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Binary black hole detection rates in inspiral gravitational wave searches

Chris Van Den Broeck
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Abstract

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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Chris Van Den Broeck. 2006-05-24. Binary black hole detection rates in inspiral gravitational wave searches. https://doi.org/10.1088/0264-9381%2F23%2F13%2Fl01

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