Examples of relativistic transformations

Size: px
Start display at page:

Download "Examples of relativistic transformations"

Transcription

1 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 = γ(e 2 βb 3 ) ; B 2 = γ(b 2 + βe 3 ) E 3 = γ(e 3 + βb 2 ) ; B 3 = γ(b 3 βe 2 ) For a boost in an arbitrary direction given by β, the transformation equations take the form; E = γ( E + β B) B = γ( B β E) γ2 γ + 1 β(β E) γ2 γ + 1 β(β B) 2 Field of a point charge Apply these to transform the field of a point charge at rest ( E = q r 2 ˆr) to a frame moving with constant velocity (Gaussian units). Restrict the E to a plane as we apply a boost in the 1 direction about which the E field is symmetric. This is shown in Figure 1. Thus obtain (assume that we take all times such that t = 0); E 1 = E 1 = qx 1 [x x 2 1 ]3/2 = qγx 1 [x γ2 x 2 1 ]3/2 E 3 = γe 3 = qγx 3 [x x 1 2 = qγx 3 ]3/2 [x γ2 x 2 1 ]3/2 Since there is no B field in the rest frame, the magnetic field is obtained from B = β E B 2 = qγβx 3 [x x 1 2 = β E ]3/2 3 B 3 = βe 2 = 0 1

2 V 1 q 3 Moving 1 q 3 Rest Figure 1: The field of a point charge in the (1,3) plane at rest and in a frame boosted in the 1 direction Put this back into spherical coordinates in the unprimed frame. E = q(1 β 2 ) r 2 [1 β 2 sin 2 3/2 ˆr (θ)] Now note that the field is radial and compressed perpendicular to the direction of motion. The paradox here is that at all points in space the E field points to the apparent position of the charge. Given causality, the question is how does an observer far away from the charge know where the charge will be? The answer is that the observed direction of the field only points to the position of where the charge is expected to be. If the charge is accelerated in some way, and the information of this acceleration does not reach the observer during the time of observation because of the maximum propagation velocity, c, the observer would believe that the charge contiuned moving in the same direction at a constant velocity. If in fact, the field lines were curved in some way this would represent radiation. A radiating charge loses energy, and a charge at rest does not. All intertial frames of reference are equivalent. Also note that a line integral; E d s 0. Of course we know that E = (1/c) B t, so that E = 0 only for static fields. 2

3 3 Wire carring a current We suppose a long straight wire carring a current, I. The curent produces a magnetic field, but there is no electric field as there is no net charge density on the wire. Suppose a charge, q is placed at rest near the wire. There is no force on the charge as its velocity is zero and there is no E field. However suppose we transform into a moving frame so that the charge has a constant velocity. In this frame there is a magnetic V B force on the charge, so that it moves either toward or away from the wire depending on the directions of the field and the velocity. As in the section above, this represents a paradox, and its resolution is instructive. Look at the current on the wire. As a model we assume that the electrons (negative charges) are moving to produce the current and the atoms of positive charge do not move, but they do cancel the charge of the negative electrons when the positive charge is at rest. Now transform to a frame so that the positive charges move. In this frame there will be a change to the positive charge density, λ + = δq/δl, because the elemental length δl is contracted to δl/γ. The negative charge density also changes, but because of the non-linear addition of velocities in the velocity transformations, it does not change the same amount. The negative charge density in the moving frame is λ = γ[1 β 0 β]. In this expression, β 0 is the initial velocity of the electrons and β the velocity of the moving frame with respect to the rest frame. Therefore the net charge density is; λ net = λ + λ = γβ 0 β Since there is now a net charge density on the wire there will be an electric field. The force due to the electric field will cancel the force due to the magentic field, so the charge does not move toward (or away from) the wire, as is the case for th erest system. 4 Proper time Suppose there are 2 space time points located at (ct 1, x 1 ) and (ct 2, x 2 ). The time for a light ray to travel between these points is; dτ 2 = (t 2 t 1 ) 2 (1/c) 2 ( x 2 x 1 ) 2 If the two events have the same space point, dτ would be the time recorded on a clock at rest in that frame of reference. Whenever two events can just be connected by a light ray that leaves one point and arrives at the other, then such events are simultaneous and dτ = 0. If the value of dτ is real then the points are time-like and events at these points can be observed. If dτ is imaginary the events would be space-like and could not be observed. Suppose we write the differential; dτ 2 = dt 2 (1/c) 2 ( d x dt )2 dt 2 = dt 2 (1 β 2 ) = (dt/γ) 2 3

4 Note here that; U α = dxα dτ = γ dxα dt = γv α which is the relativistic velocity. 5 Lorentz force As previously written, the Lorentz force is; F = d p dt = q( E + β B) (Gaussian units) Now consider the following contraction; F αδ g δβ U β = 0 E x E y E z E x 0 B z B y E y B z 0 B x E z B y B x 0 The matrix is obtained by matrix multiplication of the Field tensor F αδ by the metric g δβ. The above equation results in γ(e x V x + E y V y + E z V z F αδ g δβ U β γ(e x c + B z V y B y V z γ(e y c B z V x B x V z γ(e z c B y V x B x V y Note that dτ = dt/γ with dτ the proper time. Make the connection to the non-covarient equation by remembering that the power equals F V = q E V. The covarient form of the Lorentz force is then written; γc γv x γv y γv z (m 0 c) duα dτ = qf αβ U β The covarient force equation is then; d p dτ = γd p dt = (q/c)[ E(γc) + (γ V ) B] 6 Spin and angular momentum Consider a set of mass points which move in uniform motion with respect to each other. This system is shown in Figure 2. Locate a fixed point in the system by the vector, R. 4

5 X i X i R Figure 2: A set of mass points roatting in rigid motion with respect to each other Other points, i, in the system are located with respect to this point by the vectors x i. The energy and momentum of the points with respect to the origin are, e i and p i. Then the total energy is W = e i and total momentum P = p i. Define the angular momentum by ; L = x i p i This is an axial vector which has a dual representation by a tensor of rank 2 (matrix); M αβ = (x α i pβ i xβ i pα i ) The matrix (tensor of rank 2) is formed by the direct product of x i and p i. We wish to extend this to 4-D relativistic space, and in order to do this we need to find the time components of the angular momentum tensor. First note that M 00 = 0 because the tensor is anti-symmetric. Now consider in the rest frame; M 0k = ct p k i In the rest frame, p k i x k i e i = 0 so that; M 0k = x k i e i Take the time derivative of the above which gives, c β k i γ i m 0 i c 2 This result assumes that the total velocity of each particle β i remains constant, ie uniform rotation. The result is just the sum of the momentum which vanishes. We then choose M 0 k = 0 which satisfies this choice, and is also consistent with the CM definition in non-relativistic mechanics. Thus choose ; 5

6 R (ct, xi e i ee ) xi m i Non-relativistically γm i m i and the above spatial component approaches M. Then T xi e the 4 vector x i = x i = R which would be (0, x i ). The total angular momentum then becomes; M αβ = (x α i pβ i xβ i pα i ) + (Rp β i Rβ p α ) ei Identify the first term on the right side of the equation as the internal angular momentum of the system and the second term as the orbital angular momentum. Internal angular momentum is identified with spin, although spin in QM is not considered an internal rotation of a structureless particle, but due to the symmetry found in the equations which represent the particle. This will become more evident later. In any event the above description is classical (ignores QM) but we will call the internal angular momentum the system spin. Thus the spin can be represented by a pseudo-vector (antisymmetric tensor) whose time component is zero. (0, S 1, S 2, S 3 ). Then consider the contraction, S k p k, which is a scalar. If we evaluate this contraction in the rest frame, it equals zero. Because the contraction is a scalar it will be zero in all intetial frames. 7 Motion of Spin One way to connect spin to electromagnetism is through the magnetic moment, µ. µ = (1/2) [ r J]d 3 x Then J = ρ V and replace the charge density by the mass density multiplied by a spatially dependent function which represents the ratio of the charge density to the mass density at each spatial point. Carry out the integration to write; µ = (Qg/2M) S where Q is the system charge, M the system mass, and g is called the gyromagnetic ratio which measures the charge-to-mass ratio averaged over the system volume. Thus the spin S is related to the magnetic moment. In the rest frame, µ can be acted upon by a magnetic field. d S dt = µ B 6

7 β + δ β δ β β Figure 3: The application of 2 boosts which are not applied in the same direction Put this equation into covarient form by looking at the transformation of the time component. S 0 = 0 = γ(s 0 β S) = (1/c)U α S α In this equation U α is the relativistic 4-velocity, and S 0 = β S. Use the general transformation equation of a 4-vector and the above results to write; S = S γ γ + 1 β( β S) The primed frame is at rest. The text also shows that a covarient expression for the motion of the spin results in the BMT equation, which represents the spin precession when a particle with a magnetic moment is acted upon by an electromagnetic field; ds α dτ = (e/m)[(g/2)f αβ S β + (1/c 2 )(g/2 1)U α (S λ F λµ U µ )] Note the factor (g/2 1) which comes directly from relativity and indicates a special case. In QM a point particle satisfying a relativistic wave equation has a gyromagnetic ratio of 2, and this is no accident. Now suppose two boosts as illustrated in the Figure 3, are applied. Classically this would not be expected to change the orientation of the reference frame axes which should remain parallel. The transformation between the frames is obtained by writing the transformation matrix we previously obtained, A First boost along the 1 direction and then apply a boost which has both a component parallel to the 1 direction and a component perpendicular to the 1 direction. Then attempt to find the relation between the coordinates in the rest frames at t and t+δt. The text shows how to develop this transformation matrix. The result is; 7

8 1 γ 2 δβ 1 γδβ 2 0 A γ 2 γ + 1 δβ 1 1 = γ δβ 2 0 γδβ 2 γ + γ 1 δβ In the above, δ β i represents boosts in the i = 1 and i = 2 directions. The infinitesmal unitary operator has the form; A = I γ 1 β 2 β 1 δβ 2 S γ 2 δβ 1 κ 1 + γδβ 2 κ 2 The last 2 terms represent boosts which one might have expected. However there is also a rotation of the axes given by the 2 nd term. Thus 2 boosts which are not in the same direction, produce a rotation of the coordinates. This is called the Thomas precession, and is the relativistic effect which produces the spin precession seen in the BMT equation, for example. 8

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

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

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

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

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

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

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

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

1 Tensors and relativity

1 Tensors and relativity Physics 705 1 Tensors and relativity 1.1 History Physical laws should not depend on the reference frame used to describe them. This idea dates back to Galileo, who recognized projectile motion as free

More information

Electricity & Magnetism Qualifier

Electricity & Magnetism Qualifier Electricity & Magnetism Qualifier For each problem state what system of units you are using. 1. Imagine that a spherical balloon is being filled with a charged gas in such a way that the rate of charge

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

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

Quantum Field Theory Notes. Ryan D. Reece

Quantum Field Theory Notes. Ryan D. Reece Quantum Field Theory Notes Ryan D. Reece November 27, 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

More information

Chapter 10 Operators of the scalar Klein Gordon field. from my book: Understanding Relativistic Quantum Field Theory.

Chapter 10 Operators of the scalar Klein Gordon field. from my book: Understanding Relativistic Quantum Field Theory. Chapter 10 Operators of the scalar Klein Gordon field from my book: Understanding Relativistic Quantum Field Theory Hans de Vries November 11, 2008 2 Chapter Contents 10 Operators of the scalar Klein Gordon

More information

Tensors and Special Relativity

Tensors and Special Relativity Tensors and Special Relativity Lecture 6 1 Introduction and review of tensor algebra While you have probably used tensors of rank 1, i.e vectors, in special relativity, relativity is most efficiently expressed

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

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

Transformations. 1 The Lorentz Transformation. 2 Velocity Transformation

Transformations. 1 The Lorentz Transformation. 2 Velocity Transformation Transformations 1 The Lorentz Transformation In the last lecture we obtained the relativistic transformations for space/time between inertial frames. These transformations follow mainly from the postulate

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 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

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

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

Lorentz Transformations

Lorentz Transformations Lorentz Transformations 1 The Lorentz Transformation In the last lecture the relativistic transformations for space/time between inertial frames was obtained. These transformations esentially follow from

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

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

Chapter 2 Radiation of an Accelerated Charge

Chapter 2 Radiation of an Accelerated Charge Chapter 2 Radiation of an Accelerated Charge Whatever the energy source and whatever the object, (but with the notable exception of neutrino emission that we will not consider further, and that of gravitational

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

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

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

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

Particles and Deep Inelastic Scattering

Particles and Deep Inelastic Scattering Particles and Deep Inelastic Scattering Heidi Schellman University HUGS - JLab - June 2010 June 2010 HUGS 1 Course Outline 1. Really basic stuff 2. How we detect particles 3. Basics of 2 2 scattering 4.

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

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

Tensors, and differential forms - Lecture 2

Tensors, and differential forms - Lecture 2 Tensors, and differential forms - Lecture 2 1 Introduction The concept of a tensor is derived from considering the properties of a function under a transformation of the coordinate system. A description

More information

Phys 4322 Final Exam - Solution May 12, 2015

Phys 4322 Final Exam - Solution May 12, 2015 Phys 4322 Final Exam - Solution May 12, 2015 You may NOT use any book or notes other than that supplied with this test. You will have 3 hours to finish. DO YOUR OWN WORK. Express your answers clearly and

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

The Correct Derivation of Magnetism from Electrostatics Based on Covariant Formulation of Coulomb's Law

The Correct Derivation of Magnetism from Electrostatics Based on Covariant Formulation of Coulomb's Law The Correct Derivation of Magnetism from Electrostatics Based on Covariant Formulation of Coulomb's Law Mueiz Gafer KamalEldeen An Independent Researcher mueizphysics@gmail.com Abstract It is shown, by

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

Self field of a relativistic beam (Lecture 15)

Self field of a relativistic beam (Lecture 15) Self field of a relativistic beam (Lecture 15) February 1, 2016 259/441 Lecture outline We will study the electromagnetic field of a bunch of charged particles moving with relativistic velocity along a

More information

B(r) = µ 0a 2 J r 2ρ 2

B(r) = µ 0a 2 J r 2ρ 2 28 S8 Covariant Electromagnetism: Problems Questions marked with an asterisk are more difficult.. Eliminate B instead of H from the standard Maxwell equations. Show that the effective source terms are

More information

CHAPTER 11 RADIATION 4/13/2017. Outlines. 1. Electric Dipole radiation. 2. Magnetic Dipole Radiation. 3. Point Charge. 4. Synchrotron Radiation

CHAPTER 11 RADIATION 4/13/2017. Outlines. 1. Electric Dipole radiation. 2. Magnetic Dipole Radiation. 3. Point Charge. 4. Synchrotron Radiation CHAPTER 11 RADIATION Outlines 1. Electric Dipole radiation 2. Magnetic Dipole Radiation 3. Point Charge Lee Chow Department of Physics University of Central Florida Orlando, FL 32816 4. Synchrotron Radiation

More information

Modern Physics. Luis A. Anchordoqui. Department of Physics and Astronomy Lehman College, City University of New York. Lesson IV September 24, 2015

Modern Physics. Luis A. Anchordoqui. Department of Physics and Astronomy Lehman College, City University of New York. Lesson IV September 24, 2015 Modern Physics Luis A. Anchordoqui Department of Physics and Astronomy Lehman College, City University of New York Lesson IV September 24, 2015 L. A. Anchordoqui (CUNY) Modern Physics 9-24-2015 1 / 22

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

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

BMT Equation Analysis and Spin in Accelerator Physics

BMT Equation Analysis and Spin in Accelerator Physics Final project for Physics 342 - Quantum Mechanics II BMT Equation Analysis and Spin in Accelerator Physics T. Zolkin The University of Chicago, Department of Physics Abstract. As known from the non relativistic

More information

We begin our discussion of special relativity with a power point presentation, available on the website.

We begin our discussion of special relativity with a power point presentation, available on the website. Special Relativity We begin our discussion of special relativity with a power point presentation, available on the website.. Spacetime From the power point presentation, you know that spacetime is a four

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

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

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

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

Relativistic Transformations

Relativistic Transformations Relativistic Transformations Lecture 7 1 The Lorentz transformation In the last lecture we obtained the relativistic transformations for space/time between inertial frames. These transformations follow

More information

Postulates of Special Relativity

Postulates of Special Relativity Relativity Relativity - Seen as an intricate theory that is necessary when dealing with really high speeds - Two charged initially stationary particles: Electrostatic force - In another, moving reference

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

Synchrotron Power Cosmic rays are astrophysical particles (electrons, protons, and heavier nuclei) with extremely high energies. Cosmic-ray electrons in the galactic magnetic field emit the synchrotron

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

129 Lecture Notes More on Dirac Equation

129 Lecture Notes More on Dirac Equation 19 Lecture Notes More on Dirac Equation 1 Ultra-relativistic Limit We have solved the Diraction in the Lecture Notes on Relativistic Quantum Mechanics, and saw that the upper lower two components are large

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

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

Chapter 11. Angular Momentum

Chapter 11. Angular Momentum Chapter 11 Angular Momentum Angular Momentum Angular momentum plays a key role in rotational dynamics. There is a principle of conservation of angular momentum. In analogy to the principle of conservation

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

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

Lecture X: External fields and generation of gravitational waves

Lecture X: External fields and generation of gravitational waves Lecture X: External fields and generation of gravitational waves Christopher M. Hirata Caltech M/C 350-17, Pasadena CA 91125, USA (Dated: November 12, 2012) I. OVEVIEW Having examined weak field gravity

More information

Spacetime and 4 vectors

Spacetime and 4 vectors Spacetime and 4 vectors 1 Minkowski space = 4 dimensional spacetime Euclidean 4 space Each point in Minkowski space is an event. In SR, Minkowski space is an absolute structure (like space in Newtonian

More information

Physics 325: General Relativity Spring Final Review Problem Set

Physics 325: General Relativity Spring Final Review Problem Set Physics 325: General Relativity Spring 2012 Final Review Problem Set Date: Friday 4 May 2012 Instructions: This is the third of three review problem sets in Physics 325. It will count for twice as much

More information

= m(v) X B = m(0) 0 + m(v) x B m(0) + m(v) u = dx B dt B. m + m(v) v. 2u 1 + v A u/c 2 = v = 1 + v2. c 2 = 0

= m(v) X B = m(0) 0 + m(v) x B m(0) + m(v) u = dx B dt B. m + m(v) v. 2u 1 + v A u/c 2 = v = 1 + v2. c 2 = 0 7 Relativistic dynamics Lorentz transformations also aect the accelerated motion of objects under the inuence of forces. In Newtonian physics a constant force F accelerates an abject at a constant rate

More information

EM radiation - Lecture 14

EM radiation - Lecture 14 EM radiation - Lecture 14 1 Review Begin with a review of the potentials, fields, and Poynting vector for a point charge in accelerated motion. The retarded potential forms are given below. The source

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

Lorentz Force. Acceleration of electrons due to the magnetic field gives rise to synchrotron radiation Lorentz force.

Lorentz Force. Acceleration of electrons due to the magnetic field gives rise to synchrotron radiation Lorentz force. Set 10: Synchrotron Lorentz Force Acceleration of electrons due to the magnetic field gives rise to synchrotron radiation Lorentz force 0 E x E y E z dp µ dτ = e c F µ νu ν, F µ E x 0 B z B y ν = E y B

More information

Physical Dynamics (SPA5304) Lecture Plan 2018

Physical Dynamics (SPA5304) Lecture Plan 2018 Physical Dynamics (SPA5304) Lecture Plan 2018 The numbers on the left margin are approximate lecture numbers. Items in gray are not covered this year 1 Advanced Review of Newtonian Mechanics 1.1 One Particle

More information

2. Special Relativity (SR) explicit Lorentz transformations Particles with m > 0 can always be seen as boosted from their rest frame

2. Special Relativity (SR) explicit Lorentz transformations Particles with m > 0 can always be seen as boosted from their rest frame 2. Special Relativity (SR) explicit Lorentz transformations Particles with m > 0 can always be seen as boosted from their rest frame in frame O we see the particle as p µ = (E, p) =. (E,p,0,0) in its rest

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

Ch. 28: Sources of Magnetic Fields

Ch. 28: Sources of Magnetic Fields Ch. 28: Sources of Magnetic Fields Electric Currents Create Magnetic Fields A long, straight wire A current loop A solenoid Slide 24-14 Biot-Savart Law Current produces a magnetic field The Biot-Savart

More information

Introduction. Classical vs Modern Physics. Classical Physics: High speeds Small (or very large) distances

Introduction. Classical vs Modern Physics. Classical Physics: High speeds Small (or very large) distances Introduction Classical vs Modern Physics High speeds Small (or very large) distances Classical Physics: Conservation laws: energy, momentum (linear & angular), charge Mechanics Newton s laws Electromagnetism

More information

1. Kinematics, cross-sections etc

1. Kinematics, cross-sections etc 1. Kinematics, cross-sections etc A study of kinematics is of great importance to any experiment on particle scattering. It is necessary to interpret your measurements, but at an earlier stage to determine

More information

Physics 523, General Relativity

Physics 523, General Relativity Physics 53, General Relativity Homework Due Monday, 9 th October 6 Jacob Lewis Bourjaily Problem 1 Let frame O move with speed v in the x-direction relative to frame O. Aphotonwithfrequencyν measured in

More information

Rotational Mechanics and Relativity --- Summary sheet 1

Rotational Mechanics and Relativity --- Summary sheet 1 Rotational Mechanics and Relativity --- Summary sheet 1 Centre of Mass 1 1 For discrete masses: R m r For continuous bodies: R dm i i M M r body i Static equilibrium: the two conditions for a body in static

More information

Today s lecture: Motion in a Uniform Magnetic Field continued Force on a Current Carrying Conductor Introduction to the Biot-Savart Law

Today s lecture: Motion in a Uniform Magnetic Field continued Force on a Current Carrying Conductor Introduction to the Biot-Savart Law PHYSICS 1B Today s lecture: Motion in a Uniform Magnetic Field continued Force on a Current Carrying Conductor Introduction to the Biot-Savart Law Electricity & Magnetism A Charged Particle in a Magnetic

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

AST1100 Lecture Notes

AST1100 Lecture Notes AST1100 Lecture Notes 9 10 The special theory of relativity: Four vectors and relativistic dynamics 1 Worldlines In the spacetime diagram in figure 1 we see the path of a particle (or any object) through

More information

APPENDIX E SPIN AND POLARIZATION

APPENDIX E SPIN AND POLARIZATION APPENDIX E SPIN AND POLARIZATION Nothing shocks me. I m a scientist. Indiana Jones You ve never seen nothing like it, no never in your life. F. Mercury Spin is a fundamental intrinsic property of elementary

More information

1 Lagrangian for a continuous system

1 Lagrangian for a continuous system Lagrangian for a continuous system Let s start with an example from mechanics to get the big idea. The physical system of interest is a string of length and mass per unit length fixed at both ends, and

More information

The spacetime of special relativity

The spacetime of special relativity 1 The spacetime of special relativity We begin our discussion of the relativistic theory of gravity by reviewing some basic notions underlying the Newtonian and special-relativistic viewpoints of space

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 27 Sources of Magnetic Field

Chapter 27 Sources of Magnetic Field Chapter 27 Sources of Magnetic Field In this chapter we investigate the sources of magnetic of magnetic field, in particular, the magnetic field produced by moving charges (i.e., currents). Ampere s Law

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

PHYS 561 (GR) Homework 1 Solutions

PHYS 561 (GR) Homework 1 Solutions PHYS 561 (GR) Homework 1 Solutions HW Problem 1: A lightweight pole 20m long lies on the ground next to a barn 15m long. An Olympic athlete picks up the pole, carries it far away, and runs with it toward

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

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

Relativity SPECIAL, GENERAL, AND COSMOLOGICAL SECOND EDITION. Wolfgang Rindler. Professor of Physics The University of Texas at Dallas

Relativity SPECIAL, GENERAL, AND COSMOLOGICAL SECOND EDITION. Wolfgang Rindler. Professor of Physics The University of Texas at Dallas Relativity SPECIAL, GENERAL, AND COSMOLOGICAL SECOND EDITION Wolfgang Rindler Professor of Physics The University of Texas at Dallas OXPORD UNIVERSITY PRESS Contents Introduction l 1 From absolute space

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

Orbital Motion in Schwarzschild Geometry

Orbital Motion in Schwarzschild Geometry Physics 4 Lecture 29 Orbital Motion in Schwarzschild Geometry Lecture 29 Physics 4 Classical Mechanics II November 9th, 2007 We have seen, through the study of the weak field solutions of Einstein s equation

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

Thomas Precession and the Bargmann-Michel-Telegdi Equation

Thomas Precession and the Bargmann-Michel-Telegdi Equation Found Phys (011 41:1800 1809 DOI 10.1007/s10701-011-9579-7 Thomas Precession and the Bargmann-Michel-Telegdi Equation Krzysztof Rȩbilas Received: 8 September 010 / Accepted: 18 June 011 / Published online:

More information

Lecture 12 Notes, Electromagnetic Theory II Dr. Christopher S. Baird, faculty.uml.edu/cbaird University of Massachusetts Lowell

Lecture 12 Notes, Electromagnetic Theory II Dr. Christopher S. Baird, faculty.uml.edu/cbaird University of Massachusetts Lowell Lecture 12 Notes, Electromagnetic Theory II Dr. Christopher S. Baird, faculty.uml.edu/cbaird University of Massachusetts Lowell 1. Velocities in Special Relativity - As was done in Galilean relativity,

More information

Number-Flux Vector and Stress-Energy Tensor

Number-Flux Vector and Stress-Energy Tensor Massachusetts Institute of Technology Department of Physics Physics 8.962 Spring 2002 Number-Flux Vector and Stress-Energy Tensor c 2000, 2002 Edmund Bertschinger. All rights reserved. 1 Introduction These

More information

Rotational motion of a rigid body spinning around a rotational axis ˆn;

Rotational motion of a rigid body spinning around a rotational axis ˆn; Physics 106a, Caltech 15 November, 2018 Lecture 14: Rotations The motion of solid bodies So far, we have been studying the motion of point particles, which are essentially just translational. Bodies with

More information

Astrophysical Radiation Processes

Astrophysical Radiation Processes PHY3145 Topics in Theoretical Physics Astrophysical Radiation Processes 3: Relativistic effects I Dr. J. Hatchell, Physics 407, J.Hatchell@exeter.ac.uk Course structure 1. Radiation basics. Radiative transfer.

More information

Lecture: Lorentz Invariant Dynamics

Lecture: Lorentz Invariant Dynamics Chapter 5 Lecture: Lorentz Invariant Dynamics In the preceding chapter we introduced the Minkowski metric and covariance with respect to Lorentz transformations between inertial systems. This was shown

More information

Lecture 9 - Applications of 4 vectors, and some examples

Lecture 9 - Applications of 4 vectors, and some examples Lecture 9 - Applications of 4 vectors, and some examples E. Daw April 4, 211 1 Review of invariants and 4 vectors Last time we learned the formulae for the total energy and the momentum of a particle in

More information

A. B. Lahanas University of Athens, Physics Department, Nuclear and Particle Physics Section, Athens , Greece

A. B. Lahanas University of Athens, Physics Department, Nuclear and Particle Physics Section, Athens , Greece SPECIAL RELATIVITY A. B. Lahanas University of Athens, Physics Department, Nuclear and Particle Physics Section, Athens 157 71, Greece Abstract We give an introduction to Einstein s Special Theory of Relativity.

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