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Aspects of Spatially-Correlated Random Fields: Extreme-Value Statistics and Clustering Properties (2501.17936v1)

Published 29 Jan 2025 in astro-ph.CO, gr-qc, hep-ph, and physics.data-an

Abstract: Rare events of large-scale spatially-correlated exponential random fields are studied. The influence of spatial correlations on clustering and non-sphericity is investigated. The size of the performed simulations permits to study beyond-$7.5$-sigma events ($1$ in $10{13}$). As an application, this allows to resolve individual Hubble patches which fulfill the condition for primordial black hole formation. It is argued that their mass spectrum is drastically altered due to co-collapse of clustered overdensities as well as the mutual threshold-lowering through the latter. Furthermore, the corresponding non-sphericities imply possibly large changes in the initial black hole spin distribution.

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