Ajith, P. and Hannam, M. and Husa, S. and Chen, Y. and Brügmann, B. and Dorband, N. and Müller, D. and Ohme, F. and Pollney, D. and Reisswig, C. and Santamaría, L. and Seiler, J. (2011) Inspiral-Merger-Ringdown Waveforms for Black-Hole Binaries with Nonprecessing Spins. Physical Review Letters, 106 (24). Art. No. 241101. ISSN 0031-9007. http://resolver.caltech.edu/CaltechAUTHORS:20110705-133359175
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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.
|Additional Information:||© 2011 American Physical Society. Received 17 September 2009; revised manuscript received 15 September 2010; published 15 June 2011. S. H. was supported by VESF and EGO, DAAD grant D/07/13385 and Spanish Ministry of Science grant FPA-2007-60220. M.H. was supported by FWF grant M1178-N16 and STFC grant ST/H008438/1. P. A. and Y. C. were supported by NSF grants PHY-0653653, PHY- 0601459, PHY-0956189 and David and Barbara Groce Fund. B. B. is supported by DFG grant SFB/Transregio 7 ‘‘GW Astronomy’’, B. B. and D. M. by DLR, and L. S. by DAAD grant A/06/12630. We thank AEI, FSU Jena, LRZ, ICHEC, VSC, CESGA and BSC-CNS for computational resources, and K. G. Arun, B. Sathyaprakash, G. Faye, and R. O’Shaughnessy for discussions.|
|Classification Code:||PACS: 04.30.-w, 04.25.dg|
|Official Citation:||Inspiral-Merger-Ringdown Waveforms for Black-Hole Binaries with Nonprecessing Spins P. Ajith, M. Hannam, S. Husa, Y. Chen, B. Brügmann, N. Dorband, D. Müller, F. Ohme, D. Pollney, C. Reisswig, L. Santamaría, and J. Seiler Published 15 June 2011 (4 pages) 241101|
|Usage Policy:||No commercial reproduction, distribution, display or performance rights in this work are provided.|
|Deposited By:||Ruth Sustaita|
|Deposited On:||05 Jul 2011 20:53|
|Last Modified:||26 Dec 2012 13:22|
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