Motion of a Test Particle in a Nonstationary Spherically Symmetric Gravitational Field in Flat Space-Time Theory of Gravitation

Details Motion of a Test Particle in a Nonstationary Spherically Symmetric Gravitational Field 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

Oct 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995ap%26ss.232..233p&link_type=abstract

Astrophysics and Space Science, Volume 232, Issue 2, pp.233-240

Astronomy and Astrophysics

Astrophysics

1

Scientific paper

The previously studied 2-post-Newtonian approximation of the gravitational field of a nonstationary spherically symmetric star in flat space-time theory of gravitation is applied to the motion of a test particle in the orbit of the star. The orbit is different from the one of Einstein's general theory of relativity. A general formula for the deviation of the orbit from a circle is given. In the special case of a radially oscillating star, being homogeneous to Newtonian accuracy, the orbit of the test particle also oscillates radially with small amplitude about a fixed orbit (circle).

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