We calculate the formation probability of primordial black holes generated during the collapse at horizon re-entry of large fluctuations produced during inflation, such as those ascribed to a period of ultra-slow-roll. We show that it interpolates between a Gaussian at small values of the average density contrast and a Cauchy probability distribution at large values. The corresponding abundance of primordial black holes may be larger than the Gaussian one by several orders of magnitude. The mass function is also shifted towards larger masses.

The formation probability of primordial black holes / Biagetti, Matteo; De Luca, V.; Franciolini, G.; Kehagias, A.; Riotto, A.. - In: PHYSICS LETTERS. SECTION B. - ISSN 0370-2693. - 820:(2021). [10.1016/j.physletb.2021.136602]

The formation probability of primordial black holes

Franciolini G.;Riotto A.
2021

Abstract

We calculate the formation probability of primordial black holes generated during the collapse at horizon re-entry of large fluctuations produced during inflation, such as those ascribed to a period of ultra-slow-roll. We show that it interpolates between a Gaussian at small values of the average density contrast and a Cauchy probability distribution at large values. The corresponding abundance of primordial black holes may be larger than the Gaussian one by several orders of magnitude. The mass function is also shifted towards larger masses.
2021
primordial black holes
01 Pubblicazione su rivista::01a Articolo in rivista
The formation probability of primordial black holes / Biagetti, Matteo; De Luca, V.; Franciolini, G.; Kehagias, A.; Riotto, A.. - In: PHYSICS LETTERS. SECTION B. - ISSN 0370-2693. - 820:(2021). [10.1016/j.physletb.2021.136602]
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11573/1643214
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