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Black Holes : An Introduction

Thomas, Edwin; Raine, Derek
ISBN-10: 1848163827
ISBN-13: 9781848163829

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Preface
Relativistic Gravity
What is a black hole?
Why study black holes?
Elements of general relativity
The principle of equivalence
The Newtonian affine connection
Newtonian gravity
Metrics in relativity
The velocity and momentum 4-vector
General vectors and tensors
Locally measured physical quantities
Derivatives in relativity
Acceleration 4-vector
Paths of light
Einstein's field equations
Symmetry and Killing's equation
Spherical Black Holes
The Schwarzschild metric
Coordinates
Proper distance
Proper time
Redshift
Interpretation of M and geometric units
The Schwarzschild radius
The event horizon
Birkoff's theorem
Israel's theorem
Orbits in Newtonian gravity
Newtonian Energy
Angular momentum
The Newtonian effective potential
Classification of Newtonian orbits
Particle orbits in the Schwarzschild metric
Constants of the motion
Conserved Energy
Angular momentum
The effective potential
Newtonian approximation to the metric
Classification of orbits
Radial infall
The locally measured energy of a particle
Circular orbits
Comparison with Newtonian orbits
Orbital velocity in the frame of a hovering observer
Energy in the last stable orbit
Orbits of light rays
Radial propagation of light
Capture cross-section for light
The view of the sky for a stationary observer
Classical tests
Palling into a black hole
Free-fall time for a distant observer
Light-travel time
What the external observer sees
An infalling observer's time
What the infalling observer feels
Capture by a black hole
Case I: Capture of high angular momentum particles
Case II: Capture of low energy particles
Surface gravity of a black hole
The proper acceleration of a hovering observer
Surface gravity
Rindler coordinates
Other coordinates
Null coordinates
Eddington-Finkelstein coordinates
Inside the black hole
The infalling observer
White holes
Kruskal coordinates
The singularities at r =
0. and cosmic censorship
The spacetime of a collapsing star
Embedding diagrams
Asymptotic flatness
The Penrose-Carter diagram for the Schwarzschild metric
The Penrose-Carter diagram for the Newtonian metric
Non-isolated black holes
The infinite redshift surface
Trapped surfaces
Apparent horizon
The membrane paradigm
Rotating Black Holes
The Kerr metric
The event horizon
The circumference of the event horizon
The area of the event horizon
Properties of the Kerr metric coefficients
Identities
Contravariant components
Interpretation of m, a and geometric units
Extreme Kerr black hole
Robinson's theorem
Particle orbits in the Kerr geometry
Constants of the motion
Energy
Angular momentum
The Carter integral
The radial equation
The effective potential
Frame-dragging
Free fall with zero angular momentum
Orbits with non-zero angular momentum
Zero angular momentum observers (ZAMOs)
Some applications of ZAMOs
Photon orbits
The photon effective potential
Azimuthal motion
Photon capture cross-section
The static limit surface
The infinite redshift surface
Circular orbits in the equatorial plane
Innermost (marginally) stable circular orbit
Period of a circular orbit
Energy of the innermost stable orbit
Angular momentum of the innermost stable orbit
Marginally bound orbits
Unbound orbits
Polar orbits
Orbital period
The ergosphere
Negative energy orbits
Energy and angular momentum
The Penrose process
Realising the Penrose process
Spinning up a black hole
From Schwarzschild to extreme Kerr black hole
Other coordinates
Penrose-Carter diagram
Interior solutions and collapsing stars
Closed timelike lines
Charged black holes
Black Hole Thermodynamics
Black hole mechanics
Surface gravity
Redshift
Conservation of energy
The area of a Kerr black hole horizon cannot decrease
Area change by accretion
Area change produced by the Penrose process
The area theorem
Irreducible mass
Maximum energy extraction
Naked singularities
Scattering of waves
Superradiance
Thermodynamics
Horizon temperature
The four laws of black hole thermodynamics
Hawking radiation
Introduction
Casimir effect
Thermal vacua in accelerated frames
Hawking radiation
Properties of radiating black holes
Entropy and temperature
Radiating black holes
Black hole in a box
Entropy and microstates
Wormholes and Time Travel
Introduction
Wormholes
Traversible wormholes
Creating a wormhole
Weak energy condition
Exotic matter
Time machines
Chronology protection
Astrophysical Black Holes
Introduction
Stellar mass black holes
Formation
Finding stellar mass black holes
The black hole at the centre of the Galaxy
Supermassive black holes in other galaxies
Intermediate mass black holes
Mini black holes
Further evidence for black hole spin
Conclusions
Solutions to Problems
References
Bibliography
Index
Edwin Thomas grew up in West Germany, Belgium and America before returning to England to study history at Lincoln College, Oxford. His conclusion to the short story Death by the Invisible Hand was published in The Economist in 1997, and the first chapter of The Blighted Cliffs was runner-up in the 2001 Crime Writers Association D_but Dagger Award for new fiction. The first two installments of the adventures of Martin Jerrold, The Blighted Cliffs and The Chains of Albion, are available in Bantam paperback.


List price: $65.00
Edition: 2nd 2009
Publisher: Imperial College Press
Binding: Trade Cloth
Pages: 212
Size: 6.00" wide x 9.00" long x 0.75" tall
Weight: 1.14 lbs.
Language: English

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