- 巻冊次
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: cloth ISBN 9780226870342
内容説明
The inevitability of gravitational collapse for stellar bodies of sufficient mass was convincingly demonstarted by S. Chandrasekhar in the 1930s, black holes and neutron stars played a minor role in serious analyses of physical or astrophysical phenomena until the discovery of quasars and pulsars in the 1960s. Black holes and neutron stars are now generally recognized as key components of many astrophysical systems, and play a central role in the understanding of gravitational phenomena at both the classical and quantum levels. Based on a symposium held in honour of S. Chandrasekhar, these papers provide a comprehensive summary of progress made in the 1990s on the theory of black holes and relativistic stars.
目次
Contributors Preface 1: Gravitational Waves, Stars and Black Holes Valeria Ferrari 2: Rotating Relativistic Stars John L. Friedman 3: Probing Black Holes and Relativistic Stars with Gravitational Waves Kip S. Thorne 4: Astrophysical Evidence for Black Holes Martin J. Rees 5: The Question of Cosmic Censorship Roger Penrose 6: Black Hole Collisions, Toroidal Black Holes, and Numerical Relativity Saul A. Teukolsky 7: The Internal Structure of Black Holes Werner Israel 8: Black Holes and Thermodynamics Robert M. Wald 9: The Statistical Mechanics of Black Hole Thermodynamics Rafael D. Sorkin 10: Generalized Quantum Theory in Evaporating Black Hole Spacetimes James B. Hartle 11: Is Information Lost in Black Holes? Stephen W. Hawking 12: Quantum States of Black Holes Gary T. Horowitz Chandra: A Tribute Kameshwar C. Wali Our Song Lalitha Chandrasekhar
- 巻冊次
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: pbk ISBN 9780226870359
内容説明
The inevitability of gravitational collapse for stellar bodies of sufficient mass was convincingly demonstrated by S. Chandrasekhar in the 1930s, black holes and neutron stars played a minor role in serious analyses of physical or astrophysical phenomena until the discovery of quasars and pulsars in the 1960s. Black holes and neutron stars are now generally recognized as key components of many astrophysical systems, and play a central role in the understanding of gravitational phenomena at both the classical and quantum levels. Based on a symposium held in honour of S. Chandrasekhar, these papers provide a comprehensive summary of progress made in the 1990s on the theory of black holes and relativistic stars.
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