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This article presents a study of the sufficient accuracy of post-Newtonian and numerical relativity waveforms for the most demanding usage case: parameter estimation of strong sources in advanced gravitational wave detectors.
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B. Aylott et al · 2009
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Alessandra Buonanno, Yi Pan, Harald P. Pfeiffer, Mark A. Scheel, Luisa T. Buchman, and Lawrence E. Kidder · 2009
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Optimal calibration accuracy for gravitational wave detectors
Lee Lindblom · 2009
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Lee Lindblom · 2009
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T. Damour, B. R. Iyer, and A. Nagar · 2009
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Matching post-newtonian and numerical relativity waveforms: Systematic errors and a new phenomenological model for non-precessing black hole binaries
L. Santamaría, F. Ohme, P. Ajith, B. Brügmann, N. Dorband, M. Hannam, S. Husa, P. Mösta, D. Pollney, C. Reisswig, E. L. Robinson, J. Seiler, and B. Krishnan · 2010
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Lee Lindblom, John G. Baker, and Benjamin J. Owen · 2010
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M. Hannam, S. Husa, F. Ohme, and P. Ajith · 2010
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Observing mergers of nonspinning black-hole binaries
Sean T. McWilliams, Bernard J. Kelly, and John G. Baker · 2010
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A tapering window for time-domain templates and simulated signals in the detection of gravitational waves from coalescing compact binaries
D.J.A. McKechan, C. Robinson, and B.S. Sathyaprakash · 2010
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Simulations of black-hole binaries with unequal masses or nonprecessing spins: Accuracy, physical properties, and comparison with post-Newtonian results
Mark Hannam, Sacha Husa, Franke Ohme, Doreen Müller, and Bernd Brügmann · 2010
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Binary black hole simulations using CUDA
Abdul H. Mroué · 2010
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Accuracy and effectualness of closed-form, frequency-domain waveforms for nonspinning black hole binaries
T. Damour, A. Nagar, and M. Trias · 2011
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The uncertainty in hybrid gravitational waveforms: Optimizing initial orbital frequencies for binary black-hole simulations
Michael Boyle · 2011
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Implicit-explicit (IMEX) evolution of single black holes
Stephen R. Lau, Geoffrey Lovelace, and Harald P. Pfeiffer · 2011
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