This volume has become one of the modern classics of relativity theory. When it was written in 1983 there was little physical evidence for the existence of black holes. Recent discoveries have only served to underscore the elegant theory developed here, and the book remains one of the clearest statements of the relevant mathematics.
"Chandrasekhar has provided us with a magisterial text on the classical black holes, outstanding in the depth and detail of its coverage...Throughout, a wealth of mathematical ideas is explained and employed in the process of extracting the properties of these space-times, and the similaritiesand differences between the different black hole space-times are thoroughly treated. This book is an undoubted classic, and wil remain a standard reference work on black holes for many years." Mathematics Today, October 1999
Table Of Contents
Mathematical preliminaries
A space-time of sufficient generality
The Schwarzchild space-time
The perturbations of the Schwarzchild black hole
The Reissner-Nordstrom solution
The Kerr metric
The geodesics in the Kerr space-time
Electromagnetic waves in Kerr geometry
The gravitational perturbations of the Kerr black hole
Spin-1/2 particles in Kerr geometry
Other solutions
Other methods
Table of Contents provided by Publisher. All Rights Reserved.
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This volume has become one of the modern classics of relativity theory. When it was written in 1983 there was little physical evidence for the existence of black holes. Recent discoveries have only served to underscore the elegant theory developed here, and the book remains one of the clearest statements of the relevant mathematics.
Product Details
Not Applicable
English
Oxford University Press, Incorporated
Nov. 5th, 1998
672
9780198503705
6.14 x 9.21 x 1.38 inches
0198503709
2.20 lbs
Professional Reviews
"Chandrasekhar has provided us with a magisterial text on the classical black holes, outstanding in the depth and detail of its coverage...Throughout, a wealth of mathematical ideas is explained and employed in the process of extracting the properties of these space-times, and the similaritiesand differences between the different black hole space-times are thoroughly treated. This book is an undoubted classic, and wil remain a standard reference work on black holes for many years." Mathematics Today, October 1999
Table Of Contents
Mathematical preliminaries
A space-time of sufficient generality
The Schwarzchild space-time
The perturbations of the Schwarzchild black hole
The Reissner-Nordstrom solution
The Kerr metric
The geodesics in the Kerr space-time
Electromagnetic waves in Kerr geometry
The gravitational perturbations of the Kerr black hole
Spin-1/2 particles in Kerr geometry
Other solutions
Other methods
Table of Contents provided by Publisher. All Rights Reserved.
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