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  Detection template families for gravitational waves from the final stages of binary--black-hole inspirals: Nonspinning case

Buonanno, A., Chen, Y., & Vallisneri, M. (2003). Detection template families for gravitational waves from the final stages of binary--black-hole inspirals: Nonspinning case. Physical Review D, 67: 024016. doi:10.1103/PhysRevD.67.024016.

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Item Permalink: http://hdl.handle.net/11858/00-001M-0000-0018-FEDE-1 Version Permalink: http://hdl.handle.net/11858/00-001M-0000-0018-FEE2-6
Genre: Journal Article

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 Creators:
Buonanno, Alessandra1, 2, 3, Author              
Chen, Yanbei, Author
Vallisneri, Michele, Author
Affiliations:
1Institut d’Astrophysique de Paris (GReCO, FRE 2435 du CNRS), escidoc:persistent22              
2Theoretical Astrophysics, California Institute of Technology, Pasadena, escidoc:persistent22              
3Astrophysical and Cosmological Relativity, AEI-Golm, MPI for Gravitational Physics, Max Planck Society, escidoc:1933290              

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Free keywords: General Relativity and Quantum Cosmology, gr-qc
 Abstract: We investigate the problem of detecting gravitational waves from binaries of nonspinning black holes with masses m = 5--20 Msun, moving on quasicircular orbits, which are arguably the most promising sources for first-generation ground-based detectors. We analyze and compare all the currently available post--Newtonian approximations for the relativistic two-body dynamics; for these binaries, different approximations predict different waveforms. We then construct examples of detection template families that embed all the approximate models, and that could be used to detect the true gravitational-wave signal (but not to characterize accurately its physical parameters). We estimate that the fitting factor for our detection families is >~0.95 (corresponding to an event-rate loss <~15%) and we estimate that the discretization of the template family, for ~10^4 templates, increases the loss to <~20%. Erratum-ibid.D74:029903,2006

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 Dates: 2002-05-292006-07-262003
 Publication Status: Published in print
 Pages: 58 pages, 38 EPS figures, final PRD version; small corrections to GW flux terms as per Blanchet et al., PRD 71, 129902(E)-129904(E) (2005)
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 Rev. Method: -
 Identifiers: arXiv: gr-qc/0205122
DOI: 10.1103/PhysRevD.67.024016
URI: http://arxiv.org/abs/gr-qc/0205122
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Title: Physical Review D
  Other : Phys. Rev. D.
Source Genre: Journal
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Publ. Info: Lancaster, Pa. : American Physical Society
Pages: - Volume / Issue: 67 Sequence Number: 024016 Start / End Page: - Identifier: ISSN: 0556-2821
CoNE: http://pubman.mpdl.mpg.de/cone/journals/resource/111088197762258