Special Relativity & Radiative Processes

Size: px
Start display at page:

Download "Special Relativity & Radiative Processes"

Transcription

1 Special Relativity & Radiative Processes

2 Special Relativity Special Relativity is a theory describing the motion of particles and fields at any speed. It is based on two principles: 1. All inertial frames are equivalent for all experiments i.e. no experiment can measure absolute velocity. 2. Maxwell's equations and the speed of light must be the same for all observers.

3 Galilean Relativity Applies Appliesto toall allinertial inertialand andnon-inertial non-inertial frames framesat atlow lowspeeds. speeds. The laws of motion are the same in all inertial frames. Special Relativity Applies Appliesto toall allinertial inertialand andnon-inertial non-inertial frames. frames. The laws of motion are the same in all inertial frames. General Relativity Applies Appliesto toall allinertial inertialand andnon-inertial non-inertial frames frames++gravitational gravitationalfields. fields.

4 Lorentz Transformations Lorentz LorentzTransformations: Transformations:Both Bothspace spaceand andtime time are subject to transformation. The description of are subject to transformation. The description ofevents events occurring at a certain location in space and time depends occurring at a certain location in space and time depends on onthe theparticular particularreference referenceframe frameof ofchoice. choice.

5 Light Cones

6 Relativity of Simultaneity

7 The Andromeda Paradox Formulated first by R. Penrose to illustrate the apparent paradox of relativity of simultaneity

8 Lorentz-Fitzgerald Contraction Note: the two observers in K and K' would measure the same effect with respect to each other. How is that possible? Solution: Lorentz transformation of time is NOT Lorentz invariant since it depends also on space. Therefore temporal simultaneity is NOT Lorentz invariant. Therefore each observer does not see the other carrying the measurement of the two ends of the stick at the same time.

9 Time Dilation Time in the lab frame flows faster than in the moving frame. Same story here: both observers will see the each other's clock slowing down. Each would object that the clocks used by the other to measure the time interval were not synchronized.

10 Observability of Lorentz contraction Question for you: Lorentz contraction and time dilation assume that you are carrying your measurements with rods, i.e., you can carry the measurement in place. But what happens when you use photons? This is the situation we encounter in astronomy, basically all information is carried by photons and we make measurements by collecting photons on a detector.

11

12 Diameter: light years

13 This picture does not represent an instant of the Andromeda Galaxy. Indeed the photons you're recording were emitted with up to 200,000 years difference. Diameter: light years What you're seeing are photons arriving at the same time, but NOT emitted at the same time.

14 Question: Given that the speed of light has a finite propagation speed, can we ever observe the Lorentz contraction and time dilation when we measure photons to carry our measurements? (As is the case in astronomy) J. Teller: Invisibility of the Lorentz Contraction R. Penrose: The Apparent Shape of a Relativistically Moving Sphere A. Lampa: "Wie erscheint nach der Relativitätstheorie ein bewegter Stab einem ruhenden Beobachter?

15

16 Here the square represents an object of finite size and extension. In other words any real object we can observe.

17 Measured with a ruler Measured with photons

18 A sphere would be contracted along the direction of motion (Lorentz contraction) However, due to the finite speed of propagation of light, photons arriving simultaneously at the observer will still produce a spherical object with no visible Lorentz contraction.

19

20 Time Dilation or Contraction?

21 Relativistic Doppler Boost Let's start from this expression we derived before: Δ t =γ (1 β cos θ)δ t ' We know that frequency is the inverse of time so we can write: ' ' ν ν= =ν δ γ(1 β cos θ) This is the relativistic Doppler effect, based on the time dilation AND the finite time for light propagation.

22 Aberration of Light

23 Lorentz Transformations of Velocities There are the velocity transformations when the velocity is on the x-axis direction. What about a more general form?

24 Take v along an arbitrary direction. Take the parallel and perpendicular components of u to v. Aberration formula Aberration of light (u = c)

25

26

27

28 Radius R ASSUMPTIONS 1. Jet is moving with bulk Lorentz factor Gamma 2. BL photons are produced in a sphere of radius R 3. The radiation is monochromatic

29 Radius R Blueshifted 90 deg. 1/Gamma by a factor Γ

30 Radius R Intensity boost: 4 I ' =δ ' I Blueshifted 90 deg. 1/Gamma by a factor Γ

31 Radius R Intensity boost: 4 I ' =δ ' I Monochromatic flux spreads across frequencies. Blueshifted 90 deg. 1/Gamma by a factor Γ

32 Radius R Intensity boost: 4 I ' =δ ' I Monochromatic flux spreads across frequencies. Blueshifted 90 deg. 1/Gamma by a factor Γ

33 Intensity, opacity and emissivity Transformation Iν = Lorentz Invariant 3 ν Sν = Lorentz Invariant 3 ν

34 Intensity, opacity and emissivity Transformation Since exp(-tau) gives the fraction of photons passing through the material, the optical depth must be a Lorentz Invariant (i.e., simple counting does not change the outcome in any reference frame). l αν τ= = Lorentz Invariant sin θ Similar arguments can be used to show that also the emissivity divided by the frequency squared is a Lorentz Invariant: jν = Lorentz Invariant 2 ν

35 Superluminal Motion Special Relativity states that the speed of light cannot be crossed. So how do you explain the following image?

36 To answer this question look at the exercise 4.7 of the R&L Δ te Time to move from 1 to 2 (in reference frame K) 2 is closer to observer than 1, therefore: Δ t a=δ t 'e γ(1 β cos θ)=δ t e (1 β cos θ) 3 The displacement 3 2 is v sin θ Δ t e Therefore the apparent velocity must be: Observer v sin θ Δ t e v sin θ v app = = Δ ta 1 β cos θ

37 To answer this question look at the exercise 4.7 of the R&L How can we now find the maximum of this apparent velocity? v sin θ Δ t e v sin θ v app = = Δ ta 1 β cos θ 3 Observer

38 To answer this question look at the exercise 4.7 of the R&L How can we now find the maximum of this apparent velocity? v sin θ Δ t e v sin θ v app = = Δ ta 1 β cos θ Differentiate (wrt the angle theta) and set the expression to zero: 3 v Observer max app v 1 β = =γ v 2 1 β 2 So if the velocity v is large and gamma is >>1 you can easily go to apparent velocities >> c

39

40

41

42 Covariance of Electromagnetic Phenomena Consider a capacitor, with plate separation d and charge density σ. We know that the field within the plates is E and it does not depend on the plate separation d.

43 Covariance of Electromagnetic Phenomena E per =γ E per ' B per = γ β E per y E v B field created by surface current density: ' ' μ = σ v x ' par = E par (Remember that the E field of a capacitor does not depend on the plate separation d)

Doppler shift and aberration for spherical electromagnetic waves

Doppler shift and aberration for spherical electromagnetic waves Doppler shift and aberration for spherical electromagnetic waves Teimuraz Bregadze tebr50@yahoo.com Spherical wave vs. plane wave approximation to the nature of the electromagnetic waves in regard to the

More information

The appearance, apparent speed, and removal of optical effects for relativistically moving objects

The appearance, apparent speed, and removal of optical effects for relativistically moving objects The appearance apparent speed and removal of optical effects for relativistically moving objects Robert J. Deissler a) Physics Department Cleveland State University Cleveland Ohio 44115 Received 6 September

More information

Special relativity and light RL 4.1, 4.9, 5.4, (6.7)

Special relativity and light RL 4.1, 4.9, 5.4, (6.7) Special relativity and light RL 4.1, 4.9, 5.4, (6.7) First: Bremsstrahlung recap Braking radiation, free-free emission Important in hot plasma (e.g. coronae) Most relevant: thermal Bremsstrahlung What

More information

Special Theory of Relativity. PH101 Lec-3

Special Theory of Relativity. PH101 Lec-3 Special Theory of Relativity PH101 Lec-3 Clock Synchronization In order to measure the time at which an event occurred at a point in space, we assumed that all of space are filled with clocks, one for

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

Relativistic Effects. 1 Introduction

Relativistic Effects. 1 Introduction Relativistic Effects 1 Introduction 10 2 6 The radio-emitting plasma in AGN contains electrons with relativistic energies. The Lorentz factors of the emitting electrons are of order. We now know that the

More information

8.20 MIT Introduction to Special Relativity IAP 2005 Tentative Outline

8.20 MIT Introduction to Special Relativity IAP 2005 Tentative Outline 8.20 MIT Introduction to Special Relativity IAP 2005 Tentative Outline 1 Main Headings I Introduction and relativity pre Einstein II Einstein s principle of relativity and a new concept of spacetime III

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

Talking about general relativity Important concepts of Einstein s general theory of relativity. Øyvind Grøn Berlin July 21, 2016

Talking about general relativity Important concepts of Einstein s general theory of relativity. Øyvind Grøn Berlin July 21, 2016 Talking about general relativity Important concepts of Einstein s general theory of relativity Øyvind Grøn Berlin July 21, 2016 A consequence of the special theory of relativity is that the rate of a clock

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

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

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

ENTER RELATIVITY THE HELIOCENTRISM VS GEOCENTRISM DEBATE ARISES FROM MATTER OF CHOOSING THE BEST REFERENCE POINT. GALILEAN TRANSFORMATION 8/19/2016

ENTER RELATIVITY THE HELIOCENTRISM VS GEOCENTRISM DEBATE ARISES FROM MATTER OF CHOOSING THE BEST REFERENCE POINT. GALILEAN TRANSFORMATION 8/19/2016 ENTER RELATIVITY RVBAUTISTA THE HELIOCENTRISM VS GEOCENTRISM DEBATE ARISES FROM MATTER OF CHOOSING THE BEST REFERENCE POINT. GALILEAN TRANSFORMATION The laws of mechanics must be the same in all inertial

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

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

The Lorentz Transformations

The Lorentz Transformations The Lorentz Transformations Michael Fowler, UVa Physics. /6/08 Problems with the Galilean Transformations We have already seen that Newtonian mechanics is invariant under the Galilean transformations relating

More information

Prelims 1997 Question 6

Prelims 1997 Question 6 Prelims 1997 Question 6 Write down the Lorentz transformations and use them to derive the expressions describing the phenomena of Lorentz contraction and time dilation. [5] The Prime Minister plans a quiet

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

Recap Lecture + Thomson Scattering. Thermal radiation Blackbody radiation Bremsstrahlung radiation

Recap Lecture + Thomson Scattering. Thermal radiation Blackbody radiation Bremsstrahlung radiation Recap Lecture + Thomson Scattering Thermal radiation Blackbody radiation Bremsstrahlung radiation LECTURE 1: Constancy of Brightness in Free Space We use now energy conservation: de=i ν 1 da1 d Ω1 dt d

More information

Unit- 1 Theory of Relativity

Unit- 1 Theory of Relativity Unit- 1 Theory of Relativity Frame of Reference The Michelson-Morley Experiment Einstein s Postulates The Lorentz Transformation Time Dilation and Length Contraction Addition of Velocities Experimental

More information

Observational Appearance of Black Hole Wind Effect of Electron Scattering

Observational Appearance of Black Hole Wind Effect of Electron Scattering Observational Appearance of Black Hole Wind Effect of Electron Scattering Kazuyuki OGURA Astronomical Institute Osaka Kyoiku Univ. 29 Jun 2013 Meeting of BH Horizon Project @Nagoya Univ. Contents Introduction

More information

Chapter 1. Relativity 1

Chapter 1. Relativity 1 Chapter 1 Relativity 1 Classical Relativity inertial vs noninertial reference frames Inertial Reference Frames Galilean transformation: x = x vt; y = y; z = z; t = t u x = u x v; u y = u y ; u z = u z

More information

Relativity. An explanation of Brownian motion in terms of atoms. An explanation of the photoelectric effect ==> Quantum Theory

Relativity. An explanation of Brownian motion in terms of atoms. An explanation of the photoelectric effect ==> Quantum Theory Relativity Relativity In 1905 Albert Einstein published five articles in Annalen Der Physik that had a major effect upon our understanding of physics. They included:- An explanation of Brownian motion

More information

CHAPTER 2 Special Theory of Relativity-part 1

CHAPTER 2 Special Theory of Relativity-part 1 CHAPTER 2 Special Theory of Relativity-part 1 2.1 The Apparent Need for Ether 2.2 The Michelson-Morley Experiment 2.3 Einstein s Postulates 2.4 The Lorentz Transformation 2.5 Time Dilation and Length Contraction

More information

Physics 2D Lecture Slides Lecture 4. April 3, 2009

Physics 2D Lecture Slides Lecture 4. April 3, 2009 Physics 2D Lecture Slides Lecture 4 April 3, 2009 Synchronizing Clocks Sam v Sally After coincidence of their origins at t=0, t = 0 Sam and Sally agree to send light signals to each other after time t

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

Physics 2D Lecture Slides Oct 1. Vivek Sharma UCSD Physics

Physics 2D Lecture Slides Oct 1. Vivek Sharma UCSD Physics Physics D Lecture Slides Oct 1 Vivek Sharma UCSD Physics Einstein s Special Theory of Relativity Einstein s Postulates of SR The laws ofphysics must be the same in all inertial reference frames The speed

More information

Physics 2D Lecture Slides Lecture 3. January 8, 2010

Physics 2D Lecture Slides Lecture 3. January 8, 2010 Physics 2D Lecture Slides Lecture 3 January 8, 2010 Immediate Consequences of Einstein s Postulates: Recap Events that are simultaneous for one Observer are not simultaneous for another Observer in relative

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

2.3 The Lorentz Transformation Eq.

2.3 The Lorentz Transformation Eq. Announcement Course webpage http://highenergy.phys.ttu.edu/~slee/2402/ Textbook PHYS-2402 Lecture 3 HW1 (due 9/13) Chapter 2 20, 26, 36, 41, 45, 50, 51, 55, 58 Sep. 6, 2016 2.3 The Lorentz Transformation

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

Physics 2D Lecture Slides Jan 10. Vivek Sharma UCSD Physics

Physics 2D Lecture Slides Jan 10. Vivek Sharma UCSD Physics Physics D Lecture Slides Jan 10 Vivek Sharma UCSD Physics Time Dilation Example: Relativistic Doppler Shift Light : velocity c = f λ, f=1/t A source of light S at rest Observer S approches S with velocity

More information

arxiv:physics/ v1 [physics.pop-ph] 7 Dec 2005

arxiv:physics/ v1 [physics.pop-ph] 7 Dec 2005 arxiv:physics/0512054v1 [physics.pop-ph] 7 Dec 2005 GAMOW S BICYCLE: THE APPEARANCE OF BODIES AT RELATIVISTIC SPEEDS AND APPARENT SUPERLUMINAL VELOCITIES ANDRZEJ NOWOJEWSKI Abstract. A human creates an

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

Two postulates Relativity of simultaneity Time dilation; length contraction Lorentz transformations Doppler effect Relativistic kinematics

Two postulates Relativity of simultaneity Time dilation; length contraction Lorentz transformations Doppler effect Relativistic kinematics Two postulates Relativity of simultaneity Time dilation; length contraction Lorentz transformations Doppler effect Relativistic kinematics Phys 2435: Chap. 37, Pg 1 Two postulates New Topic Phys 2435:

More information

E & M Qualifier. January 11, To insure that the your work is graded correctly you MUST:

E & M Qualifier. January 11, To insure that the your work is graded correctly you MUST: E & M Qualifier 1 January 11, 2017 To insure that the your work is graded correctly you MUST: 1. use only the blank answer paper provided, 2. use only the reference material supplied (Schaum s Guides),

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

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

in Electromagnetics Numerical Method Introduction to Electromagnetics I Lecturer: Charusluk Viphavakit, PhD

in Electromagnetics Numerical Method Introduction to Electromagnetics I Lecturer: Charusluk Viphavakit, PhD 2141418 Numerical Method in Electromagnetics Introduction to Electromagnetics I Lecturer: Charusluk Viphavakit, PhD ISE, Chulalongkorn University, 2 nd /2018 Email: charusluk.v@chula.ac.th Website: Light

More information

Gravity and action at a distance

Gravity and action at a distance Gravitational waves Gravity and action at a distance Newtonian gravity: instantaneous action at a distance Maxwell's theory of electromagnetism: E and B fields at distance D from charge/current distribution:

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

SPECIAL RELATIVITY. Introduction:

SPECIAL RELATIVITY. Introduction: SPECIAL RELATIVITY Introduction: When Mr. La Rosa started talking about relativity in class, I first was lost and didn t get the idea. At That time I was thinking of a subject for my project. I thought

More information

Announcements. Muon Lifetime. Lecture 4 Chapter. 2 Special Relativity. SUMMARY Einstein s Postulates of Relativity: EXPERIMENT

Announcements. Muon Lifetime. Lecture 4 Chapter. 2 Special Relativity. SUMMARY Einstein s Postulates of Relativity: EXPERIMENT Announcements HW1: Ch.2-20, 26, 36, 41, 46, 50, 51, 55, 58, 63, 65 Lab start-up meeting with TA tomorrow (1/26) at 2:00pm at room 301 Lab manual is posted on the course web *** Course Web Page *** http://highenergy.phys.ttu.edu/~slee/2402/

More information

Superluminal motion in the quasar 3C273

Superluminal motion in the quasar 3C273 1 Superluminal motion in the quasar 3C273 The cowboys have a way of trussing up a steer or a pugnacious bronco which fixes the brute so that it can neither move nor think. This is the hog-tie, and it is

More information

Massachusetts Institute of Technology Physics Department

Massachusetts Institute of Technology Physics Department Massachusetts Institute of Technology Physics Department Physics 8.0 IAP 005 Introduction to Special Relativity Midterm Exam Solutions. (a). The laws of physics should take the same form in all inertial

More information

General relativity, 3

General relativity, 3 General relativity, 3 Gravity as geometry: part II Even in a region of space-time that is so small that tidal effects cannot be detected, gravity still seems to produce curvature. he argument for this

More information

I ν. di ν. = α ν. = (ndads) σ ν da α ν. = nσ ν = ρκ ν

I ν. di ν. = α ν. = (ndads) σ ν da α ν. = nσ ν = ρκ ν Absorption Consider a beam passing through an absorbing medium. Define the absorption coefficient, α ν, by ie the fractional loss in intensity in travelling a distance ds is α ν ds (convention: positive

More information

Consequences of special relativity.

Consequences of special relativity. PHYS419 Lecture 12 Consequences of special relativity 1 Consequences of special relativity. The length of moving objects. Recall that in special relativity, simultaneity depends on the frame of reference

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

The Problem of Slow-witted Aliens, or. The Transverse Doppler Effect Simply Explained

The Problem of Slow-witted Aliens, or. The Transverse Doppler Effect Simply Explained The Problem of Slow-witted Aliens, or The Transverse Doppler Effect Simply Explained Vadim Matvejev 1, Oleg Matvejev 2 1-Jun-2016 Abstract The subject of this article is the dependence of observation results

More information

Massachusetts Institute of Technology Physics Department Physics 8.20 IAP 2005 Introduction to Special Relativity

Massachusetts Institute of Technology Physics Department Physics 8.20 IAP 2005 Introduction to Special Relativity Massachusetts Institute of Technology Physics Department Physics 8.20 IAP 2005 Introduction to Special Relativity Problem Set 1 1. Speeds What fraction of the speed of light does each of the following

More information

The Other Meaning of Special Relativity

The Other Meaning of Special Relativity The Other Meaning of Special Relativity Robert A. Close* ABSTRACT Einstein s special theory of relativity postulates that the speed of light is a constant for all inertial observers. This postulate can

More information

JRE Group of Institutions ASSIGNMENT # 1 Special Theory of Relativity

JRE Group of Institutions ASSIGNMENT # 1 Special Theory of Relativity ASSIGNMENT # 1 Special Theory of Relativity 1. What was the objective of conducting the Michelson-Morley experiment? Describe the experiment. How is the negative result of the experiment interpreted? 2.

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

Derivation of Special Theory of Relativity from Absolute Inertial Reference Frame

Derivation of Special Theory of Relativity from Absolute Inertial Reference Frame Derivation of Special Theory of Relativity from Absolute Inertial Reference Frame: Michelson-Morley Experiment, Lorentz Contraction, Transverse Doppler Red-Shift, Time Dilation Justin Lee October 8 th,

More information

Consequences of special relativity.

Consequences of special relativity. PHYS419 Lecture 12 Consequences of special relativity 1 Consequences of special relativity. The length of moving objects. Recall that in special relativity, simultaneity depends on the frame of reference

More information

Notes on x-ray scattering - M. Le Tacon, B. Keimer (06/2015)

Notes on x-ray scattering - M. Le Tacon, B. Keimer (06/2015) Notes on x-ray scattering - M. Le Tacon, B. Keimer (06/2015) Interaction of x-ray with matter: - Photoelectric absorption - Elastic (coherent) scattering (Thomson Scattering) - Inelastic (incoherent) scattering

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

Class 1: Special Relativity

Class 1: Special Relativity Class 1: Special Relativity In this class we will review some important concepts in Special Relativity, that will help us build up to the General theory Class 1: Special Relativity At the end of this session

More information

dt = p m, (2.1.1) dt = p

dt = p m, (2.1.1) dt = p Chapter 2 Special relativity 2.1 Galilean relativity We start our discussion of symmetries by considering an important example of an invariance, i.e. an invariance of the equations of motion under a change

More information

High-Energy Astrophysics

High-Energy Astrophysics Oxford Physics: Part C Major Option Astrophysics High-Energy Astrophysics Garret Cotter garret@astro.ox.ac.uk Office 756 DWB Michaelmas 2011 Lecture 9 Today s lecture: Black Holes and jets Part I Evidence

More information

Topics: Relativity: What s It All About? Galilean Relativity Einstein s s Principle of Relativity Events and Measurements

Topics: Relativity: What s It All About? Galilean Relativity Einstein s s Principle of Relativity Events and Measurements Chapter 37. Relativity Topics: Relativity: What s It All About? Galilean Relativity Einstein s s Principle of Relativity Events and Measurements The Relativity of Simultaneity Time Dilation Length g Contraction

More information

Chapter 2: The Special Theory of Relativity. A reference fram is inertial if Newton s laws are valid in that frame.

Chapter 2: The Special Theory of Relativity. A reference fram is inertial if Newton s laws are valid in that frame. Chapter 2: The Special Theory of Relativity What is a reference frame? A reference fram is inertial if Newton s laws are valid in that frame. If Newton s laws are valid in one reference frame, they are

More information

1st Year Relativity - Notes on Lectures 3, 4 & 5

1st Year Relativity - Notes on Lectures 3, 4 & 5 1st Year Relativity - Notes on Lectures 3, 4 & 5 Lecture Three 1. Now lets look at two very important consequences of the LTs, Lorentz-Fitzgerald contraction and time dilation. We ll start with time dilation.

More information

The Four-Frequency of Light. William O. Straub Pasadena, California June 28, 2014

The Four-Frequency of Light. William O. Straub Pasadena, California June 28, 2014 The Four-Frequency of Light William O. Straub Pasadena, Califnia 91104 June 28, 2014 Abstract A basic overview of the photon four-frequency is given, demonstrating its use in the explanation of the aberration

More information

CONSEQUENCES FOR SPECIAL RELATIVITY THEORY OF RESTORING EINSTEIN S NEGLECTED ADDITIVE CONSTANTS IN THE LORENTZ TRANSFORMATION

CONSEQUENCES FOR SPECIAL RELATIVITY THEORY OF RESTORING EINSTEIN S NEGLECTED ADDITIVE CONSTANTS IN THE LORENTZ TRANSFORMATION Fundamental J. Modern Physics, Vol. 2, Issue 2, 2011, Pages 139-145 Published online at http://www.frdint.com/ CONSEQUENCES FOR SPECIAL RELATIVITY THEORY OF RESTORING EINSTEIN S NEGLECTED ADDITIVE CONSTANTS

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

Introduction: Special Relativity

Introduction: Special Relativity Introduction: Special Relativity Observation: The speed c e.g., the speed of light is the same in all coordinate systems i.e. an object moving with c in S will be moving with c in S Therefore: If " r!

More information

Inflation, vacua and the end of the Universe

Inflation, vacua and the end of the Universe Inflation, 10 500 vacua and the end of the Universe Homework Problems: 1-7 (15 points) 1-10 (25 points) 2-9 (20 points) 2-13 (20 points) from Spacetime Physics Physics 311 Special Relativity Lecture 4:

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

Title. Author(s)OZAKI, Yuki. Issue Date Doc URL. Type. Additional There Information. File Information. Citationthe Physical Sciences )

Title. Author(s)OZAKI, Yuki. Issue Date Doc URL. Type. Additional There Information. File Information. Citationthe Physical Sciences ) itle Measurement in Berkeley's philosophy : from the view Author(s)OZAKI, Yuki 15th Congress of Methodology and Philosophy of Scien Citationthe Physical Sciences ) Issue Date 2015-08-04 Doc URL http://hdl.handle.net/2115/59658

More information

Modern Physics. Third Edition RAYMOND A. SERWAY CLEMENT J. MOSES CURT A. MOYER

Modern Physics. Third Edition RAYMOND A. SERWAY CLEMENT J. MOSES CURT A. MOYER Modern Physics Third Edition RAYMOND A. SERWAY CLEMENT J. MOSES CURT A. MOYER 1 RELATIVITY 1.1 Special Relativity 1.2 The Principle of Relativity, The Speed of Light 1.3 The Michelson Morley Experiment,

More information

Massachusetts Institute of Technology Department of Physics. Physics Out: Friday 29 September 2006 Due: Friday 6 October 2006.

Massachusetts Institute of Technology Department of Physics. Physics Out: Friday 29 September 2006 Due: Friday 6 October 2006. Massachusetts Institute of Technology Department of Physics Physics 8.033 Out: Friday 29 September 2006 Due: Friday 6 October 2006 Problem Set 4 Due: Friday 6 October 2006 at 4:00PM. Please deposit the

More information

Tuesday, February 15, Ice Cube Neutrino Facility

Tuesday, February 15, Ice Cube Neutrino Facility Ice Cube Neutrino Facility Semester Report This Thursday, Feb 17th, due in class: a list of resources (books, websites, articles, etc.), along with title. 1% will be deducted from your paper grade for

More information

Chapter 37. Relativity. PowerPoint Lectures for University Physics, 14th Edition Hugh D. Young and Roger A. Freedman Lectures by Jason Harlow

Chapter 37. Relativity. PowerPoint Lectures for University Physics, 14th Edition Hugh D. Young and Roger A. Freedman Lectures by Jason Harlow Chapter 37 Relativity PowerPoint Lectures for University Physics, 14th Edition Hugh D. Young and Roger A. Freedman Lectures by Jason Harlow Learning Goals for Chapter 37 Looking forward at why different

More information

Relativistic Kinematics

Relativistic Kinematics PH0008 Quantum Mechanics and Special Relativity Lecture 8 (Special Relativity) Relativistic Kinematics Velocities in Relativistic Frames & Doppler Effect Prof Department of Physics Brown University Main

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

Special Theory of Relativity. PH101 Lec-2

Special Theory of Relativity. PH101 Lec-2 Special Theory of Relativity PH101 Lec-2 Newtonian Relativity! The transformation laws are essential if we are to compare the mathematical statements of the laws of physics in different inertial reference

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

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

Announcement. Einstein s Postulates of Relativity: PHYS-3301 Lecture 3. Chapter 2. Sep. 5, Special Relativity

Announcement. Einstein s Postulates of Relativity: PHYS-3301 Lecture 3. Chapter 2. Sep. 5, Special Relativity Announcement PHYS-3301 Lecture 3 Sep. 5, 2017 2 Einstein s Postulates of Relativity: Chapter 2 Special Relativity 1. Basic Ideas 6. Velocity Transformation 2. Consequences of Einstein s Postulates 7. Momentum

More information

Einstein s Relativity and Black Holes

Einstein s Relativity and Black Holes Einstein s Relativity and Black Holes Guiding Questions 1. What are the two central ideas behind Einstein s special theory of relativity? 2. How do astronomers search for black holes? 3. In what sense

More information

Covariant Electromagnetic Fields

Covariant Electromagnetic Fields Chapter 8 Covariant Electromagnetic Fields 8. Introduction The electromagnetic field was the original system that obeyed the principles of relativity. In fact, Einstein s original articulation of relativity

More information

Electrodynamics of Radiation Processes

Electrodynamics of Radiation Processes Electrodynamics of Radiation Processes 7. Emission from relativistic particles (contd) & Bremsstrahlung http://www.astro.rug.nl/~etolstoy/radproc/ Chapter 4: Rybicki&Lightman Sections 4.8, 4.9 Chapter

More information

Einstein for Everyone Lecture 2: Background to Special Relativity

Einstein for Everyone Lecture 2: Background to Special Relativity Einstein for Everyone Lecture 2: Background to Special Relativity Dr. Erik Curiel Munich Center For Mathematical Philosophy Ludwig-Maximilians-Universität 1 Special Relativity 2 Principle of Relativity

More information

Tech Notes 4 and 5. Let s prove that invariance of the spacetime interval the hard way. Suppose we begin with the equation

Tech Notes 4 and 5. Let s prove that invariance of the spacetime interval the hard way. Suppose we begin with the equation Tech Notes 4 and 5 Tech Notes 4 and 5 Let s prove that invariance of the spacetime interval the hard way. Suppose we begin with the equation (ds) 2 = (dt) 2 (dx) 2. We recall that the coordinate transformations

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 - 6 Length Contraction and Time Dilation (Refer Slide Time: 00:29) In our last lecture,

More information

Welcome back to PHY 3305

Welcome back to PHY 3305 Welcome back to PHY 3305 Today s Lecture: Consequences of Einstein s Postulates Lorentz Transformations Albert Einstein 1879-1955 Einstein s Postulates: 1. The laws of physics are invariant to observers

More information

Physics PhD Qualifying Examination Part I Wednesday, August 26, 2015

Physics PhD Qualifying Examination Part I Wednesday, August 26, 2015 Physics PhD Qualifying Examination Part I Wednesday, August 26, 2015 Name: (please print) Identification Number: STUDENT: Designate the problem numbers that you are handing in for grading in the appropriate

More information

Interstellar Medium Physics

Interstellar Medium Physics Physics of gas in galaxies. Two main parts: atomic processes & hydrodynamic processes. Atomic processes deal mainly with radiation Hydrodynamics is large scale dynamics of gas. Start small Radiative transfer

More information

Modelling the Big Bang with True Relativity

Modelling the Big Bang with True Relativity Modelling the Big Bang with True Relativity copyright 2007 Tony Stanton Abstract This paper is based on the theory of True Relativity to view spacetime using simple geometry and represents a paradigm shift

More information

Rotational Behavior of Einsteinian Space

Rotational Behavior of Einsteinian Space Rotational Behavior of Einsteinian Space Ling Jun Wang Published in IL Nuovo Cimento, Vol. 5B, N.6, pp65-624, 2 Department of Physics, Geology and Astronomy University of Tennessee at Chattanooga Chattanooga,

More information

Relativity and Quantum Electrodynamics in the Theory of Reference Frames: the Origin of Physical Time

Relativity and Quantum Electrodynamics in the Theory of Reference Frames: the Origin of Physical Time Relativity and Quantum Electrodynamics in the Theory of Reference Frames: the Origin of Physical Time Abstract Daniele Sasso * In this paper the main aspects of the Theory of Reference Frames are presented:

More information

We search for the ether. Next time: The ether is missing Conspiracy? I think not!

We search for the ether. Next time: The ether is missing Conspiracy? I think not! We search for the ether Next time: The ether is missing Conspiracy? I think not! Waves Wave phenomena are important for the development of special relativity and for understanding quantum mechanics, so

More information

- Synchrotron emission: A brief history. - Examples. - Cyclotron radiation. - Synchrotron radiation. - Synchrotron power from a single electron

- Synchrotron emission: A brief history. - Examples. - Cyclotron radiation. - Synchrotron radiation. - Synchrotron power from a single electron - Synchrotron emission: A brief history - Examples - Cyclotron radiation - Synchrotron radiation - Synchrotron power from a single electron - Relativistic beaming - Relativistic Doppler effect - Spectrum

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

Lecture 10: General Relativity I

Lecture 10: General Relativity I Lecture 10: General Relativity I! Recap: Special Relativity and the need for a more general theory! The strong equivalence principle! Gravitational time dilation! Curved space-time & Einstein s theory

More information

The Theory of Relativity

The Theory of Relativity The Theory of Relativity Lee Chul Hoon chulhoon@hanyang.ac.kr Copyright 2001 by Lee Chul Hoon Table of Contents 1. Introduction 2. The Special Theory of Relativity The Galilean Transformation and the Newtonian

More information

X Rays must be viewed from space used for detecting exotic objects such as neutron stars and black holes also observing the Sun.

X Rays must be viewed from space used for detecting exotic objects such as neutron stars and black holes also observing the Sun. 6/25 How do we get information from the telescope? 1. Galileo drew pictures. 2. With the invention of photography, we began taking pictures of the view in the telescope. With telescopes that would rotate

More information

FIBER OPTICS. Prof. R.K. Shevgaonkar. Department of Electrical Engineering. Indian Institute of Technology, Bombay. Lecture: 15. Optical Sources-LASER

FIBER OPTICS. Prof. R.K. Shevgaonkar. Department of Electrical Engineering. Indian Institute of Technology, Bombay. Lecture: 15. Optical Sources-LASER FIBER OPTICS Prof. R.K. Shevgaonkar Department of Electrical Engineering Indian Institute of Technology, Bombay Lecture: 15 Optical Sources-LASER Fiber Optics, Prof. R.K. Shevgaonkar, Dept. of Electrical

More information