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• W3100124837 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." @default.
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• W3100124837 date "2006-06-09" @default.
• W3100124837 modified "2023-09-27" @default.
• W3100124837 title "Binary black hole detection rates in inspiral gravitational wave searches" @default.
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• W3100124837 doi "https://doi.org/10.1088/0264-9381/23/13/l01" @default.
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