The effect of a periodic gravitational wave on the parameters of a binary system

Details The effect of a periodic gravitational wave on the parameters of a binary system The effect of a periodic gravitational wave on the parameters of a binary system

Oct 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987azh....64.1030k&link_type=abstract

Astronomicheskii Zhurnal (ISSN 0004-6299), vol. 64, Sept.-Oct. 1987, p. 1030-1036. In Russian.

Astronomy and Astrophysics

Astronomy

Binary Stars, Gravitational Effects, Gravitational Waves, Secular Variations, Stellar Structure, Stellar Systems, Equations Of Motion, Orbital Elements, Periodic Variations, Resonance

Scientific paper

The method of averaging is used in analysing secular terms in the perturbed parameters of a binary system which is subject to the action of a periodical gravitational wave under resonance conditions. The formulae for secular variation of the eccentricity, semimajor axis and pericenter position are derived. For two values of the ratio of the gravitational wave frequency ω to that of the orbital motion ω0, ω/ω0 = 1, 3, the secular terms in the pericenter shifts depend on the eccentricity e as e-1, resulting in a possibility of increasing the effect as e decreases.

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