2-post-Newtonian approximation of a nonstationary spherically symmetric star in flat space-time theory of gravitation

DOI10.1007/BF00628237zbMath0815.53083MaRDI QIDQ1342448

Walter Petry

Publication date: 16 February 1995

Published in: Astrophysics and Space Science (Search for Journal in Brave)

zbMATH Keywords

total energyequations of motionflat space-timeBirkhoff's theoremspherically symmetric star2-post-Newtonian approximation

Mathematics Subject Classification ID

Applications of differential geometry to physics (53Z05) Gravitational energy and conservation laws; groups of motions (83C40) Equations of motion in general relativity and gravitational theory (83C10)

Related Items (1)

Motion of a test particle in a nonstationary spherically symmetric gravitational field in flat space-time theory of gravitation

Cites Work

• The gravitational field of static spherically symmetric bodies
• Post-Newtonian approximation of a nonstationary spherically symmetric star in flat space-time theory of gravitation

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