC JOURNL 24, 113-129 (2001) THE REFRCTION OF LIGHT IN STTIONRY ND MOVING REFRCTIVE MEDI C. K. Thornhill 39 Crofton Road Orpington, Kent, BR6 8E United Kingdom Reeived Deember 10, 2000 Revised: Marh
More informationTemperature-Gradient-Driven Tearing Modes
1 TH/S Temperature-Gradient-Driven Tearing Modes A. Botrugno 1), P. Buratti 1), B. Coppi ) 1) EURATOM-ENEA Fusion Assoiation, Frasati (RM), Italy ) Massahussets Institute of Tehnology, Cambridge (MA),
More informationThe Reason of Photons Angular Distribution at Electron-Positron Annihilation in a Positron-Emission Tomograph
Advanes in Natural Siene ol 7, No,, pp -5 DOI: 3968/66 ISSN 75-786 [PRINT] ISSN 75-787 [ONLINE] wwwsanadanet wwwsanadaorg The Reason of Photons Angular Distribution at Eletron-Positron Annihilation in
More informationFig Review of Granta-gravel
0 Conlusion 0. Sope We have introdued the new ritial state onept among older onepts of lassial soil mehanis, but it would be wrong to leave any impression at the end of this book that the new onept merely
More informationThe Concept of Mass as Interfering Photons, and the Originating Mechanism of Gravitation D.T. Froedge
The Conept of Mass as Interfering Photons, and the Originating Mehanism of Gravitation D.T. Froedge V04 Formerly Auburn University Phys-dtfroedge@glasgow-ky.om Abstrat For most purposes in physis the onept
More informationThe gravitational phenomena without the curved spacetime
The gravitational phenomena without the urved spaetime Mirosław J. Kubiak Abstrat: In this paper was presented a desription of the gravitational phenomena in the new medium, different than the urved spaetime,
More information( x vt) m (0.80)(3 10 m/s)( s) 1200 m m/s m/s m s 330 s c. 3.
Solutions to HW 10 Problems and Exerises: 37.. Visualize: At t t t 0 s, the origins of the S, S, and S referene frames oinide. Solve: We have 1 ( v/ ) 1 (0.0) 1.667. (a) Using the Lorentz transformations,
More information