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Black hole spin-mass correlation and vector resonant relaxation in gaseous star clusters: the origin of GW231123?
During the formation of a star cluster a spin-mass correlation of stellar black holes is generated as they grow via accretion of the residual gas. Moreover, the black hole spin tends to be anti-aligned with its orbital angular momentum in the cluster. We show that GW231123, reported by the LIGO-Virg
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