Second MAYA catalog of binary black hole numerical relativity waveforms

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 7 simulations that 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.

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Publication Details

Journal
Physical review. D/Physical review. D.
Published
2025-07-30
DOI
https://doi.org/10.1103/gk7x-9cds
Citations
5
Primary Topic
Pulsars and Gravitational Waves Research
Type
article
Field-Weighted Citation Impact
5.77

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Second MAYA catalog of binary black hole numerical relativity waveforms

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5 citations
Physical review. D/Physical review. D.
Pulsars and Gravitational Waves Research
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article

Second MAYA catalog of binary black hole numerical relativity waveforms

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article en
5 citations

Abstract

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 7 simulations that 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.

Physical review. D/Physical review. D.Vol. 112(4)
University of Illinois Urbana-Champaign (US), The University of Texas at Austin (US)
National Science Foundation, National Aeronautics and Space Administration
Openalex Percentile: Top 4%
Pulsars and Gravitational Waves Research
5.77
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