The importance of gravitational self-field effects in binary systems with compact objects. I. The static two-body problem and the attraction law in a Post-Newtonian approximation of general relativity

DOI10.1007/BF00760870zbMath0431.70005OpenAlexW2086028785MaRDI QIDQ1138394

S. H. Smith

Publication date: 1978

Published in: General Relativity and Gravitation (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1007/bf00760870

zbMATH Keywords

Einstein's theory of gravitationbinary systems with compact objectspost- Newtonian approximation of general relativitystatic two-body problem

Mathematics Subject Classification ID

Two-body problems (70F05) Einstein's equations (general structure, canonical formalism, Cauchy problems) (83C05) Statics (70C20)

Related Items

The force law for the dynamic two-body problem in the second post- Newtonian approximation of general relativity, Testing general relativity with compact-body orbits: a modified Einstein–Infeld–Hoffmann framework

Cites Work

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• Equations of hydrodynamics in general relativity in the slow motion approximation