Non-Gaussian Formation of Primordial Black Holes: Effects on the Threshold
arXiv:1906.07135 · doi:10.1088/1475-7516/2019/12/029
Abstract
Primordial black holes could have been formed in the early universe from sufficiently large cosmological perturbations re-entering the horizon when the Universe is still radiation dominated. These originate from the spectrum of curvature perturbations generated during inflation at small-scales. Because of the non-linear relation between the curvature perturbation and the overdensity , the formation of the primordial black holes is affected by intrinsic non-Gaussianity even though the curvature perturbation is Gaussian. We investigate the impact of this non-Gaussianity on the critical threshold which measures the excess of mass of the perturbation, finding a relative change with respect to the value obtained using a linear relation between and , of a few percent. This shows that the value of the critical threshold is rather robust against non-linearities. The same holds also when cosmologically interesting values of local primordial non-Gaussianity are added to the curvature perturbation.
24 pages, 6 figures. This last updated version contains minor fine-tunings according to the published one
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