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.
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Galaxy evolution is reframed as transport-plus-merger dynamics of a population density on a latent manifold, with all observed statistics as non-closing projections; the abstract's claimed simulation validation is absent from the body.
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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.
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Joint State-and-Dynamics Inference for Galaxy Population Evolution on an Effective Manifold
Galaxy evolution is reframed as transport-plus-merger dynamics of a population density on a latent manifold, with all observed statistics as non-closing projections; the abstract's claimed simulation validation is absent from the body.