New Class of Gravitational Wave Templates for Inspiralling Compact Binaries

Details New Class of Gravitational Wave Templates for Inspiralling Compact Binaries New Class of Gravitational Wave Templates for Inspiralling Compact Binaries

2007-12-19

arxiv.org/abs/0712.3236v1

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

5 pages

Scientific paper

Compact binaries inspiralling along quasi-circular orbits are the most plausible gravitational wave (GW) sources for the operational, planned and proposed laser interferometers. We provide new class of restricted post-Newtonian accurate GW templates for non-spinning compact binaries inspiralling along PN accurate quasi-circular orbits. Arguments based on data analysis, theoretical and astrophysical considerations are invoked to show why these time-domain Taylor approximants should be interesting to various GW data analysis communities.

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