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Second MAYA Catalog of Binary Black Hole Numerical Relativity Waveforms

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arxiv 2309.00262 v3 pith:PDGOX2BH submitted 2023-09-01 gr-qc astro-ph.IM

classification gr-qcastro-ph.IM
keywords catalogwaveformsnumericalrelativitybinarysimulationsblackeccentric
verification ladder T0 review T1 audit T2 compute T3 formal
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Numerical relativity waveforms are a critical resource in the quest to deepen our understanding of the dynamics of, and gravitational waves emitted from, merging binary systems. We present 181 new numerical relativity simulations as the second MAYA catalog of binary black hole waveforms (a sequel to the Georgia Tech waveform catalog). Most importantly, these include 55 high mass ratio (q >= 4), 48 precessing, and 92 eccentric (e > 0.01) simulations, including seven simulations which are both eccentric and precessing. With these significant additions, this new catalog fills in considerable gaps in existing public numerical relativity waveform catalogs. The waveforms presented in this catalog are shown to be convergent and are consistent with current gravitational wave models. They are available to the public at https://cgpstorage.ph.utexas.edu/waveforms.

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Cited by 6 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

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