Quasi-Stationary Binary in Spiral

Details Quasi-Stationary Binary in Spiral Quasi-Stationary Binary in Spiral

Dec 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998tx19.confe.498w&link_type=abstract

Abstracts of the 19th Texas Symposium on Relativistic Astrophysics and Cosmology, held in Paris, France, Dec. 14-18, 1998. Eds.:

Astronomy and Astrophysics

Astrophysics

Scientific paper

A binary system of compact objects is stable in Newtonian gravity, but will decay due to emission of gravitational waves in General Relativity. (Such a system is a prime candidate for detection by forthcoming gravitational wave observatories such as LIGO, VIRGO, and LISA.) This project considers the regime where the gravitational interaction is too strong to use weak-field approximation methods, but the time scale for decay of the orbits is still long compared to the orbital period, and attempts to approximate the slowly evolving spacetime by a stationary one.

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