The apsidal motion of a binary star in the nonsymmetric gravitation theory

Details The apsidal motion of a binary star in the nonsymmetric gravitation theory The apsidal motion of a binary star in the nonsymmetric gravitation theory

Mar 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985cajph..63..428m&link_type=abstract

Canadian Journal of Physics (ISSN 0008-4204), vol. 63, March 1985, p. 428-430.

Physics

5

Eclipsing Binary Stars, Gravitation Theory, Stellar Motions, Apsides, Equations Of Motion

Scientific paper

The two-body post-Newtonian equations of motion in the nonsymmetric
gravitational theory are reduced to the one-body form in the
center-of-mass coordinates. The periastron shift formula is calculated
and an additional negative contribution is found that can have important
consequences for apsidal motion in close binary systems.

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