Post-Newtonian approximation in the relativistic theory of gravity

DOI10.1007/BF02067496zbMath0866.53076OpenAlexW1965722145MaRDI QIDQ676895

A. A. Logunov

Publication date: 20 July 1997

Published in: Theoretical and Mathematical Physics (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1007/bf02067496

zbMATH Keywords

relativistic theory of gravitypost-Newtonian approximationgravitational effects in the solar system

Mathematics Subject Classification ID

Applications of differential geometry to physics (53Z05) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Observational and experimental questions in relativity and gravitational theory (83B05) Approximation procedures, weak fields in general relativity and gravitational theory (83C25)

Related Items (3)

Isotropic geodesics in the neighborhood of a singularity of the static, spherically symmetric solution ⋮ Motion of a massive particle in the vicinity of a singular sphere ⋮ A particular solution of the relativistic theory of gravity obtained by the indefinite coordinate method

Cites Work

• The gravitational equations and the problem of motion
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