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Suitability of hybrid gravitational waveforms for unequal-mass binaries · Around

2012

Suitability of hybrid gravitational waveforms for unequal-mass binaries

MacDonald, Ilana, Mroue, Abdul H., Pfeiffer, Harald P. et al.

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This article studies sufficient accuracy criteria of hybrid post-Newtonian (PN) and numerical relativity (NR) waveforms for parameter estimation of strong binary black-hole sources in second- generation ground-based gravitational-wave detectors.

We investigate equal-mass non-spinning binaries with a new 33-orbit NR waveform, as well as unequal-mass binaries with mass ratios 2, 3, 4 and 6.
For equal masses, the 33-orbit NR waveform allows us to recover previous results and to extend the analysis toward matching at lower frequencies.
For unequal masses, the errors between different PN approximants increase with mass ratio.

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