Monte Carlo solutions of the Smoluchowski equation for PBH clusters yield finite runaway timescales and evolving mass distributions that form high-redshift SMBHs, shortened further by mass segregation.
Gentile et al.,Not-so-little Red Dots: Two Massive and Dusty Starbursts at z∼5–7 Pushing the Limits of Star Formation Discovered by JWST in the COSMOS-Web Survey,Astrophys
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Smoluchowski Coagulation Equation and the Evolution of Primordial Black Hole Clusters
Monte Carlo solutions of the Smoluchowski equation for PBH clusters yield finite runaway timescales and evolving mass distributions that form high-redshift SMBHs, shortened further by mass segregation.