Inspiral-Merger-Ringdown Waveforms for Black-Hole Binaries with Nonprecessing Spins

被引：428

作者：

Ajith, P. ^{[1
]}

Hannam, M. ^{[2
,3
]}

Husa, S. ^{[4
]}

Chen, Y.

Bruegmann, B. ^{[5
]}

Dorband, N. ^{[6
]}

Mueller, D. ^{[5
]}

Ohme, F. ^{[6
]}

Pollney, D. ^{[4
,6
]}

Reisswig, C. ^{[6
]}

Santamaria, L. ^{[1
,6
]}

Seiler, J. ^{[6
]}

机构：

[1] CALTECH, LIGO Lab, Pasadena, CA 91125 USA

[2] Univ Vienna, Fac Phys, A-1090 Vienna, Austria

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

[4] Univ Illes Balears, Dept Fis, E-07122 Palma De Mallorca, Spain

[5] Univ Jena, Inst Theoret Phys, D-07743 Jena, Germany

[6] Albert Einstein Inst, Max Planck Inst Gravitat Phys, D-14476 Golm, Germany

来源：

PHYSICAL REVIEW LETTERS | 2011年 / 106卷 / 24期

基金：

美国国家科学基金会;

关键词：

D O I：

10.1103/PhysRevLett.106.241101

中图分类号：

O4 [物理学];

学科分类号：

0702 ;

摘要：

We present the first analytical inspiral-merger-ringdown gravitational waveforms from binary black holes (BBHs) with nonprecessing spins, that is based on a description of the late-inspiral, merger and ringdown in full general relativity. By matching a post-Newtonian description of the inspiral to a set of numerical-relativity simulations, we obtain a waveform family with a conveniently small number of physical parameters. These waveforms will allow us to detect a larger parameter space of BBH coalescence, including a considerable fraction of precessing binaries in the comparable-mass regime, thus significantly improving the expected detection rates.

引用

页数：4

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