Primordial black hole formation in the radiative era: investigation of the critical nature of the collapse
Ilia Musco, John C. Miller, Alexander G. Polnarev

TL;DR
This study investigates whether primordial black hole formation in the early universe's radiative era exhibits critical collapse behavior, using advanced simulations to analyze near-threshold perturbations and scaling laws.
Contribution
It demonstrates that primordial black hole formation follows a continuous scaling law down to very small masses, challenging previous findings of shock-induced deviations.
Findings
Scaling-law behavior persists at small black hole masses
No evidence of shock production in the collapse process
Results depend on initial conditions used in simulations
Abstract
Following on after two previous papers discussing the formation of primordial black holes in the early universe, we present here results from an in-depth investigation of the extent to which primordial black hole formation in the radiative era can be considered as an example of the critical collapse phenomenon. We focus on initial supra-horizon-scale perturbations of a type which could have come from inflation, with only a growing component and no decaying component. In order to study perturbations with amplitudes extremely close to the supposed critical limit, we have modified our previous computer code with the introduction of an adaptive mesh refinement scheme. This has allowed us to follow black hole formation from perturbations whose amplitudes are up to eight orders of magnitude closer to the threshold than we could do before. We find that scaling-law behaviour continues down to…
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