Post-Newtonian effect on the variation of time of periastron passage of binary stars in three gravitational theories

Details Post-Newtonian effect on the variation of time of periastron passage of binary stars in three gravitational theories Post-Newtonian effect on the variation of time of periastron passage of binary stars in three gravitational theories

May 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010ap%26ss.327...59l&link_type=abstract

Astrophysics and Space Science, Volume 327, Issue 1, pp.59-65

Astronomy and Astrophysics

Astrophysics

5

Post-Newtonian Effect, Variation Of Time Of Periastron Passage, Binary Stars

Scientific paper

The equation for the variation of the time of a periastron passage of binary stars has been solved by using the perturbation approach. The post-Newtonian effect on the variation of the time of a periastron passage has been examined within three gravitational theories. The results clearly show that the periastron passage of a binary star occurs earlier (advances) at each revolution. This effect has been calculated and discussed for ten binary stars.

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