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

DOI10.1007/BF00658044zbMath0803.53051OpenAlexW4235087862MaRDI QIDQ1331348

Walter Petry

Publication date: 21 August 1994

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

Full work available at URL: https://doi.org/10.1007/bf00658044

zbMATH Keywords

gravitational fieldpost-Newtonian approximationcollapsing starspherically symmetric star

Mathematics Subject Classification ID

Applications of differential geometry to physics (53Z05) Approximation procedures, weak fields in general relativity and gravitational theory (83C25)

Related Items (4)

2-post-Newtonian approximation of a nonstationary spherically symmetric star in flat space-time theory of gravitation ⋮ Nonsingular cosmological model with background field in flat space-time theory of gravitation ⋮ Theory of linear cosmological perturbations in flat space-time theory of gravitation ⋮ Motion of a test particle in a nonstationary spherically symmetric gravitational field in flat space-time theory of gravitation

Cites Work

• Post-Newtonian gravitational radiation from binary systems in flat space- time theory of gravitation
• Angular momentum and gyroscope in flat space-time theory of gravitation
• Cosmological models without singularities
• Nonsingular cosmological model with matter creation and entropy production
• Superluminal velocity and deviation from Newton's inverse square law
• Lorentz-covariant theory of gravitation
• Gravitation in flat space-time
• The gravitational field of static spherically symmetric bodies
• Post-Newtonian approximation of gravitation theory in flat space-time
• Unnamed Item

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