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Beschreibung
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.
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.
Inhaltsverzeichnis
  • 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

Details
Erscheinungsjahr: 1998
Fachbereich: Astronomie
Genre: Importe, Physik
Rubrik: Naturwissenschaften & Technik
Medium: Taschenbuch
Inhalt: Kartoniert / Broschiert
ISBN-13: 9780198503705
ISBN-10: 0198503709
Sprache: Englisch
Einband: Kartoniert / Broschiert
Autor: Chandrasekhar, S.
Hersteller: OUP Oxford
Verantwortliche Person für die EU: Libri GmbH, Europaallee 1, D-36244 Bad Hersfeld, gpsr@libri.de
Maße: 234 x 156 x 36 mm
Von/Mit: S. Chandrasekhar
Erscheinungsdatum: 03.09.1998
Gewicht: 1,004 kg
Artikel-ID: 108640733

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