Physics 4183 Electricity and Magnetism II. Covariant Formulation of Electrodynamics-1

Size: px
Start display at page:

Download "Physics 4183 Electricity and Magnetism II. Covariant Formulation of Electrodynamics-1"

Transcription

1 Physics 4183 Electricity and Magnetism II Covariant Formulation of Electrodynamics 1 Introduction Having briefly discussed the origins of relativity, the Lorentz transformations, 4-vectors and tensors, and invariants, we are now prepared to discuss the relativity as it applies to electromagnetism. We will start with the formal aspects, that is we will discuss the covariant forms of the continuity equation, and the Maxwell equations. From this point we will move on to discussing how the fields transform. 1.1 The Continuity Equation We will use the continuity equation charge conservation) as the starting point in our development of a covariant form of electrodynamics. The continuity equation has the simple form of time derivative of a scalar function plus the divergence of a vector function equal to a constant ρ + J = 0 1) The derivatives can be written in the compact form µ µ = ct, x, y, ) z 2) If we assume that a current density 4-vector can be define as J µ = cρ, J), then the continuity equation takes on the very compact form µ J µ = 0 3) which is an invariant. This states that charge is conserved locally in all Lorentz frames; note the derivatives and the components of the J µ are not the same in all frames, but the form of the equation remains the same, the continuity equation is covariant. Based on the invariance of the continuity equation, the 4-vector J µ transforms like J ν = Λ ν µj µ µ J µ = µ Λ µ ν Λ ν µ J µ = ν J ν 4) An alternate way of show that the charge and current densities form a 4-vector, is to recall that in a given frame where the charge density has a relative velocity to the observer the current density is given by J = ρ v 5) where ρ corresponds to the charge density as observed in the observers frame. The charge and current densities written in terms of the charge density in its rest frame is ρ = γρ 0 J x = γv x ρ 0 6) Covariant Formulation of Electrodynamics-1

2 where for simplicity we have oriented our axis parallel to the direction of motion. Again, recall that the boost factor can be written in terms of derivatives γ = dt dτ γv x = dt dx dτ dt = dx dτ but this implies that γ is the zeroth component of the 4-velocity and v x γ is the first component of the 4-velocity. Therefore, the charge and current densities can be written as 7) J µ = ρ 0 u µ 8) The first question that we must ask ourselves, does this make sense? We start by looking at the charge density. Transforming from its rest frame, the charge density is note in the rest frame of the charge density the current density is zero) ρ = γρ while the current density is J 1 = cβ x γρ 9) To see whether this makes sense or not, let s consider a charge distribution place in a cube of length l in its rest frame. The cube is assumed to be traveling along the x-axis at a velocity β x, with one of the sides parallel to the x-axis see Fig. 1). The length of the cube is therefore contracted along the x-axis l = l 10) γ Next we assume that the container has impenetrable walls, therefore the total charge remains within the cube in both frame. The charge density as observed relative to the unprimed coordinates is ρ = Q l 3 /γ = γρ 11) as we had already deduced from the invariance of the continuity equation. The current density is the charge density multiplied by the velocity J x = cβ x γρ. The continuity equation implies charge conservation. The total charge is the volume integral over the charge density. In the rest frame, the total charge is Q = ρ dx dy dz 12) V In the unprimed frame, the total charge is Q = ρdx dy dz = V V γρ dx γ dy dz = Q 13) therefore both observers see the same total charge, and our original assumption of treating the charge and current densities as components of a 4-vector is correct. Covariant Formulation of Electrodynamics-2

3 t Frame S β x PSfrag replacements x Figure 1: Box in uniform motion relative to the frame S. 1.2 The Maxwell Equations As was previously shown, the Maxwell equations are not covariant. The example we used was Faraday s law. In the rest frame of a loop, the induced EMF is equal to minus the rate of change of the magnetic flux, while in a moving frame, the induce EMF has an added term that depends on the relative velocity of the two frames E d l = Φ B E v B) d l = Φ B Even though this is correct and consistent with what relativity tells us, it is not in the spirit of Einstein s first postulate, which states the the laws of physics are independent of what inertial frame they are viewed from. In this instance, we expect that Maxwell s equations retain the same form in all frames; the equations must be covariant form invariant), the values of the fields can change, but the form of the equation cannot. So how do we show the equations to be covariant? To begin with, let s write the Maxwell equations in free space 14) E = ρ ɛ 0 B = 0 These equation can be expressed in terms of potential E = B B = µ0 J + µ0 ɛ 0 E 15) B = 0 B = A 16) E = B E = Φ + A ) Let s assume that these equations can be rewritten in a covariant form by defining the 4-potential A µ = Φ/c, A ) 17) Covariant Formulation of Electrodynamics-3

4 where we justify this by noting that using the 4-current density leads back to the equations for the potentials in terms of there sources 1 A µ = µ 0 J µ 4π R d3 r 18) It is clear that the current density is a 4-vector, based on our previous arguments, but for the 4-potential to be a 4-vector the ratio d 3 r/ R must be an invariant. We start with an observer in the frame S, which is stationary with respect to the field point. The field point is located at 0, 0, 0, 0). The source point, in this frame, is located at ct, x, y, z) where ct = x 2 + y 2 + z 2 corresponds to the propagation time between the two points, in other words, we have to take into account that any change that occurs at the source takes some amount of time to be felt elsewhere. The component of R along its direction is R = ct. Let s now ask what an observer sees in the S frame that is traveling at a velocity β to the right relative to S. We will also assume that the time origins coincide t = t = 0. The value of the component of R along its direction is given by R = ct = γct βx) = Rγ 1 + x ) R β = Rγ1 + β cos θ) 19) see Fig. 2) The quantity d 3 r must take into account that changes that occur in the back end of the volume element takes a time cdt longer to propagate to the field point. The differential element is d 3 r = dx dy dz, where dy and dz are invariant. The other element is given by dx = γdx βc dt) 20) but as we stated, the time difference between front and back has to be account for dr = c dt dx = γdx + βdr) = γdx 1 + β dr ) = γdx1 + β cos θ) 21) dx Therefore d 3 r R = d3 r 22) R The 4-potential as defined above it a 4-vector, since it is composed of a 4-vector J µ and an invariant d 3 r/r. This 4-vector is given by A µ = φ/c, A x, A y, A z ) 23) where the factor of 1/c comes from the definition of the zeroth component of the 4-current cρ) and the units used in Eq. 18. Using the 4-potential, the relation between the electric field and the potential is written as follows E j c = j A A j) = j A 0 0 A j) = 0 A j j A 0) = F 0j 24) where we use µ = g µν ν µ = 0, 1, 2, 3 ) 25) 1 In order to prove that the 4-potential as defined has the correct transformation properties, requires the introduction of the retarded potential. That is the propagation speed of the field lines has to be taken into account. We will return to this subject later. Covariant Formulation of Electrodynamics-4

5 PSfrag replacements S S R dx θ dr θ x Figure 2: This shows the geometry used to show the invariance of d 3 r/r. The magnetic field becomes B k = i A j j A i) = i A j j A i) = F ij 26) Combining the two sets together leads to 0 E x /c E y /c E z /c F µν = µ A ν ν A µ = E x /c 0 B z B y E y /c B z 0 B x 27) E z /c B y B x 0 where µ corresponds to the row and ν to the column, and this tensor is called the Maxwell field strength tensor. Note that we started out with electric and magnetic fields, and ended up with a tensor that combines the two fields together. To get back to the Maxwell equations, we need to find mathematical operations that give back the curl and divergence of the fields. Notice that if we apply µ on F 0µ we get the divergence of the electric field E = ρ ɛ 0 c µ F 0µ = x E x + y E y + z E z = µ 0 J 0 = µ 0 cɛ 0 c 2 ρ ɛ 0 = ρ ɛ 0 28) while j acting on F ij we get the curl of the magnetic field, as an example take i = 1 [ B ] x = µ 0J x + ɛ 0 µ 0 E x ν F 1ν = 0 F F F F 13 = y B z z B y 1 c 2 te x = µ 0 J x 29) Therefore, taking the derivative of the field strength tensor gives ν F µν = µ 0 J µ 30) To arrive at the homogeneous set of Maxwell equations, expand them out using the field strength tensor B = 0 1 F F F 21 = 0 31) and [ ] E + B = 0 x 2 F F F 23 = 0 32) Covariant Formulation of Electrodynamics-5

6 The two equations can be combined to give α F βγ + γ F αβ + β F γα = ɛαβγδ F γδ = 0 33) where the totally antisymmetric tensor ɛ αβγδ is defined as + 1 if α = 0, β = 1, γ = 2, δ = 3 and even permutations of the indices ɛ αβγδ = 1 for odd permutations of the indices 0 if any indices are the same 34) This equation can be put into a simpler form by using a duality transformation as discussed earlier in the semester. We make the replacements E B and B E; note that since there is no magnetic charge it transform into not magentic charge after the transformation. The new new tensor, G µν, leads to the following form for the homogeneous Maxwell equation 0 B x B y B z ν G µν = 0 G µν = B x 0 E z /c E y /c B y E z /c 0 E y /c 35) B z E y /c E x /c 0 Note that the equation for G µν is the same equation as Eq. 33 for F µν using G αβ = 1 2 ɛαβγδ F γδ. 1.3 The Lorentz Force To complete the discussion of the equations of electrodynamics, we examine the Lorentz force, and put it into a covariant form. The standard form of the Lorentz force is d p ) dt = q E + v B Clearly this is not in a form that allows for simple transformations. Therefore, we rewrite the Lorentz force in replacing the time derivatives with the proper time derivatives, and add in the proper time derivative of p 0 d p ) dτ = q u 0 E/c + u B and where the term dp 0 /dτ is the rate of change of energy of the particle 36) dp 0 dτ = q u E 37) W = F l dw dt = F v 38) note there is no magnetic field term since it doesn t change the energy of a electrically charged particle. In the rest frame of the observer, this reduces to the standard form of the Lorentz force. Combining the Lorentz force with the components of the field strength tensor, we get which is in a covariant form the product of tensor and 4-vector). dp α dτ = qu βf αβ 39) Covariant Formulation of Electrodynamics-6

7 1.4 Field Transformations The final item that needs to calculated is the transformation equations of the electric and magnetic fields. We will determine these by examining how the Maxwell field strength tensor transforms. If we blindly apply the rules that we have discussed, we find that the field strength tensor transforms like F α β = Λ α µλ β νf µν 40) one transformation tensor per index. tensor in terms of the potential and transform each of the 4-vectors To verify that this is correct, we write the field strength F µν = µ A ν ν A µ 41) F α β = α A β β A α = Λ α µ µ Λ β νa ν Λ β ν ν Λ α µa µ = Λ β µλ α ν [ µ A ν ν A µ ] = Λ β µλ α νf µν 42) where we have used the known 4-vector transformations. Based on the transformation of the field strength tensor, we can now derive the transformations for the electric and magnetic fields. As usual, we will assume that the primed frame travels with velocity β along the x-axis of the unprimed frame. The y and y axis are assumed to be parallel as are the z and z axis. In matrix notation, the Lorentz transformation is γ βγ 0 0 [Λ µν ] = βγ γ ) We can start by calculating E x where we only write down the terms that are non-zero) E x = F 0 1 = Λ 0 µλ 1 νf µν = Λ 0 1Λ 1 0F 10 + Λ 0 0Λ 1 1F 01 = 1 β 2 )γ 2 E x = E x 44) therefore the component of the electric field along direction of relative motion stays the same. Next we E y the transformation for E z will have a similar form) E y = F 0 2 = Λ 0 µλ 2 νf µν = Λ 0 0Λ 2 2F 02 + Λ 0 1Λ 2 2F 12 = γe y βγb z = γ E y cβb z ) 45) while the E z transforms like E z = F 0 3 = Λ 0 µλ 3 νf µν = Λ 0 0Λ 3 3F 03 + Λ 0 1Λ 3 3F 13 = γ E z + cβb y ) 46) To calculate the transformations for the magnetic field, we proceed in the same manner as for calculating the electric fields. Start with B x B x = F 2 3 = Λ 2 µλ 3 νf µν = F 23 = B x 47) as was the case for E x. The B y component transforms as B y = F 31 = Λ 3 µλ 1 νf µν = Λ 3 3 Λ 1 0F 30 + Λ 1 1F 31) = γ B y + βe z /c) 48) Covariant Formulation of Electrodynamics-7

8 and finally the transformation for B z B z = F 1 2 = Λ 1 µλ 2 νf µν = Λ 2 2 Combining all the transformation equations together we have Λ 1 0F 02 + Λ 1 1F 12) = γ B z βe y /c) 49) E x = E x E y = γe y βcb z ) E z = γe z + βcb y ) 50) B x = B x B y = γb y + β/ce z ) B z = γb z β/ce y ) Covariant Formulation of Electrodynamics-8

Special Theory of Relativity

Special Theory of Relativity June 17, 2008 1 1 J.D.Jackson, Classical Electrodynamics, 3rd Edition, Chapter 11 Introduction Einstein s theory of special relativity is based on the assumption (which might be a deep-rooted superstition

More information

Overthrows a basic assumption of classical physics - that lengths and time intervals are absolute quantities, i.e., the same for all observes.

Overthrows a basic assumption of classical physics - that lengths and time intervals are absolute quantities, i.e., the same for all observes. Relativistic Electrodynamics An inertial frame = coordinate system where Newton's 1st law of motion - the law of inertia - is true. An inertial frame moves with constant velocity with respect to any other

More information

Introduction to Covariant Formulation

Introduction to Covariant Formulation Introduction to Covariant Formulation by Gerhard Kristensson April 1981 (typed and with additions June 2013) 1 y, z y, z S Event x v S x Figure 1: The two coordinate systems S and S. 1 Introduction and

More information

Lecture 13 Notes, Electromagnetic Theory II Dr. Christopher S. Baird, faculty.uml.edu/cbaird University of Massachusetts Lowell

Lecture 13 Notes, Electromagnetic Theory II Dr. Christopher S. Baird, faculty.uml.edu/cbaird University of Massachusetts Lowell Lecture 13 Notes, Electromagnetic Theory II Dr. Christopher S. Baird, faculty.uml.edu/cbaird University of Massachusetts Lowell 1. Covariant Geometry - We would like to develop a mathematical framework

More information

Module II: Relativity and Electrodynamics

Module 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 information

Covariant Formulation of Electrodynamics

Covariant Formulation of Electrodynamics Chapter 7. Covariant Formulation of Electrodynamics Notes: Most of the material presented in this chapter is taken from Jackson, Chap. 11, and Rybicki and Lightman, Chap. 4. Starting with this chapter,

More information

Physics 506 Winter 2006 Homework Assignment #8 Solutions

Physics 506 Winter 2006 Homework Assignment #8 Solutions Physics 506 Winter 2006 Homework Assignment #8 Solutions Textbook problems: Ch. 11: 11.13, 11.16, 11.18, 11.27 11.13 An infinitely long straight wire of negligible cross-sectional area is at rest and has

More information

FYS 3120: Classical Mechanics and Electrodynamics

FYS 3120: Classical Mechanics and Electrodynamics FYS 3120: Classical Mechanics and Electrodynamics Formula Collection Spring semester 2014 1 Analytical Mechanics The Lagrangian L = L(q, q, t), (1) is a function of the generalized coordinates q = {q i

More information

A Brief Introduction to Relativistic Quantum Mechanics

A Brief Introduction to Relativistic Quantum Mechanics A Brief Introduction to Relativistic Quantum Mechanics Hsin-Chia Cheng, U.C. Davis 1 Introduction In Physics 215AB, you learned non-relativistic quantum mechanics, e.g., Schrödinger equation, E = p2 2m

More information

Covariant Formulation of Electrodynamics

Covariant Formulation of Electrodynamics Chapter 7. Covariant Formulation of Electrodynamics Notes: Most of the material presented in this chapter is taken from Jackson, Chap. 11, and Rybicki and Lightman, Chap. 4. Starting with this chapter,

More information

Special Relativity. Chapter The geometry of space-time

Special Relativity. Chapter The geometry of space-time Chapter 1 Special Relativity In the far-reaching theory of Special Relativity of Einstein, the homogeneity and isotropy of the 3-dimensional space are generalized to include the time dimension as well.

More information

Covariant electrodynamics

Covariant electrodynamics Lecture 9 Covariant electrodynamics WS2010/11: Introduction to Nuclear and Particle Physics 1 Consider Lorentz transformations pseudo-orthogonal transformations in 4-dimentional vector space (Minkowski

More information

Physics 506 Winter 2008 Homework Assignment #8 Solutions. Textbook problems: Ch. 11: 11.5, 11.13, 11.14, 11.18

Physics 506 Winter 2008 Homework Assignment #8 Solutions. Textbook problems: Ch. 11: 11.5, 11.13, 11.14, 11.18 Physics 506 Winter 2008 Homework Assignment #8 Solutions Textbook problems: Ch. 11: 11.5, 11.13, 11.14, 11.18 11.5 A coordinate system K moves with a velocity v relative to another system K. In K a particle

More information

Chapter 11. Special Relativity

Chapter 11. Special Relativity Chapter 11 Special Relativity Note: Please also consult the fifth) problem list associated with this chapter In this chapter, Latin indices are used for space coordinates only eg, i = 1,2,3, etc), while

More information

Alternative method of developing Maxwell s fields

Alternative method of developing Maxwell s fields Apeiron, Vol. 14, No. 4, October 2007 464 Alternative method of developing Maxwell s fields Krzysztof Rȩbilas Zak lad Fizyki. Akademia Rolnicza im. Hugona Ko l l ataja Al. Mickiewicza 21, 31-120 Kraków.

More information

Examples of relativistic transformations

Examples of relativistic transformations Examples of relativistic transformations Lecture 9 1 Field transformations In the last lecture we obtained the field transformation equations. For a boost in the 1 direction E 1 = E 1 ; B 1 = B 1 E 2 =

More information

Mechanics Physics 151

Mechanics Physics 151 Mechanics Physics 151 Lecture 15 Special Relativity (Chapter 7) What We Did Last Time Defined Lorentz transformation Linear transformation of 4-vectors that conserve the length in Minkowski space Derived

More information

Übungen zur Elektrodynamik (T3)

Übungen zur Elektrodynamik (T3) Arnold Sommerfeld Center Ludwig Maximilians Universität München Prof. Dr. Ivo Sachs SoSe 08 Übungen zur Elektrodynamik (T3) Lösungen zum Übungsblatt 7 Lorentz Force Calculate dx µ and ds explicitly in

More information

Covarient Formulation Lecture 8

Covarient Formulation Lecture 8 Covarient Formulation Lecture 8 1 Covarient Notation We use a 4-D space represented by the Cartesian coordinates, x 0 (orx 4 ), x 1, x 2, x 3. The components describe a vector (tensor of rank 1) in this

More information

New Transformation Equations and the Electric Field Four-vector

New Transformation Equations and the Electric Field Four-vector New Transformation Equations and the Electric Field Four-vector Copyright c 1999 2008 David E. Rutherford All Rights Reserved E-mail: drutherford@softcom.net http://www.softcom.net/users/der555/newtransform.pdf

More information

New Transformation Equations and the Electric Field Four-vector

New Transformation Equations and the Electric Field Four-vector New Transformation Equations and the Electric Field Four-vector c Copyright 1999 2003 David E. Rutherford All Rights Reserved E-mail: drutherford@softcom.net http://www.softcom.net/users/der555/newtransform.pdf

More information

Einstein Toolkit Workshop. Joshua Faber Apr

Einstein Toolkit Workshop. Joshua Faber Apr Einstein Toolkit Workshop Joshua Faber Apr 05 2012 Outline Space, time, and special relativity The metric tensor and geometry Curvature Geodesics Einstein s equations The Stress-energy tensor 3+1 formalisms

More information

Relativistic Electrodynamics

Relativistic Electrodynamics Relativistic Electrodynamics Notes (I will try to update if typos are found) June 1, 2009 1 Dot products The Pythagorean theorem says that distances are given by With time as a fourth direction, we find

More information

General Relativity (225A) Fall 2013 Assignment 2 Solutions

General Relativity (225A) Fall 2013 Assignment 2 Solutions University of California at San Diego Department of Physics Prof. John McGreevy General Relativity 5A) Fall 13 Assignment Solutions Posted October 3, 13 Due Monday, October 15, 13 1. Special relativity

More information

Relativistic Dynamics

Relativistic Dynamics Chapter 4 Relativistic Dynamics The most important example of a relativistic particle moving in a potential is a charged particle, say an electron, moving in an electromagnetic field, which might be that

More information

Lorentz Transformations and Special Relativity

Lorentz Transformations and Special Relativity Lorentz Transformations and Special Relativity Required reading: Zwiebach 2.,2,6 Suggested reading: Units: French 3.7-0, 4.-5, 5. (a little less technical) Schwarz & Schwarz.2-6, 3.-4 (more mathematical)

More information

4/13/2015. Outlines CHAPTER 12 ELECTRODYNAMICS & RELATIVITY. 1. The special theory of relativity. 2. Relativistic Mechanics

4/13/2015. Outlines CHAPTER 12 ELECTRODYNAMICS & RELATIVITY. 1. The special theory of relativity. 2. Relativistic Mechanics CHAPTER 12 ELECTRODYNAMICS & RELATIVITY Lee Chow Department of Physics University of Central Florida Orlando, FL 32816 Outlines 1. The special theory of relativity 2. Relativistic Mechanics 3. Relativistic

More information

Instructor: Sudipta Mukherji, Institute of Physics, Bhubaneswar

Instructor: Sudipta Mukherji, Institute of Physics, Bhubaneswar Chapter 1 Lorentz and Poincare Instructor: Sudipta Mukherji, Institute of Physics, Bhubaneswar 1.1 Lorentz Transformation Consider two inertial frames S and S, where S moves with a velocity v with respect

More information

Uniformity of the Universe

Uniformity of the Universe Outline Universe is homogenous and isotropic Spacetime metrics Friedmann-Walker-Robertson metric Number of numbers needed to specify a physical quantity. Energy-momentum tensor Energy-momentum tensor of

More information

Examples - Lecture 8. 1 GPS System

Examples - Lecture 8. 1 GPS System Examples - Lecture 8 1 GPS System The global positioning system, GPS, was established in 1973, and has been updated almost yearly. The GPS calculates postion on the earth s surface by accurately measuring

More information

Gravitation: Special Relativity

Gravitation: Special Relativity An Introduction to General Relativity Center for Relativistic Astrophysics School of Physics Georgia Institute of Technology Notes based on textbook: Spacetime and Geometry by S.M. Carroll Spring 2013

More information

Special Relativity - QMII - Mechina

Special Relativity - QMII - Mechina Special Relativity - QMII - Mechina 2016-17 Daniel Aloni Disclaimer This notes should not replace a course in special relativity, but should serve as a reminder. I tried to cover as many important topics

More information

Physics 236a assignment, Week 2:

Physics 236a assignment, Week 2: Physics 236a assignment, Week 2: (October 8, 2015. Due on October 15, 2015) 1. Equation of motion for a spin in a magnetic field. [10 points] We will obtain the relativistic generalization of the nonrelativistic

More information

Examples. Figure 1: The figure shows the geometry of the GPS system

Examples. Figure 1: The figure shows the geometry of the GPS system Examples 1 GPS System The global positioning system was established in 1973, and has been updated almost yearly. The GPS calcualtes postion on the earth ssurface by accurately measuring timing signals

More information

Problem 1, Lorentz transformations of electric and magnetic

Problem 1, Lorentz transformations of electric and magnetic Problem 1, Lorentz transformations of electric and magnetic fields We have that where, F µν = F µ ν = L µ µ Lν ν F µν, 0 B 3 B 2 ie 1 B 3 0 B 1 ie 2 B 2 B 1 0 ie 3 ie 2 ie 2 ie 3 0. Note that we use the

More information

Dynamics of Relativistic Particles and EM Fields

Dynamics of Relativistic Particles and EM Fields October 7, 2008 1 1 J.D.Jackson, Classical Electrodynamics, 3rd Edition, Chapter 12 Lagrangian Hamiltonian for a Relativistic Charged Particle The equations of motion [ d p dt = e E + u ] c B de dt = e

More information

Simultaneity, Time Dilation, and Length Contraction Using Minkowski Diagrams and Lorentz Transformations

Simultaneity, Time Dilation, and Length Contraction Using Minkowski Diagrams and Lorentz Transformations Simultaneity, Time Dilation, and Length Contraction Using Minkowski Diagrams and Lorentz Transformations Dr. Russell L. Herman January 25, 2008 (modified: January 17, 2018) Abstract In these notes we present

More information

Radiative Processes in Astrophysics

Radiative Processes in Astrophysics Radiative Processes in Astrophysics 6. Relativistic Covariance & Kinematics Eline Tolstoy http://www.astro.rug.nl/~etolstoy/astroa07/ Practise, practise, practise... mid-term, 31st may, 9.15-11am As we

More information

SPECIAL RELATIVITY AND ELECTROMAGNETISM

SPECIAL RELATIVITY AND ELECTROMAGNETISM SPECIAL RELATIVITY AND ELECTROMAGNETISM MATH 460, SECTION 500 The following problems (composed by Professor P.B. Yasskin) will lead you through the construction of the theory of electromagnetism in special

More information

Lecture 9: RR-sector and D-branes

Lecture 9: RR-sector and D-branes Lecture 9: RR-sector and D-branes José D. Edelstein University of Santiago de Compostela STRING THEORY Santiago de Compostela, March 6, 2013 José D. Edelstein (USC) Lecture 9: RR-sector and D-branes 6-mar-2013

More information

E&M. 1 Capacitors. January 2009

E&M. 1 Capacitors. January 2009 E&M January 2009 1 Capacitors Consider a spherical capacitor which has the space between its plates filled with a dielectric of permittivity ɛ. The inner sphere has radius r 1 and the outer sphere has

More information

221A Miscellaneous Notes Continuity Equation

221A Miscellaneous Notes Continuity Equation 221A Miscellaneous Notes Continuity Equation 1 The Continuity Equation As I received questions about the midterm problems, I realized that some of you have a conceptual gap about the continuity equation.

More information

4-Vector Notation. Chris Clark September 5, 2006

4-Vector Notation. Chris Clark September 5, 2006 4-Vector Notation Chris Clark September 5, 2006 1 Lorentz Transformations We will assume that the reader is familiar with the Lorentz Transformations for a boost in the x direction x = γ(x vt) ȳ = y x

More information

General Relativity (j µ and T µν for point particles) van Nieuwenhuizen, Spring 2018

General Relativity (j µ and T µν for point particles) van Nieuwenhuizen, Spring 2018 Consistency of conservation laws in SR and GR General Relativity j µ and for point particles van Nieuwenhuizen, Spring 2018 1 Introduction The Einstein equations for matter coupled to gravity read Einstein

More information

Vectors in Special Relativity

Vectors in Special Relativity Chapter 2 Vectors in Special Relativity 2.1 Four - vectors A four - vector is a quantity with four components which changes like spacetime coordinates under a coordinate transformation. We will write the

More information

Particle Notes. Ryan D. Reece

Particle Notes. Ryan D. Reece Particle Notes Ryan D. Reece July 9, 2007 Chapter 1 Preliminaries 1.1 Overview of Special Relativity 1.1.1 Lorentz Boosts Searches in the later part 19th century for the coordinate transformation that

More information

2.1 The Ether and the Michelson-Morley Experiment

2.1 The Ether and the Michelson-Morley Experiment Chapter. Special Relativity Notes: Some material presented in this chapter is taken The Feynman Lectures on Physics, Vol. I by R. P. Feynman, R. B. Leighton, and M. Sands, Chap. 15 (1963, Addison-Wesley)..1

More information

A5682: Introduction to Cosmology Course Notes. 2. General Relativity

A5682: Introduction to Cosmology Course Notes. 2. General Relativity 2. General Relativity Reading: Chapter 3 (sections 3.1 and 3.2) Special Relativity Postulates of theory: 1. There is no state of absolute rest. 2. The speed of light in vacuum is constant, independent

More information

Tensors - Lecture 4. cos(β) sin(β) sin(β) cos(β) 0

Tensors - Lecture 4. cos(β) sin(β) sin(β) cos(β) 0 1 Introduction Tensors - Lecture 4 The concept of a tensor is derived from considering the properties of a function under a transformation of the corrdinate system. As previously discussed, such transformations

More information

Math. 460, Sec. 500 Fall, Special Relativity and Electromagnetism

Math. 460, Sec. 500 Fall, Special Relativity and Electromagnetism Math. 460, Sec. 500 Fall, 2011 Special Relativity and Electromagnetism The following problems (composed by Professor P. B. Yasskin) will lead you through the construction of the theory of electromagnetism

More information

Lecturer: Bengt E W Nilsson

Lecturer: Bengt E W Nilsson 9 3 19 Lecturer: Bengt E W Nilsson Last time: Relativistic physics in any dimension. Light-cone coordinates, light-cone stuff. Extra dimensions compact extra dimensions (here we talked about fundamental

More information

3.1 Transformation of Velocities

3.1 Transformation of Velocities 3.1 Transformation of Velocities To prepare the way for future considerations of particle dynamics in special relativity, we need to explore the Lorentz transformation of velocities. These are simply derived

More information

Journal of Physics: Conference Series. Related content. Recent citations OPEN ACCESS

Journal of Physics: Conference Series. Related content. Recent citations OPEN ACCESS Journal of Physics: Conference Series OPEN ACCESS The Lorentz transformations of the vectors E, B, P, M and the external electric fields from a stationary superconducting wire with a steady current and

More information

Physics 209 Fall 2002 Notes 5 Thomas Precession

Physics 209 Fall 2002 Notes 5 Thomas Precession Physics 209 Fall 2002 Notes 5 Thomas Precession Jackson s discussion of Thomas precession is based on Thomas s original treatment, and on the later paper by Bargmann, Michel, and Telegdi. The alternative

More information

Electromagnetic energy and momentum

Electromagnetic energy and momentum Electromagnetic energy and momentum Conservation of energy: the Poynting vector In previous chapters of Jackson we have seen that the energy density of the electric eq. 4.89 in Jackson and magnetic eq.

More information

General Relativity and Differential

General Relativity and Differential Lecture Series on... General Relativity and Differential Geometry CHAD A. MIDDLETON Department of Physics Rhodes College November 1, 2005 OUTLINE Distance in 3D Euclidean Space Distance in 4D Minkowski

More information

Chapter 17 The bilinear covariant fields of the Dirac electron. from my book: Understanding Relativistic Quantum Field Theory.

Chapter 17 The bilinear covariant fields of the Dirac electron. from my book: Understanding Relativistic Quantum Field Theory. Chapter 17 The bilinear covariant fields of the Dirac electron from my book: Understanding Relativistic Quantum Field Theory Hans de Vries November 10, 008 Chapter Contents 17 The bilinear covariant fields

More information

Field Theory exam II Solutions

Field Theory exam II Solutions Field Theory exam II Solutions Problem 1 (a) Consider point charges, one with charge q located at x 1 = (1, 0, 1), and the other one with charge q at x = (1, 0, 1). Compute the multipole moments q lm in

More information

Special Relativity and Maxwell Equations

Special Relativity and Maxwell Equations Special Relativity and Maxwell Equations by Bernd A. Berg Department of Physics Florida State University Tallahassee, FL 32306, USA. (Version March 11, 2011) Copyright c by the author. Chapter 1 An introduction

More information

Lecture III: Tensor calculus and electrodynamics in flat spacetime

Lecture III: Tensor calculus and electrodynamics in flat spacetime Lecture III: Tensor calculus and electrodynamics in flat spacetime Christopher M. Hirata Caltech M/C 350-17, Pasadena CA 91125, USA (Dated: October 5, 201 I. OVERVIEW In this lecture we will continue to

More information

Lecture Notes on Electromagnetism

Lecture Notes on Electromagnetism Lecture Notes on Electromagnetism Abstract. The contents of this text is based on the class notes on Electromagnetism for the PH412 course by Prof. Ananda Dasgupta, IISER Kolkata. Contents Chapter 1. Introduction

More information

Properties of Traversable Wormholes in Spacetime

Properties of Traversable Wormholes in Spacetime Properties of Traversable Wormholes in Spacetime Vincent Hui Department of Physics, The College of Wooster, Wooster, Ohio 44691, USA. (Dated: May 16, 2018) In this project, the Morris-Thorne metric of

More information

GRAVITATION F10. Lecture Maxwell s Equations in Curved Space-Time 1.1. Recall that Maxwell equations in Lorentz covariant form are.

GRAVITATION F10. Lecture Maxwell s Equations in Curved Space-Time 1.1. Recall that Maxwell equations in Lorentz covariant form are. GRAVITATION F0 S. G. RAJEEV Lecture. Maxwell s Equations in Curved Space-Time.. Recall that Maxwell equations in Lorentz covariant form are. µ F µν = j ν, F µν = µ A ν ν A µ... They follow from the variational

More information

Relativistic Kinematics

Relativistic Kinematics Chapter 3 Relativistic Kinematics Recall that we briefly discussed Galilean boosts, transformation going from one inertial frame to another one, the first moving with an infinitesimal velocity δv with

More information

A Dyad Theory of Hydrodynamics and Electrodynamics

A Dyad Theory of Hydrodynamics and Electrodynamics arxiv:physics/0502072v5 [physics.class-ph] 19 Jan 2007 A Dyad Theory of Hydrodynamics and Electrodynamics Preston Jones Department of Mathematics and Physics University of Louisiana at Monroe Monroe, LA

More information

Appendix Lecture 1. Special Relativity & General Relativity. introduc)on to Astrophysics, C. Bertulani, Texas A&M-Commerce 1

Appendix Lecture 1. Special Relativity & General Relativity. introduc)on to Astrophysics, C. Bertulani, Texas A&M-Commerce 1 Appendix Lecture 1 Special Relativity & General Relativity introduc)on to Astrophysics, C. Bertulani, Texas A&M-Commerce 1 A.1 Galileo s relativity Newton s laws of motion must be implemented relative

More information

Special and General Relativity (PHZ 4601/5606) Fall 2018 Classwork and Homework. Every exercise counts 10 points unless stated differently.

Special and General Relativity (PHZ 4601/5606) Fall 2018 Classwork and Homework. Every exercise counts 10 points unless stated differently. 1 Special and General Relativity (PHZ 4601/5606) Fall 2018 Classwork and Homework Every exercise counts 10 points unless stated differently. Set 1: (1) Homework, due ( F ) 8/31/2018 before ( ) class. Consider

More information

MATH 423 January 2011

MATH 423 January 2011 MATH 423 January 2011 Examiner: Prof. A.E. Faraggi, Extension 43774. Time allowed: Two and a half hours Full marks can be obtained for complete answers to FIVE questions. Only the best FIVE answers will

More information

Solution to Problem Set 4

Solution to Problem Set 4 Solution to Problem Set 4 October 017 Pb 1. 0 pts. There are many ways of doing this problem but the easiest would be â α =â ˆD(α) 0 = â exp ( αâ α â ) 0 = â e α α/ e αâ 0 = α + α e α α/ e αâ 0 = α + α

More information

General Relativity and Cosmology Mock exam

General Relativity and Cosmology Mock exam Physikalisches Institut Mock Exam Universität Bonn 29. June 2011 Theoretische Physik SS 2011 General Relativity and Cosmology Mock exam Priv. Doz. Dr. S. Förste Exercise 1: Overview Give short answers

More information

Scott Hughes 12 May Massachusetts Institute of Technology Department of Physics Spring 2005

Scott Hughes 12 May Massachusetts Institute of Technology Department of Physics Spring 2005 Scott Hughes 12 May 2005 24.1 Gravity? Massachusetts Institute of Technology Department of Physics 8.022 Spring 2005 Lecture 24: A (very) brief introduction to general relativity. The Coulomb interaction

More information

611: Electromagnetic Theory II

611: Electromagnetic Theory II 611: Electromagnetic Theory II CONTENTS Special relativity; Lorentz covariance of Maxwell equations Scalar and vector potentials, and gauge invariance Relativistic motion of charged particles Action principle

More information

Special Relativity-General Discussion

Special Relativity-General Discussion Chapter 1 Special Relativity-General Discussion Let us consider a space-time event. By this we mean a physical occurence at some point in space at a given time. In order to characterize this event we introduce

More information

2.1 The metric and and coordinate transformations

2.1 The metric and and coordinate transformations 2 Cosmology and GR The first step toward a cosmological theory, following what we called the cosmological principle is to implement the assumptions of isotropy and homogeneity withing the context of general

More information

A873: Cosmology Course Notes. II. General Relativity

A873: Cosmology Course Notes. II. General Relativity II. General Relativity Suggested Readings on this Section (All Optional) For a quick mathematical introduction to GR, try Chapter 1 of Peacock. For a brilliant historical treatment of relativity (special

More information

A WAY TO DISCOVER MAXWELL S EQUATIONS THEORETICALLY. Krzysztof Rȩbilas

A WAY TO DISCOVER MAXWELL S EQUATIONS THEORETICALLY. Krzysztof Rȩbilas A WAY TO DISCOER MAXWELL S EQUATIONS THEORETICALLY Krzysztof Rȩbilas arxiv:1309.6531v1 [physics.class-ph] 23 Aug 2013 Zak lad Fizyki. Akademia Rolnicza im. Hugona Ko l l ataja. Al. Mickiewicza 21, 31-120

More information

Special Theory of Relativity Prof. Shiva Prasad Department of Physics Indian Institute of Technology, Bombay

Special Theory of Relativity Prof. Shiva Prasad Department of Physics Indian Institute of Technology, Bombay Special Theory of Relativity Prof. Shiva Prasad Department of Physics Indian Institute of Technology, Bombay Lecture - 24 Current Density Four Vector and Maxwell Equation Hello, so we have now come to

More information

Construction of Field Theories

Construction of Field Theories Physics 411 Lecture 24 Construction of Field Theories Lecture 24 Physics 411 Classical Mechanics II October 29th, 2007 We are beginning our final descent, and I ll take the opportunity to look at the freedom

More information

Figure 1: Grad, Div, Curl, Laplacian in Cartesian, cylindrical, and spherical coordinates. Here ψ is a scalar function and A is a vector field.

Figure 1: Grad, Div, Curl, Laplacian in Cartesian, cylindrical, and spherical coordinates. Here ψ is a scalar function and A is a vector field. Figure 1: Grad, Div, Curl, Laplacian in Cartesian, cylindrical, and spherical coordinates. Here ψ is a scalar function and A is a vector field. Figure 2: Vector and integral identities. Here ψ is a scalar

More information

Fundamental equations of relativistic fluid dynamics

Fundamental equations of relativistic fluid dynamics CHAPTER VI Fundamental equations of relativistic fluid dynamics When the energy density becomes large as may happen for instance in compact astrophysical objects, in the early Universe, or in high-energy

More information

2 Feynman rules, decay widths and cross sections

2 Feynman rules, decay widths and cross sections 2 Feynman rules, decay widths and cross sections 2.1 Feynman rules Normalization In non-relativistic quantum mechanics, wave functions of free particles are normalized so that there is one particle in

More information

Chapter 12. Electrodynamics and Relativity. Does the principle of relativity apply to the laws of electrodynamics?

Chapter 12. Electrodynamics and Relativity. Does the principle of relativity apply to the laws of electrodynamics? Chapter 12. Electrodynamics and Relativity Does the principle of relativity apply to the laws of electrodynamics? 12.1 The Special Theory of Relativity Does the principle of relativity apply to the laws

More information

Minkowski spacetime. Pham A. Quang. Abstract: In this talk we review the Minkowski spacetime which is the spacetime of Special Relativity.

Minkowski spacetime. Pham A. Quang. Abstract: In this talk we review the Minkowski spacetime which is the spacetime of Special Relativity. Minkowski spacetime Pham A. Quang Abstract: In this talk we review the Minkowski spacetime which is the spacetime of Special Relativity. Contents 1 Introduction 1 2 Minkowski spacetime 2 3 Lorentz transformations

More information

Special Relativity and Maxwell Equations

Special Relativity and Maxwell Equations Special Relativity and Maxwell Equations by Bernd A. Berg Department of Physics Florida State University Tallahassee, FL 32306, USA. Copyright c by the author. Chapter 1 A self-contained summary of the

More information

PROBLEM SET 1 SOLUTIONS

PROBLEM SET 1 SOLUTIONS MASSACHUSETTS INSTITUTE OF TECHNOLOGY Physics Department 8.323: Relativistic Quantum Field Theory I Prof.Alan Guth February 29, 2008 PROBLEM SET 1 SOLUTIONS Problem 1: The energy-momentum tensor for source-free

More information

Lorentz covariance and special relativity

Lorentz covariance and special relativity Chapter 4 Lorentz covariance and special relativity To go beyond Newtonian gravitation we must consider, with Einstein, the intimate relationship between the curvature of space and the gravitational field.

More information

Review and Notation (Special relativity)

Review and Notation (Special relativity) Review and Notation (Special relativity) December 30, 2016 7:35 PM Special Relativity: i) The principle of special relativity: The laws of physics must be the same in any inertial reference frame. In particular,

More information

Electrodynamics Exam Solutions

Electrodynamics Exam Solutions Electrodynamics Exam Solutions Name: FS 215 Prof. C. Anastasiou Student number: Exercise 1 2 3 4 Total Max. points 15 15 15 15 6 Points Visum 1 Visum 2 The exam lasts 18 minutes. Start every new exercise

More information

CHAPTER 8 CONSERVATION LAWS

CHAPTER 8 CONSERVATION LAWS CHAPTER 8 CONSERVATION LAWS Outlines 1. Charge and Energy 2. The Poynting s Theorem 3. Momentum 4. Angular Momentum 2 Conservation of charge and energy The net amount of charges in a volume V is given

More information

General Lorentz Boost Transformations, Acting on Some Important Physical Quantities

General Lorentz Boost Transformations, Acting on Some Important Physical Quantities General Lorentz Boost Transformations, Acting on Some Important Physical Quantities We are interested in transforming measurements made in a reference frame O into measurements of the same quantities as

More information

Contravariant and covariant vectors

Contravariant and covariant vectors Faculty of Engineering and Physical Sciences Department of Physics Module PHY08 Special Relativity Tensors You should have acquired familiarity with the following ideas and formulae in attempting the questions

More information

Electromagnetic Theory I

Electromagnetic Theory I Electromagnetic Theory I Final Examination 18 December 2009, 12:30-2:30 pm Instructions: Answer the following 10 questions, each of which is worth 10 points. Explain your reasoning in each case. Use SI

More information

Maxwell's Equations and Conservation Laws

Maxwell's Equations and Conservation Laws Maxwell's Equations and Conservation Laws 1 Reading: Jackson 6.1 through 6.4, 6.7 Ampère's Law, since identically. Although for magnetostatics, generally Maxwell suggested: Use Gauss's Law to rewrite continuity

More information

Special Relativity and Electromagnetism

Special Relativity and Electromagnetism 1/32 Special Relativity and Electromagnetism Jonathan Gratus Cockcroft Postgraduate Lecture Series October 2016 Introduction 10:30 11:40 14:00? Monday SR EM Tuesday SR EM Seminar Four lectures is clearly

More information

Introduction and Review Lecture 1

Introduction and Review Lecture 1 Introduction and Review Lecture 1 1 Fields 1.1 Introduction This class deals with classical electrodynamics. Classical electrodynamics is the exposition of electromagnetic interactions between the develoment

More information

The Lorentz Transformation

The Lorentz Transformation The Lorentz Transformation During the fourth week of the course, we spent some time discussing how the coordinates of two different reference frames were related to each other. Now that we know about the

More information

General Relativity I

General Relativity I General Relativity I presented by John T. Whelan The University of Texas at Brownsville whelan@phys.utb.edu LIGO Livingston SURF Lecture 2002 July 5 General Relativity Lectures I. Today (JTW): Special

More information

Physics 411 Lecture 22. E&M and Sources. Lecture 22. Physics 411 Classical Mechanics II

Physics 411 Lecture 22. E&M and Sources. Lecture 22. Physics 411 Classical Mechanics II Physics 411 Lecture 22 E&M and Sources Lecture 22 Physics 411 Classical Mechanics II October 24th, 2007 E&M is a good place to begin talking about sources, since we already know the answer from Maxwell

More information

Special Relativity-General Discussion

Special Relativity-General Discussion Chapter 1 Special Relativity-General Discussion Let us consider a spacetime event. By this we mean a physical occurence at some point in space at a given time. in order to characterize this event we introduce

More information

Electromagnetic Wave Propagation. in a Moving Chiral Medium

Electromagnetic Wave Propagation. in a Moving Chiral Medium Adv. Studies Theor. Phys., Vol. 4, 2010, no. 4, 165-172 Electromagnetic Wave Propagation in a Moving Chiral Medium P. Hillion Institut Henri Poincaré, 86 Bis Route de Croissy, 78110 Le Vésinet, France

More information