This 2004 textbook fills a gap in the literature on general relativity by providing the advanced student with practical tools for the computation of many physically interesting quantities. The context is provided by the mathematical theory of black holes, one of the most elegant, successful, and relevant applications of general relativity. Among the topics discussed are congruencies of timelike and null geodesics, the embedding of spacelike, timelike and null hypersurfaces in spacetime, and the Lagrangian and Hamiltonian formulations of general relativity. Although the book is self-contained, it is not meant to serve as an introduction to general relativity. Instead, it is meant to help the reader acquire advanced skills and become a competent researcher in relativity and gravitational physics. The primary readership consists of graduate students in gravitational physics. It will also be a useful reference for more seasoned researchers working in this field.
Rezensionen / Stimmen
'... an elegant, thoughtful, useful and altogether commendable publication.' Contemporary Physics 'The author puts emphasis on training the readers and equipping them with the relevant skills of a working relativist. The text reaches a high pedagogical standard ... In this way the author succeeds in closing a gap in the existing text book literature especially for a readership mainly oriented towards physics.' Monatshefte fuer Mathematik
Sprache
Verlagsort
Zielgruppe
Produkt-Hinweis
Illustrationen
Worked examples or Exercises; 3 Tables, unspecified; 39 Line drawings, unspecified
Maße
Höhe: 244 mm
Breite: 170 mm
Dicke: 14 mm
Gewicht
ISBN-13
978-0-521-53780-3 (9780521537803)
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
Eric Poisson is Professor of Physics at the University of Guelph.
Autor*in
University of Guelph, Ontario
Preface; Notation and conventions; 1. Fundamentals; 2. Geodesic congruences; 3. Hypersurfaces; 4. Lagrangian and Hamiltonian formulation of general relativity; 5. Black holes; References; Index.
