Gravitational Waves from Inspiralling Compact Binaries: A Post-Newtonian Approach

Details Gravitational Waves from Inspiralling Compact Binaries: A Post-Newtonian Approach Gravitational Waves from Inspiralling Compact Binaries: A Post-Newtonian Approach

1994-03-17

arxiv.org/abs/gr-qc/9403033v1

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

16 pages, WUGRAV-94-3

Scientific paper

Inspiralling binary systems of neutron stars or black holes are promising sources of gravitational radiation detectable by large-scale laser interferometric gravitational observatories, such as the US LIGO and Italian-French VIRGO projects. Accurate theoretical gravitational-waveform templates will be needed to carry out matched filtering data analysis of the detectors' output once they are on the air by the end of this decade. For all but the final, strongly general relativistic coalescence of the two bodies, high-order post-Newtonian methods are playing a major role in the theorists' efforts to develop the needed templates. This paper discusses the foundations of this method, and provides a compendium of useful formulae and results. Figures available upon request. (Invited talk given at the 8th Nishinomiya-Yukawa Memorial Symposium, October 28, 1993.)

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