Gravitational waves from inspiraling compact binaries: Accuracy of the post-Newtonian waveforms

Details Gravitational waves from inspiraling compact binaries: Accuracy of the post-Newtonian waveforms Gravitational waves from inspiraling compact binaries: Accuracy of the post-Newtonian waveforms

1998-01-12

arxiv.org/abs/gr-qc/9801038v1

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

3 pages, ReVTeX, to appear in the Proceedings of the Second Gravitational Wave Data Analysis Workshop, held in Orsay, France

Scientific paper

The accuracy of the post-Newtonian waveforms, both in standard and Pade form,
is determined by computing their matched-filtering overlap integral with a
reference waveform obtained from black-hole perturbation theory.

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