Physics 214: Special Relativity. An Introduction

Similar documents
Physics 171: General Relativity. An Introduction

Einstein for Everyone Lecture 2: Background to Special Relativity

Newton s First Law of Motion

The Philosophy of Physics. Is Space Absolute or Relational?

Topics for today. Galileo s Physics Newton s philosophy & physics How to test a theory

Simultaneity and Light Propagation in the context of the Galilean Principle of Relativity

Astronomy 2 Special Relativity Part 2 The axioms

The relativity and equivalence principles for self-gravitating systems

Special Relativity. Mário Pimenta Udine, September 2009

06. The Aristotelian Tradition

Perfect Symmetries. Abstract. use to represent them. An empirical symmetry is perfect if and only if any two situations it relates

Tuesday, February 15, Ice Cube Neutrino Facility

Question from last week

Einstein s Space and Time

Special Theory of Relativity. PH101 Lec-2

arxiv: v2 [physics.hist-ph] 15 Jun 2014

The Problem of Slowing Clocks in Relativity Theory

5-1. Chapter 5 GALILEO S SENSORY AND EMPIRICAL CONCEPTS OF RELATIVITY. A. Galileo s Relativity

Might have Minkowski discovered the cause of gravity before Einstein? Vesselin Petkov Minkowski Institute Montreal, Canada

Special Theory of Relativity. A Brief introduction

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

Physics 110. Electricity and Magnetism. Professor Dine. Spring, Handout: Vectors and Tensors: Everything You Need to Know

2.1 The Ether and the Michelson-Morley Experiment

We saw last time how the development of accurate clocks in the 18 th and 19 th centuries transformed human cultures over the world.

Special Relativity - QMII - Mechina

Aristotle: If a man on top of a mast in a moving ship drops an object, it would fall toward the back of the ship.

Lecture 12: Arguments for the absolutist and relationist views of space

NEWTON S LAWS OF MOTION. Review

Redhound Day 2 Assignment (continued)

Covariant Formulation of Electrodynamics

Newton s Laws of Motion. Steve Case NMGK-8 University of Mississippi October 2005

Relativistic Dynamics

THE HIGGS BOSON AND THE SPACETIME METRIC (Revised June, 2016) JOHN A. GOWAN

Light and Relativity

Space, Time and Simultaneity

Higgs Field and Quantum Gravity

A Revolution in Space and Time: Einstein's Special Relativity. LIGO-G Z Francesco Fidecaro

Dynamics and Relativity

Relativity as the quantum mechanics of space-time. measurements

PHILOSOPHY OF SPACE AND TIME various authors. Philosophy of space and time is the branch of philosophy concerned with the issues

Curved Spacetime... A brief introduction

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

A New Conception of Science

CHAPTER 2 Special Theory of Relativity Part 2

The Lorentz Transformation

The Lorentz Transformation

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

In defence of classical physics

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

General Physics I. Lecture 16: The Principles of the Theory of Relativity. Prof. WAN, Xin 万歆.

Chapter 11. Special Relativity

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

UNIT 1 MECHANICS PHYS:1200 LECTURE 2 MECHANICS (1)

Boscovich s theory: strict Newtonian physics, by Roger J. Anderton

Simply Einstein A Mini-Course in Relativity

Astronomy 102, Fall September 2009

Correct Resolution of the Twin Paradox

Unit- 1 Theory of Relativity

FRAME S : u = u 0 + FRAME S. 0 : u 0 = u À

Forces. A force is a push or a pull on an object

Module 2: Special Theory of Relativity - Basics

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

8.20 MIT Introduction to Special Relativity IAP 2005 Tentative Outline

Einstein for Everyone Lecture 3: Special Relativity

PHYS 340 ( From Atoms to the Universe ): SECTION A

Class 5: Equivalence Principle

ASTR 1010 Spring 2016 Study Notes Dr. Magnani

Limitations of Newtonian Physics

Figure 5.1: Force is the only action that has the ability to change motion. Without force, the motion of an object cannot be started or changed.

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

Introduction. You know, it would be sufficient to really understand. If I can t picture it, I can t understand it.

The Principle of Relativity

Kepler problem and Lorentz transformations

Special Theory of Relativity. PH101 Lec-1 Soumitra Nandi

Bell s spaceship paradox

Today in Astronomy 102: relativity

Electromagnetic Fields. Lecture 2. Fundamental Laws

Lecture III : Jan 30, 2017

The result is; distances are contracted in the direction of motion.

Galilean velocity transformation

Introduction to Quantum Mechanics: Syllabus

Chapter 33 Special Relativity

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

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

These two lengths become equal when m is the Planck mass. And when this happens, they both equal the Planck length!

Relativity. Class 16 Prof J. Kenney June 18, boss

ALBERT EINSTEIN AND THE FABRIC OF TIME by Gevin Giorbran

From Quantum Mechanics to String Theory

General Relativity and Black Holes

Relativity. Transcript.

Astronomy 102 Lecture 04

Quantum Physics and General Relativity

AN INTRODUCTION TO LAGRANGE EQUATIONS. Professor J. Kim Vandiver October 28, 2016

The Constancy of the Speed of Light

Relativity. No Ether! Spacetime. Your bicycle cannot go as fast as light.

JF Theoretical Physics PY1T10 Special Relativity

Your (primed) frame frame

Light Quantum Hypothesis

SPECIAL RELATIVITY. Introduction:

Special Relativity. Frames of Reference. Introduction

Transcription:

Physics 214: Special Relativity An Introduction

Many books

Indices: Summation Convention Introduced in 1916 (with final formulation of GR). Repeated indices summed. Einstein joked I have made a great discovery in mathematics; I have suppressed the summation sign every time that the summation must be made over an index which occurs twice x i x i = x i x i

Features of Newton s Laws Action at a distance -- almost ghostly. A source of skepticism, initially; Newton was defensive about it. Equivalence of gravitational mass and inertial mass (Eotvos) Galilean Invariance

Galileo and Galilean Invariance Galileo on Relativity: Galileo Defends Copernicus Shut yourself up with some friend in the main cabin below decks on some large ship, and have with you there some flies, butterflies, and other small flying animals. Have a large bowl of water with some fish in it; hang up a bottle that empties drop by drop into a wide vessel beneath it. With the ship standing still, observe carefully how the little animals fly with equal speed to all sides of the cabin. The fish swim indifferently in all directions; the drops fall into the vessel beneath; and, in throwing something to your friend, you need throw it nor more strongly in one direction than another, the distances being equal; jumping with your feet together, you pass equal spaces in every direction. When you have observed all these things carefully, have the ship proceed with any speed you like, so long as the motion is uniform and not fluctuating this way and that. You will discover not the least change in all the effects named, nor could you tell from any of them whether the ship was moving or standing still.

Modern Description of Galilean Invariance

Not a feature of Maxwell s equations Speed of light just a constant Einstein s Problem With Galileo/Maxwell If I pursue a beam of light with the velocity c, I should observe such a beam of light as an electromagnetic field at rest though spatially oscillating. There is no such thing.

The fall of absolute time Newton: Newton on Absolute Time (Principia): Absolute, true and mathematical time, of itself and from its own nature, flows equably without relation to anything external Absolute space, in its own nature, without relation to anything stable, remains always similar and immovable. But: Absolute time is not an object of perception The Deity endures forever and is everywhere present, and by existing always and everywhere, He constitutes duration and space. And Mach (one of Einstein s early heroes): absolute time is a useless metaphysical concept, and cannot be produced in experience. Newton acted contrary to his expressed intention only to investigate actual facts. And Poincare Not only do we have no direct intuition of the equality of two times, we do not even have one of the simultaneity of two events occurring in different places. Poincare had much of the mathematics of special relativity, as did Lorentz, but neither made the final leap; they were too wedded to the ether concept.

Difference between Einstein and Poincare (Dyson) The essential difference between Poincare and Einstsein was that Poincare and Einstein was that Poincare was by temperament conservative and Einstein was by temperament revolutionary. When Poincare looked for a new theory of electromagnetism, he tried to preserve as much as he could of the old. He loved the ether and continued to believe in it, even when his own theory showed that it was unobservable. His version of relativity theory was a patchwork quilt. The new idea of local time, depending on the motion of the observer, was patched onto the old framework of absolute space and time defined by a rigid and immovable ether. Einstein, on the other hand, saw the old framework as cumbersome and unnecessary and was delighted to be rid of it All the complicated explanations of electric and magnetic forces as elastic stresses in the ether could be swept into the dustbin of history, together with the famous old professors who still believed in them.

Special Relativity Einstein: realized that the symmetry of Maxwell s equations is not Galilean invariance, but Lorentz invariance argues this is what should be taken seriously. [Demise of action at a distance] Indices again: Upstairs/downstairs: Einstein borrowed, it seems, from mathematicians: Following Ricci and Levi-Civita, we denote the contravariant character in such a way that we place the index in the upper position But other notational improvements only came later. In this way, Maxwell s equations look simple:

Maxwell s Equations in Relativistic Form

Einstein on Maxwell and the field concept A new concept appeared in physics, the most important invention since Newton s time: the field. It needed great scientific imagination to realize that it is not the charges nor the particles but the field in the space between the charges and the particles that is essential for the description of physical phenomena. The field concept proved successful when it led to the formulation of Maxwell s equations describing the structure of the electromagnetic field.