Binary black hole detection rates in inspiral gravitational wave searches

被引：20

作者：

Van den Broeck, Chris ^{[1
]}

机构：

[1] Cardiff Univ, Sch Phys & Astron, Cardiff CF24 3YB, S Glam, Wales

来源：

CLASSICAL AND QUANTUM GRAVITY | 2006年 / 23卷 / 13期

关键词：

D O I：

10.1088/0264-9381/23/13/L01

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

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.

引用

页码：L51 / L58

页数：8

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