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

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

Jan 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994ap%26ss.211...71p&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 211, no. 1, p. 71-91

Astronomy and Astrophysics

Astrophysics

4

Collapse, Gravitation Theory, Stars, Symmetrical Bodies, Energy Conservation, Equations Of Motion, Gravitational Fields

Scientific paper

Starting from a previously studied theory of gravitation in flat space-time the post-Newtonian approximation of the gravitational field of a nonstationary spherically symmetric star is derived. To the post-Newtonian order the equations of motion and the conserved total energy of a collapsing star are given. Birkhoff's theorem holds to this accuracy.

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