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Mass Distribution of Binary Black Hole Mergers from Young and Old Dense Star Clusters

Dense star clusters are thought to contribute significantly to the merger rates of stellar-mass binary black holes (BBHs) detected by the LIGO–Virgo–KAGRA collaboration. We combine N -body dynamic models of realistic dense star clusters with cluster formation histories to estimate the merger rate di...

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Bibliografiset tiedot
Päätekijät: Claire S. Ye, Maya Fishbach, Kyle Kremer, Marta Reina-Campos
Aineistotyyppi: Artigo
Kieli:Inglês
Julkaistu: IOP Publishing 2026-01-01
Sarja:The Astrophysical Journal
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Linkit:https://doi.org/10.3847/1538-4357/ae317f
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