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Relativity Made Relatively Easy

✍ Scribed by Andrew M. Steane


Publisher
Oxford University Press, USA
Year
2012
Tongue
English
Leaves
436
Category
Library

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✦ Synopsis


Offers a thorough treatment suitable for any undergraduate course on relativity
Clear and careful explanations
Profound insights into many wonderful physical phenomena
Richly illustrated
Opens up General Relativity with precision but without the need for tensor analysis
Relativity Made Relatively Easy presents an extensive study of Special Relativity and a gentle (but exact) introduction to General Relativity for undergraduate students of physics. Assuming almost no prior knowledge, it allows the student to handle all the Relativity needed for a university course, with explanations as simple, thorough, and engaging as possible.

The aim is to make manageable what would otherwise be regarded as hard; to make derivations as simple as possible and physical ideas as transparent as possible. Lorentz invariants and four-vectors are introduced early on, but tensor notation is postponed until needed. In addition to the more basic ideas such as Doppler effect and collisions, the text introduces more advanced material such as radiation from accelerating charges, Lagrangian methods, the stress-energy tensor, and introductory General Relativity, including Gaussian curvature, the Schwarzschild solution, gravitational lensing, and black holes. A second volume will extend the treatment of General Relativity somewhat more thoroughly, and also introduce Cosmology, spinors, and some field theory.

Readership: Physics students at the undergraduate and beginning graduate level.

✦ Table of Contents


Cover

S Title

Relativity Made Relatively Easy

Copyright

 Andrew M. Steane 2012

 ISBN 978-0-19-966285-2 (hbk)

 ISBN 978-0-19-966286-9 (pbk)

Dedication

Preface

Acknowledgements

Contents

Part I The relativistic world

 1  Basic ideas

      1.1 Newtonian physics

      1.2 Special Relativity

           1.2.1 The Postulates of Special Relativity

           1.2.2 Central ideas about spacetime

      1.3 Matrix methods

      1.4 Spacetime diagrams

      exercises

 2  The Lorentz transformation

      2.1 Introducing the Lorentz transformation

           2.1.1 Derivation of Lorentz transformation

      2.2 Velocities

      2.3 Lorentz invariance and 4-vectors

           2.3.1 Rapidity

      2.4 Lorentz-invariant quantities

      2.5 Basic 4-vectors

           2.5.1 Proper time

           2.5.2 Velocity, acceleration

           2.5.3 Momentum, energy

           2.5.4 The direction change of a 4-vector under a boost

           2.5.5 Force

           2.5.6 Wave vector

      2.6 The joy of invariants

      2.7 Summary

      Exercises

 3  Moving light sources

      3.1 The Doppler effect

      3.2 Aberration and the headlight effect

           3.2.1 Stellar aberration

      3.3 Visual appearances

      Exercises

 4  Dynamics

      4.1 Force

           4.1.1 Transformation of force

      4.2 Motion under a pure force

           4.2.1 Linear motion and rapidity

           4.2.2 Hyperbolic motion: the `relativistic rocket'

           4.2.3 4-vector treatment of hyperbolic motion

           4.2.4 Motion under a constant force

           4.2.5 Circular motion

           4.2.6 Motion under a central force

           4.2.7 (An) harmonic motion

      Exercises

 5  The conservation of energy-momentum

      5.1 Elastic collision, following Lewis and Tolman

      5.2 Energy-momentum conservation using 4-vectors

           5.2.1 Mass-energy equivalence

      5.3 Collisions

           5.3.1 'Isolate and square

      5.4 Elastic collisions

           5.4.1 Billiards

           5.4.2 Compton scattering

           5.4.3 More general treatment of elastic collisions

      5.5 Composite systems

      5.6 Energy flux, momentum density, and force

      Exercises

 6  Further kinematics

      6.1 The Principle of Most Proper Time

      6.2 Four-dimensional gradient

      6.3 Current density, continuity

      6.4 Wave motion

           6.4.1 Wave equation

           6.4.2 Particles and waves

           6.4.3 Group velocity and particle velocity

      6.5 Acceleration and rigidity

           6.5.1 The great train disaster

           6.5.2 Lorentz contraction and internal stress

      6.6 General Lorentz boost

      6.7 Lorentz boosts and rotations

           6.7.1 Two boosts at right angles

           6.7.2 The Thomas precession

           6.7.3 Analysis of circular motion

      6.8 Generators of boosts and rotations

      6.9 The Lorentz group*

           6.9.1 Further group terminology

      Exercises

 7  Relativity and electromagnetism

      7.1 Definition of electric and magnetic fields

           7.1.1 Transformation of the fields (first look)

      7.2 Maxwell's equations

           7.2.1 Moving capacitor plates

      7.3 The fields due to a moving point charge

      7.4 Covariance of Maxwell's equations

           7.4.1 Transformation of the fields: 4-vector method*

      7.5 Introducing the Faraday tensor

           7.5.1 Tensors

           7.5.2 Application to electromagnetism

      Exercises

 8  Electromagnetic radiation

      8.1 Plane waves in vacuum

      8.2 Solution of Maxwell's equations for a given charge distribution

           8.2.1 The 4-vector potential of a uniformly moving point charge

           8.2.2 The general solution

           8.2.3 The Lienard-Wierhert potentials

           8.2.4 The field of an arbitrarily moving charge

           8.2.5 Two example fields

      8.3 Radiated power

           8.3.1 Linear and circular motion

           8.3.2 Angular distribution

      Exercises

Part II An Introduction to General Relativity

 9  The Principle of Equivalence

      9.1 Flee fall

           9.1.1 Free fall or free float?

           9.1.2 weak Principle of Equivalence

           9.1.3 The Eotvas-Pekar-Fekete experiment

           9.1.4 The Strong Equivalence Principle

           9.1.5 Falling light and gravitational time dilation

      9.2 The uniformly accelerating reference frame

           9.2.1 Accelerated rigid motion

           9.2.2 Rigid constantly accelerating frame

      9.3 Newtonian gravity from the Principle of Most Proper Time

      9.4 Gravitational redshift and energy conservation

           9.4.1 Equation of motion

      Exercises

 10  Warped spacetime

      10.1 Two-dimensional spatial surfaces

           10.1.1 Conformal flatness

      10.2 Three spatial dimensions

      10.3 Time and space together

      10.4 Gravity and curved spacetime

      Exercises

 11  Physics from the metric

      11.1 Example exact solutions

           11.1.1 The acceleration due to gravity

      11.2 Schwarzschild metric: basic properties

      11.3 Geometry of Schwarzschild solution

           11.3.1 Radial motion

           11.3.2 Circular orbits

           11.3.4 Photon orbits

           11.3.5 Shapiro time delay

      11.4 Gravitational lensing

      11.5 Black holes

           1.5.1 Horison

           11.5.2 Energy near an horizon

      11.6 What next?

           11.6.1 Black-hole thermodynamics

      Exercises

Part III Further Special Relativity

 12  Tensors and index notation

      12.1 Index notation in a nutshell

      12.2 Tensor analysis

           12.2.1 Rules for tensor algeb

           12.2.2 Contravariant and covariant

           12.2.3 Useful methods and ideas

           12.2.4 Parity inversion and the vector product

           12.2.5 Differentiation

      12.3 Antisymmetric tensors and the dual

      Exercises

 13  Rediscovering electromagnetism

      13.1 Fundamental equations

      13.2 Invariants of the electromagnetic field

           13.2.1 Motion of particles in an electromagnetic field

      Exercises

 14  Lagrangian mechanics

      14.1 Classical Lagrangian mechanics

      14.2 Relativistic motion

           14.2.1 From classical Euler-Lagrange

           14.2.2 Manifestly covaria

      14.3 Conservation

      14.4 Equation of motion in General Relativity

      Exercises

 15  Angular momentum

      15.1 Conservation of angular momentum

      15.2 Spin

           15.2.1 Introducing spin

           15.2.2 Paull-Lubanski vector

           15.2.3 Thomas precesion revisited

           15.2.4 Precession of the spin of a charged particle

      Exercises

 16  Energy density

      16.1 Introducing the stress-energy tensor

           16.1.1 Transport of energy and momentum

           16.1.2 Ideal fluid

      16.2 Stress-energy tensor for an arbitrary system

           16.2.1 Interpreting the terms

      16.3 Conservation of energy and momentum for a fluid

      16.4 Electromagnetic energy and momentum

           16.4.1 Examples of energy density and energy flow

           16.4.2 Field momentum

           16.4.3 Stress-energy tensor of the electromagnetic field

      16.5 Field and matter pushing on one another

           16.5.1 Resolution of the `4/3 problem' and the origin of mass

      Exercises

 17  What is spacetime?

A Some basic arguments

 A.1 Early experiments

 A.2 Simultaneity and radar coordinates

 A.3 Proper time and time dilation

 A.4 Lorentz contraction

 A.5 Doppler effect, addition of velocities

B Constants and length scales

C Derivatives and index notation

D The field of an arbitrarily moving charge

 D.1 Light-cone volume element

 D.2 The field tensor

Bibliography

Index


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