Black holes present one of the most fascinating predictions of Einstein's general theory of relativity. There is strong evidence of their existence through observation of active galactic nuclei, including the centre of our galaxy, observations of gravitational waves, and others.
There exists a large scientific literature on black holes, including many excellent textbooks at various levels. However, most of these steer clear from the mathematical niceties needed to make the theory of black holes a mathematical theory. Those which maintain a high mathematical standard are either focused on specific topics, or skip many details. The objective of this book is to fill this gap and present a detailed, mathematically oriented, extended introduction to the subject.
The book provides a wide background to the current research on all mathematical aspects of the geometry of black hole spacetimes.
Rezensionen / Stimmen
Written with a high standard of rigor and care, with very good treatments of many topics that are hard to find elsewhere. * Robert Wald, University of Chicago * Including some very interesting and unique material, the book is written in a manner that will be accessible for students, and provide a valuable resource for experts working in mathematical general relativity. * Greg Galloway, University of Miami *
Reihe
Auflage
Sprache
Verlagsort
Zielgruppe
Produkt-Hinweis
Fadenheftung
Gewebe-Einband
Illustrationen
82 b/w figures, 15 colour illustrations
Maße
Höhe: 249 mm
Breite: 176 mm
Dicke: 26 mm
Gewicht
ISBN-13
978-0-19-885541-5 (9780198855415)
Copyright in bibliographic data and cover images is held by Nielsen Book Services Limited or by the publishers or by their respective licensors: all rights reserved.
Schweitzer Klassifikation
Univ. Prof. Dr. Piotr T. Chrusciel is Professor of Gravitational Physics and Head of the Gravitational Physics Group, Faculty of Physics, University of Vienna, Austria.
Autor*in
Professor of Gravitational Physics, Head of the Gravitational Physics GroupProfessor of Gravitational Physics, Head of the Gravitational Physics Group, Faculty of Physics, University of Vienna
PART I GLOBAL LORENTZIAN GEOMETRY
1: Basic notions
2: Elements of causality
3: Some applications
PART II BLACK HOLES
4: An introduction to black holes
5: Further selected solutions
6: Extensions, conformal diagrams
7: Projection diagrams
8: Dynamical black holes
Appendices
References
Index