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2016

Accuracy of binary black hole waveform models for aligned-spin binaries

Kumar, Prayush, Chu, Tony, Fong, Heather et al.

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Coalescing binary black holes are among the primary science targets for second generation ground-based gravitational wave (GW) detectors.

Reliable GW models are central to detection of such systems and subsequent parameter estimation.
This paper performs a comprehensive analysis of the accuracy of recent waveform models for binary black holes with aligned spins, utilizing a new set of $84$ high-accuracy numerical relativity simulations.
Our analysis covers comparable mass binaries ($1\le m_1/m_2\le 3$), and samples independently both black hole spins up to dimensionless spin-magnitude of $0.9$ for equal-mass binaries and $0.85$ for unequal mass binaries.

Accuracy of binary black hole waveform models for aligned-spin binaries · Around

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