Einstein's theory of general relativity describes the gravitational field of a system of stars and predicts their paths by providing the 'equations of motion' of each star. Extracting these equations from his field equations is a highly technical procedure described in this book. Observable quantities can then be calculated to test the theory.
Einstein's theory of general relativity describes the gravitational field of a system of stars and predicts their paths by providing the 'equations of motion' of each star. Extracting these equations from his field equations is a highly technical procedure described in this book. Observable quantities can then be calculated to test the theory.
Hideki Asada [Research Fellow, previously: Yukawa Institute for Theoretical Physics, Kyoto University; Institut d'Astrophysique de Paris] Toshifumi Futamase [Research Fellow, previously: Max Planck Institute, Munich; Washington University, St. Louis; University College Cardiff] Peter Hogan [Research Fellow, previously: School of Theoretical Physics, Dublin Institute for Advanced Studies; University of Texas, Austin; Trinity College, Dublin]
Inhaltsangabe
1: Introduction 2: Foundations of the Post Newtonian Approximation 3: The Third Post Newtonian Approximation 4: Two-Body Problem in General Relativity 5: Small Black Holes: Geometrical Preliminaries 6: Small Charged Black Holes: Equations of Motion 7: Gravitational Physics of Few Body Systems
1: Introduction 2: Foundations of the Post Newtonian Approximation 3: The Third Post Newtonian Approximation 4: Two-Body Problem in General Relativity 5: Small Black Holes: Geometrical Preliminaries 6: Small Charged Black Holes: Equations of Motion 7: Gravitational Physics of Few Body Systems
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