Binary black hole detection rates in inspiral gravitational wave searches

Details Binary black hole detection rates in inspiral gravitational wave searches Binary black hole detection rates in inspiral gravitational wave searches

2006-04-07

arxiv.org/abs/gr-qc/0604032v2

Class.Quant.Grav. 23 (2006) L51-L58

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

9 pages, 1 figure

Scientific paper

10.1088/0264-9381/23/13/L01

The signal-to-noise ratios (SNRs) for quasi-circular binary black hole inspirals computed from restricted post-Newtonian waveforms are compared with those attained by more complete post-Newtonian signals, which are superpositions of amplitude-corrected harmonics of the orbital phase. It is shown that if one were to use the best available amplitude-corrected waveforms for detection templates, one should expect SNRs in actual searches to be significantly lower than those suggested by simulations based purely on restricted waveforms.

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