Coalescing binary systems of compact objects to (post) exp 5/2-Newtonian order

Details Coalescing binary systems of compact objects to (post) exp 5/2-Newtonian order Coalescing binary systems of compact objects to (post) exp 5/2-Newtonian order

Aug 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991nyasa.631..126w&link_type=abstract

(Nonlinear problems in relativity and cosmology; Proceedings of the 6th Florida Workshop in Nonlinear Astronomy, Gainesville, Oc

Astronomy and Astrophysics

Astronomy

1

Black Holes (Astronomy), Gravitational Waves, Laser Interferometry, Neutron Stars, Newton Theory, Binary Stars, Equations Of Motion, Galactic Evolution

Scientific paper

Approximate equations of motion based on an assumption of weak interbody gravitational fields and slow orbital motions, known as the post-Newtonian approximation, are used here to study the orbital evolution of coalescing binary sytems of compact objects. The gravitational radiation emitted by the system is determined using post-Newtonian gravitational waveforms derived by Wagoner and Will (1976). The gravitational-radiation recoil is calculated.

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