The Mathematical Theory of Black Holes
Price: 1100.00 INR
ISBN:
9780198863137
Publication date:
16/12/2019
Paperback
672 pages
234.0x156.0mm
Price: 1100.00 INR
ISBN:
9780198863137
Publication date:
16/12/2019
Paperback
672 pages
234.0x156.0mm
The late S. Chandrasekhar
First published in 1983, this book is one of the great modern classics of relativity theory. It details one of the most beautiful areas of ...
Rights: OUP UK (Indian Territory)
The late S. Chandrasekhar
Description
First published in 1983, this book is one of the great modern classics of relativity theory. It details one of the most beautiful areas of mathematical physics; the theory of black holes.
`There is no doubt in my mind that this book is a masterpiece ... beautifully written and well-presented.' Roger Penrose in Nature.
About the Author
S. Chandrasekhar, late Professor Emeritus, University of Chicago, USA
The late S. Chandrasekhar
Table of contents
1: Mathematical preliminaries
2: A space-time of sufficient generality
3: The Schwarzchild space-time
4: The perturbations of the Schwarzchild black hole
5: The Reissner-Nordstrom solution
6: The Kerr metric
7: The geodesics in the Kerr space-time
8: Electromagnetic waves in Kerr geometry
9: The gravitational perturbations of the Kerr black hole
10: Spin-1/2 particles in Kerr geometry
11: Other solutions
12: Other methods
The late S. Chandrasekhar
The late S. Chandrasekhar
Review
There is no doubt in my mind that this book is a masterpiece...beautifully written and well-presented. - Roger Penrose in Nature
"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 similarities and 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
Description
First published in 1983, this book is one of the great modern classics of relativity theory. It details one of the most beautiful areas of mathematical physics; the theory of black holes.
`There is no doubt in my mind that this book is a masterpiece ... beautifully written and well-presented.' Roger Penrose in Nature.
About the Author
S. Chandrasekhar, late Professor Emeritus, University of Chicago, USA
Read MoreReviews
There is no doubt in my mind that this book is a masterpiece...beautifully written and well-presented. - Roger Penrose in Nature
"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 similarities and 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
Read MoreTable of contents
1: Mathematical preliminaries
2: A space-time of sufficient generality
3: The Schwarzchild space-time
4: The perturbations of the Schwarzchild black hole
5: The Reissner-Nordstrom solution
6: The Kerr metric
7: The geodesics in the Kerr space-time
8: Electromagnetic waves in Kerr geometry
9: The gravitational perturbations of the Kerr black hole
10: Spin-1/2 particles in Kerr geometry
11: Other solutions
12: Other methods