Class 1: Special Relativity

Similar documents
8.20 MIT Introduction to Special Relativity IAP 2005 Tentative Outline

CHAPTER 2 Special Theory of Relativity-part 1

Therefore F = ma = ma = F So both observers will not only agree on Newton s Laws, but will agree on the value of F.

Special Relativity: Derivations

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

Special Relativity-General Discussion

Chapter 1. Relativity 1

Special Theory of Relativity (I) Newtonian (Classical) Relativity. Newtonian Principle of Relativity. Inertial Reference Frame.

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

Einstein Toolkit Workshop. Joshua Faber Apr

2.6 Invariance of the Interval

Special Relativity-General Discussion

Relativity. Overview & Postulates Events Relativity of Simultaneity. Relativity of Time. Relativity of Length Relativistic momentum and energy

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

Module 2: Special Theory of Relativity - Basics

Welcome back to PHY 3305

Introduction to Relativity & Time Dilation

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

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

College Physics B - PHY2054C. Special Relativity 11/10/2014. My Office Hours: Tuesday 10:00 AM - Noon 206 Keen Building.

Lecture 4 - Lorentz contraction and the Lorentz transformations

Newtonian or Galilean Relativity

Extra notes on rela,vity. Wade Naylor

Lecture Notes on Relativity. Last updated 10/1/02 Pages 1 65 Lectures 1 10

Special Relativity 05/09/2008. Lecture 14 1

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

The Foundations of Special Relativity

0 : Einstein s postulates of Special Relativity

Kinematics of special relativity

Postulates of Special Relativity

CHAPTER 2 Special Theory of Relativity

The Special Theory of relativity

Tuesday, February 15, Ice Cube Neutrino Facility

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

Inconsistencies in Special Relativity? Sagnac Effect and Twin Paradox

The Lorentz Transformations

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

Physics 2D Lecture Slides Lecture 2. Jan. 5, 2010

ASTR 1040 Recitation: Relativity

General Physics I. Lecture 18: Lorentz Transformation. Prof. WAN, Xin ( 万歆 )

Modern Physics Part 2: Special Relativity

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

dt = p m, (2.1.1) dt = p

Chapter 36 The Special Theory of Relativity. Copyright 2009 Pearson Education, Inc.

Class Notes Introduction to Relativity Physics 375R Under Construction

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

PH-101:Relativity and Quantum Mechanics

2.1 Einstein s postulates of Special Relativity. (i) There is no ether (there is no absolute system of reference).

E = mc 2. Inertial Reference Frames. Inertial Reference Frames. The Special Theory of Relativity. Slide 1 / 63. Slide 2 / 63.

Einstein and his theory of Special Relativity (1905) General relativity came later and deals more with gravity (1915) 07 relativity.

Final Review Prof. WAN, Xin

Physics 280 Lecture 2

The spacetime of special relativity

2.1 The Ether and the Michelson-Morley Experiment

Consequences of special relativity.

The True Nature of the Special Relativity Light Clock. Copyright 2012 Joseph A. Rybczyk

Special Relativity. Christopher R. Prior. Accelerator Science and Technology Centre Rutherford Appleton Laboratory, U.K.

Chapter 26 Special Theory of Relativity

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

Accelerated Observers

Consequences of special relativity.

The Lorentz Transformation

College Physics B - PHY2054C. Special & General Relativity 11/12/2014. My Office Hours: Tuesday 10:00 AM - Noon 206 Keen Building.

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

Spacetime and 4 vectors

Physics 2D Lecture Slides Lecture 2. March 31, 2009

Lecture 3 and 4. Relativity of simultaneity. Lorentz-Einstein transformations

Introduction to Covariant Formulation

Physics 2D Lecture Slides Sept 29. Vivek Sharma UCSD Physics

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

RELATIVITY. Einstein published two theories of relativity. In The Special Theory. For uniform motion a = 0. In The General Theory

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

Lecture 13 Notes: 07 / 20. Invariance of the speed of light

JF Theoretical Physics PY1T10 Special Relativity

Lorentz Transformations and Special Relativity

Superluminal motion in the quasar 3C273

CHAPTER 2 Special Theory of Relativity Part 2

Midterm Solutions. 1 1 = 0.999c (0.2)

General Physics I. Lecture 21: Relativistic Energy and Momentum. Prof. WAN, Xin ( 万歆 )

Special Theory of Relativity. A Brief introduction

2.4 The Lorentz Transformation

Special Relativity. Asaf Pe er The Michelson - Morley experiment

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

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

Before we work on deriving the Lorentz transformations, let's first look at the classical Galilean transformation.

Q W u e. c t o u m m e P h B. B e. s c i k c s 2. John Harris 1

Vectors in Special Relativity

Class Notes Introduction to Modern Physics Physics 321 Plan II Under Construction

Class Notes for Modern Physics, Part 1

General Physics I. Lecture 20: Lorentz Transformation. Prof. WAN, Xin ( 万歆 )

Massachusetts Institute of Technology Physics Department

Unit- 1 Theory of Relativity

RELATIVITY. The End of Physics? A. Special Relativity. 3. Einstein. 2. Michelson-Morley Experiment 5

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

= 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

Lecture 8 : Special Theory of Relativity

Particle Physics: Special Relativity

In special relativity, it is customary to introduce the dimensionless parameters 1

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

Gravitation: Special Relativity

Transcription:

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 you should be familiar with the basic ingredients of Special Relativity: reference/inertial frames, the Lorentz transformations, Einstein s postulate and its consequences understand the significance of the space-time interval ds # between two events be able to use space-time diagrams to describe some simple visualizations of events in space-time understand how the definitions of classical momentum and energy must be modified in Special Relativity

Reference frames How do we describe occurrences in nature? A reference frame is an informationgathering system consisting of a field of synchronized clocks on a coordinate grid http://www.pitt.edu/~jdnorton/teaching/hps_0410/chapters/special_relativity_principles An event is an occurrence with definite location/time

Reference frames The locations and times of events together form a 4D co-ordinate system known as space-time. https://xkcd.com/1524/

Inertial frames Some reference frames are special In an inertial frame, a freely-moving body (no external forces) moves with constant velocity Inertial frames move uniformly with respect to each other https://en.wikipedia.org/wiki/special_relativity

Inertial frames Some examples of non-inertial frames! https://www.thinglink.com/scene/877700809561735169 https://www.pinterest.com.au/bestonamusement/beston-frisbee-rides-for-sale-or-fairground-pendul/

Principle of relativity Laws of nature are identical in all inertial frames (mathematically, they have the same form in each frame s co-ordinate system) There is no such thing as absolute rest/velocity (Due to Galileo) https://owlcation.com/stem/what-were- Galileos-Contributions-to-Astronomy

Principle of relativity Example: Newton s Laws F = ma are invariant under the transformation v * t = v t + V./012302 Not true for non-inertial frames, in which we experience forces we cannot account for https://xkcd.com/123/

Transformations between frames If (t, x, y, z) are the co-ordinates of an event in frame S, what are its co-ordinates (t *, x *, y *, z * ) in frame S moving with speed v with respect to S? Galilean transformation: clocks in S and S run at the same rate (t * = t), and velocities add (u = u * + v)

The role of light https://brooklyntom ars.com/laser-beamfocus-352154e6acaf According to the Galilean transformation, the speed of light c slows down to c v in S This can be tested experimentally and is false (e.g. Michelson-Morley experiment) The Galilean transformation is inconsistent with electromagnetism

The role of light In classical physics, interactions are instantaneous (change in one thing instantaneously affects another) This is not true there is a finite maximum velocity at which interactions propagate, which turns out to be the speed of light c = 3 10 C m/s (large) https://www.ihkplus.de/das_ende_der_ketteninsolvenz.axcms Consequences: (1) bodies cannot move faster than c, (2) c is the same in all frames, (3) causality

The role of light The finite velocity at which signals can propagate is deeply connected to the idea of causality https://en.wikipedia.org/wiki/light_cone

Einstein s postulate Einstein s postulate (1905): the speed of light is the same in all inertial frames (regardless of the motion of the source/observer) The Galilean transformations are wrong! https://www.patana.ac.th/seco ndary/science/anrophysics/rela tivity_option/commentary.html

Lorentz transformations How should we transform the co-ordinates of events? Imagine sending out a light signal from the origin: In S: x # + y # + z # = (ct) # In S : x # + y # + z # = (ct ) #

Lorentz transformations These equations are satisfied by the Lorentz transformations: t = γ(t vx/c # ) x = γ(x vt) y = y z = z γ = t = γ(t * + vx /c # ) x = γ(x * + vt ) y = y z = z 1 1 v # /c #

Simultaneity The Lorentz transformations have some remarkable consequences First, consider two events that are simultaneous in S (t G = t # ). By the Lorentz transformations: t G * t # * = γv c # x # x G These events are not simultaneous in S! There is no such thing as absolute time, the order of events depends on the reference frame!

Length contraction Consider a stick at rest in S with ends at (x G *, x # * ) Observers in S measure its length by recording the end positions (x G, x # ) simultaneously in S. They find: x # x G = x # * x G * /γ The length of a moving object is contracted by γ https://www.slideshare.net/cscottthomas/ch-28-special-relativity-online-6897295

Time dilation A clock at the origin of S ticks at times (t * G, t * # ) The spacing of these ticks in S is: t # t G = γ t * * # t G A moving clock ticks at longer intervals https://patriceayme.wordpress. com/2014/06/17/time-dilation/

Space-time interval The Lorentz transformation has a special property for how the difference in the space-time co-ordinates of two events transform between S and S : c # t # + x # + y # + z # = c # t # + x # + y # + z # This combination is the space-time interval s 2 It is an invariant (has the same value in all frames)

Importance of invariants Invariants quantities which all observers agree to be the same are useful! In Euclidean geometry, the distance between 2 points is the same if you rotate co-ordinates The space-time interval in relativity (same in all inertial frames) is analogous to a distance in Euclidean geometry (same in all rotated frames) https://www.mathsisfun.com/algebra/distance-2-points.html

Classifying intervals The invariant space-time interval, s # = c # t # + x # + y # + z #, may be used to classify pairs of events Events for which s # < 0 are timelike ( time wins ) an inertial observer can pass through them both. The time between the events in this frame is the proper time τ Events for which s # > 0 are spacelike there s an inertial frame in which they are simultaneous. The separation between the events in this frame is the proper separation. Events for which s # = 0 are lightlike they occur along the same light ray

Relativistic momentum Conservation of momentum can be preserved if we modify the concept of the mass of a particle such that it depends on velocity m v = γm T = m T 1 v# c # We have introduced the rest mass m 0 As v 0 we recover classical momentum p = m T v

Relativistic energy Considering the work done on a particle VW the energy gained, we recover a modified expression for relativistic energy E = γm T c # = m Tc # 1 v# c # Particles have a rest energy m 0 c 2 V2 dx as As v 0 we find E = m T c # + G # m Tv # Mathematically we find: E # p # c # = m T c # #