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

Ajith, P., Hannam, M., Husa, S., Chen, Y., Bruegmann, B., Dorband, N., et al. (2011). Inspiral-Merger-Ringdown Waveforms for Black-Hole Binaries with Nonprecessing Spins. Pysical Review Letters, 106: 241101. doi:10.1103/PhysRevLett.106.241101.

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Item Permalink: http://hdl.handle.net/11858/00-001M-0000-0012-9C95-2 Version Permalink: http://hdl.handle.net/11858/00-001M-0000-0012-9C9B-5
Genre: Journal Article

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0909.2867 (Preprint), 781KB
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 Creators:
Ajith, P.1, Author
Hannam, M., Author
Husa, Sascha2, Author              
Chen, Yanbei2, Author              
Bruegmann, B., Author
Dorband, Nils2, Author              
Mueller, D., Author
Ohme, Frank2, Author              
Pollney, Denis2, Author              
Reisswig, Christian2, Author              
Santamaria, Lucia2, Author              
Seiler, Jennifer2, Author              
Affiliations:
1Observational Relativity and Cosmology, AEI-Hannover, MPI for Gravitational Physics, Max Planck Society, Hannover, DE, escidoc:24011              
2Astrophysical Relativity, AEI-Golm, MPI for Gravitational Physics, Max Planck Society, escidoc:24013              

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Free keywords: General Relativity and Quantum Cosmology, gr-qc,Astrophysics, Cosmology and Extragalactic Astrophysics, astro-ph.CO
 Abstract: We present the first analytical inspiral-merger-ringdown gravitational waveforms from black-hole (BH) binaries with non-precessing spins. By matching a post-Newtonian description of the inspiral to a set of numerical calculations performed in full general relativity, we obtain a waveform family with a conveniently small number of physical parameters. The physical content of these waveforms includes the "orbital hang-up" effect, when BHs are spinning rapidly along the direction of the orbital angular momentum. These waveforms will allow us to detect a larger parameter space of BH binary coalescence, to explore various scientific questions related to GW astronomy, and could dramatically improve the expected detection rates of GW detectors.

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 Dates: 2009-09-1520102011
 Publication Status: Published in print
 Pages: 4 pages, 5 figures
 Publishing info: -
 Table of Contents: -
 Rev. Method: -
 Identifiers: arXiv: 0909.2867
DOI: 10.1103/PhysRevLett.106.241101
URI: http://arxiv.org/abs/0909.2867
 Degree: -

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Title: Pysical Review Letters
  Alternative Title : Phys. Rev. Lett.
Source Genre: Journal
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Publ. Info: Woodbury, N.Y., etc. : American Physical Society.
Pages: 4 Volume / Issue: 106 Sequence Number: 241101 Start / End Page: - Identifier: Other: 954925433406
Other: 0031-9007