Exact solution of Peters-Mathews equations for any orbital eccentricity.

Details Exact solution of Peters-Mathews equations for any orbital eccentricity. Exact solution of Peters-Mathews equations for any orbital eccentricity.

May 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996ncimb.111..631p&link_type=abstract

Nuovo Cimento B, Vol. 111B, No. 5, p. 631 - 644

Mathematics

7

Binaries: Gravitational Radiation, Binaries: Orbits

Scientific paper

The standard (Peters-Mathews) model for binary star orbital damping under gravitational wave emission is completely solved in analytic form, for any value of the initial orbital eccentricity, resulting into a universal decay scenario. The limits of validity of the model are established in a general handy form. Possible extensions of these results to higher-order post-Newtonian models are discussed.

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