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Mathematical Theory of Black Holes [Minkštas viršelis]

(late Professor Emeritus, University of Chicago, USA)
  • Formatas: Paperback / softback, 672 pages, aukštis x plotis x storis: 231x155x35 mm, weight: 955 g
  • Serija: Oxford Classic Texts in the Physical Sciences
  • Išleidimo metai: 03-Sep-1998
  • Leidėjas: Oxford University Press
  • ISBN-10: 0198503709
  • ISBN-13: 9780198503705
Kitos knygos pagal šią temą:
  • Formatas: Paperback / softback, 672 pages, aukštis x plotis x storis: 231x155x35 mm, weight: 955 g
  • Serija: Oxford Classic Texts in the Physical Sciences
  • Išleidimo metai: 03-Sep-1998
  • Leidėjas: Oxford University Press
  • ISBN-10: 0198503709
  • ISBN-13: 9780198503705
Kitos knygos pagal šią temą:
Part of the reissued Oxford Classic Texts in the Physical Sciences series, this book was first published in 1983, and has swiftly become one of the great modern classics of relativity theory. It represents a personal testament to the work of the author, who spent several years writing and working-out the entire subject matter.

The theory of black holes is the most simple and beautiful consequence of Einstein's relativity theory. At the time of writing there was no physical evidence for the existence of these objects, therefore all that Professor Chandrasekhar used for their construction were modern mathematical concepts of space and time. Since that time a growing body of evidence has pointed to the truth of Professor Chandrasekhar's findings, and the wisdom contained in this book has become fully evident.

Recenzijos

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


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