Supermassive black holes from runaway mergers and accretion in nuclear star clusters
Monthly Notices of the Royal Astronomical Society(2024)
摘要
Rapid formation of supermassive black holes occurs in dense nuclear star
clusters that are initially gas-dominated. Stellar-mass black hole remnants of
the most massive cluster sink into the core, where a massive runaway black hole
forms as a consequence of combined effects of repeated mergers and
Eddington-limited gas accretion. The associated gravitational-wave signals of
high-redshift extreme mass-ratio inspirals are a unique signature of the
nuclear star cluster scenario.
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