Fully-conservative BH accretion is disfavored for high-mass BBH mergers; Eddington/GRRMHD accretion with kicks can match part of the LVK high-mass population but still needs another channel.
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High-mass binary black hole mergers from detailed binary evolution models
Fully-conservative BH accretion is disfavored for high-mass BBH mergers; Eddington/GRRMHD accretion with kicks can match part of the LVK high-mass population but still needs another channel.