Loss-cone limited dark matter accretion onto early black hole seeds becomes supply-limited after phase-space depletion, yielding negligible sustained growth in standard NFW halos even with optimistic refilling.
Supermassive black hole growth in hierarchically merging nuclear star clusters
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Machine learning regressors trained on Rapster simulations forecast that globular clusters rarely host black holes above 100 solar masses while a few nuclear star clusters may exceed this threshold.
LGWA could observe more than one third of known binary black hole events, detect ~90 mergers per year, and measure chirp mass better than third-generation detectors for massive systems.
Dark matter clustering, possibly via self-interaction, may help stellar-remnant black holes reach over 10^7 solar masses by z=10.
citing papers explorer
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Loss-Cone-Limited Dark Matter Accretion onto Early Black Hole Seeds
Loss-cone limited dark matter accretion onto early black hole seeds becomes supply-limited after phase-space depletion, yielding negligible sustained growth in standard NFW halos even with optimistic refilling.
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Predicting intermediate-mass black hole formation in star clusters with machine learning
Machine learning regressors trained on Rapster simulations forecast that globular clusters rarely host black holes above 100 solar masses while a few nuclear star clusters may exceed this threshold.
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Gravitational-wave parameter estimation to the Moon and back: massive binaries and the case of GW231123
LGWA could observe more than one third of known binary black hole events, detect ~90 mergers per year, and measure chirp mass better than third-generation detectors for massive systems.
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Dark Matter and the Early Formation of Supermassive Black Holes
Dark matter clustering, possibly via self-interaction, may help stellar-remnant black holes reach over 10^7 solar masses by z=10.