Gravitational waves from inspiraling compact binaries: Second post-Newtonian waveforms as search templates II

Details Gravitational waves from inspiraling compact binaries: Second post-Newtonian waveforms as search templates II Gravitational waves from inspiraling compact binaries: Second post-Newtonian waveforms as search templates II

1998-06-19

arxiv.org/abs/gr-qc/9806077v1

Phys.Rev. D59 (1999) 064030

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

5 pages, 3 Figures, RevTeX

Scientific paper

10.1103/PhysRevD.59.064030

We present further evidence that the second post-Newtonian (pN) approximation to the gravitational waves emitted by inspiraling compact binaries is sufficient for the detection of these systems. This is established by comparing the 2-pN wave forms to signals calculated from black hole perturbation theory. Results are presented for different detector noise curves. We also discuss the validity of this type of analysis.

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