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Title: Investigating the mixing between two black hole populations in LIGO-Virgo-KAGRA GWTC-3

Journal Article · · Physical Review. D.

Here, we introduce a population model to analyze the mixing between hypothesised power-law and ~ 35M Gaussian bump black hole populations in the latest gravitational wave catalog, GWTC 3, estimating their co-location and separation. We find a relatively low level of mixing, $$3.1^{+5.0}_{-3.1}$$%, between the power-law and Gaussian populations, compared to the percentage of mergers containing two Gaussian bump black holes, $$5.0^{+3.2}_{-1.7}$$%. Our analysis indicates that black holes within the Gaussian bump are generally separate from the power-law population, with only a minor fraction engaging in mixing and contributing to the $$\mathcal{M}$$ ~ 14M peak in the chirp mass. This leads us to identify a distinct population of Binary Gaussian Black Holes (BGBHs) that arise from mergers within the Gaussian bump. We suggest that current theories for the formation of the massive 35M Gaussian bump population may need to reevaluate the underlying mechanisms that drive the preference for BGBHs.

Research Organization:
Lawrence Livermore National Laboratory (LLNL), Livermore, CA (United States)
Sponsoring Organization:
USDOE National Nuclear Security Administration (NNSA); USDOE Laboratory Directed Research and Development (LDRD) Program; National Aeronautics and Space Administration (NASA); National Science Foundation (NSF); National Institutes of Health (NIH)
Grant/Contract Number:
AC52-07NA27344
OSTI ID:
2472517
Report Number(s):
LLNL--JRNL-862034; 1094530
Journal Information:
Physical Review. D., Journal Name: Physical Review. D. Journal Issue: 6 Vol. 110; ISSN 2470-0010
Publisher:
American Physical Society (APS)Copyright Statement
Country of Publication:
United States
Language:
English

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