Dark matter clustering, possibly via self-interaction, may help stellar-remnant black holes reach over 10^7 solar masses by z=10.
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2 Pith papers cite this work, alongside 5 external citations. Polarity classification is still indexing.
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UNVERDICTED 2representative citing papers
High-resolution simulations produce compact galaxies where gas inflows and dynamical processes accumulate enough mass in 10 Myr to form ~10^6 solar mass central black holes under 10% feedback efficiency.
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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.
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Little Red Dot progenitors from Compact Starbursts: A Natural Path to Early AGN Formation
High-resolution simulations produce compact galaxies where gas inflows and dynamical processes accumulate enough mass in 10 Myr to form ~10^6 solar mass central black holes under 10% feedback efficiency.