The Large Scale Structure of Space-Time (Cambridge Monographs on Mathematical Physics) Ellis G. F., R. and W. Hawking Stephen Einstein's General Theory of Relativity leads to two remarkable predictions: first, that the ultimate destiny of many massive stars is to undergo gravitational collapse and to disappear from view, leaving behind a 'black hole' in space; and secondly, that there will exist singularities in space-time itself. These singularities are places where space-time begins or ends, and the presently known laws of physics break down. They will occur inside black holes, and in the past are what might be construed as the beginning of the universe. To show how these predictions arise, the authors discuss the General Theory of Relati

Ellis G. F., R. and W. Hawking Stephen

ISBN 10: 0521200164 / ISBN 13: 9780521200165

Edité par Cambridge University Press, 1973

A propos de cet article

Einstein's General Theory of Relativity leads to two remarkable predictions: first, that the ultimate destiny of many massive stars is to undergo gravitational collapse and to disappear from view, leaving behind a 'black hole' in space; and secondly, that there will exist singularities in space-time itself. These singularities are places where space-time begins or ends, and the presently known laws of physics break down. They will occur inside black holes, and in the past are what might be construed as the beginning of the universe. To show how these predictions arise, the authors discuss the General Theory of Relativity in the large. Starting with a precise formulation of the theory and an account of the necessary background of differential geometry, the significance of space-time curvature is discussed and the global properties of a number of exact solutions of Einstein's field equations are examined. The theory of the causal structure of a general space-time is developed, and is used to study black holes and to prove a number of theorems establishing the inevitability of singualarities under certain conditions. A discussion of the Cauchy problem for General Relativity is also included in this 1973 book. The Large Scale Structure of Space-Time (Cambridge Monographs on Mathematical Physics) EAN (ISBN-13): 9780521200165 ISBN (ISBN-10): 0521200164 Gebundene Ausgabe Erscheinungsjahr: 1973 Herausgeber: Cambridge University Press ISBN/EAN: 0521200164 ISBN: 0-521-20016-4, 978-0-521-20016-5 Autor des Buches: hawking ellis, steven hawking, stephen hawking Titel des Buches: structure physics, the large scale structure space time, mathematical structure, space into Ellis G. F., R. and W. Hawking Stephen The Large Scale Structure of Space-Time Cambridge Monographs on Mathematical Physics In englischer Sprache. 400 pages. 15.8 x 2.5 x 23.5 cm.

N° de réf. du vendeur BN441675

Détails bibliographiques

• Titre: The Large Scale Structure of Space-Time (Cambridge Monographs on Mathematical Physics) Ellis G. F., R. and W. Hawking Stephen Einstein's General Theory of Relativity leads to two remarkable predictions: first, that the ultimate destiny of many massive stars is to undergo gravitational collapse and to disappear from view, leaving behind a 'black hole' in space; and secondly, that there will exist singularities in space-time itself. These singularities are places where space-time begins or ends, ...
• Éditeur: Cambridge University Press
• Date de parution: 1973
• Langue: anglais
• ISBN à 10 chiffres: 0521200164
• ISBN à 13 chiffres: 9780521200165
• Reliure: Hardcover
• Édition: 1973.
• État de l'article: gut
• Poids: 700 grammes

A propos de ce titre

Synopsis

Einstein's General Theory of Relativity leads to two remarkable predictions: first, that the ultimate destiny of many massive stars is to undergo gravitational collapse and to disappear from view, leaving behind a 'black hole' in space; and secondly, that there will exist singularities in space-time itself. These singularities are places where space-time begins or ends, and the presently known laws of physics break down. They will occur inside black holes, and in the past are what might be construed as the beginning of the universe. To show how these predictions arise, the authors discuss the General Theory of Relativity in the large. Starting with a precise formulation of the theory and an account of the necessary background of differential geometry, the significance of space-time curvature is discussed and the global properties of a number of exact solutions of Einstein's field equations are examined. The theory of the causal structure of a general space-time is developed, and is used to study black holes and to prove a number of theorems establishing the inevitability of singualarities under certain conditions. A discussion of the Cauchy problem for General Relativity is also included in this 1973 book.