Abundance of primordial black holes with local non-Gaussianity in peak theory

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Hauptverfasser: Yoo, Chul-Moon, Gong, Jinn-Ouk, Yokoyama, Shuichiro
Format: Preprint
Veröffentlicht: 2019
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author Yoo, Chul-Moon
Gong, Jinn-Ouk
Yokoyama, Shuichiro
author_facet Yoo, Chul-Moon
Gong, Jinn-Ouk
Yokoyama, Shuichiro
contents We discuss the effect of local type non-Gaussianity on the abundance of primordial black holes (PBH) based on the peak theory. We provide the PBH formation criterion based on the so-called compaction function and use the peak theory statistics associated with the curvature perturbation with the local type non-Gaussianity. Providing a method to estimate the PBH abundance, we demonstrate the effects of non-Gaussianity. It is explicitly shown that the value of non-linear parameter $|f_{\rm NL}| \sim 1$ induces a similar effect to a few factors of difference in the amplitude of the power spectrum.
format Preprint
id arxiv_https___arxiv_org_abs_1906_06790
institution arXiv
publishDate 2019
record_format arxiv
spellingShingle Abundance of primordial black holes with local non-Gaussianity in peak theory
Yoo, Chul-Moon
Gong, Jinn-Ouk
Yokoyama, Shuichiro
Cosmology and Nongalactic Astrophysics
General Relativity and Quantum Cosmology
We discuss the effect of local type non-Gaussianity on the abundance of primordial black holes (PBH) based on the peak theory. We provide the PBH formation criterion based on the so-called compaction function and use the peak theory statistics associated with the curvature perturbation with the local type non-Gaussianity. Providing a method to estimate the PBH abundance, we demonstrate the effects of non-Gaussianity. It is explicitly shown that the value of non-linear parameter $|f_{\rm NL}| \sim 1$ induces a similar effect to a few factors of difference in the amplitude of the power spectrum.
title Abundance of primordial black holes with local non-Gaussianity in peak theory
topic Cosmology and Nongalactic Astrophysics
General Relativity and Quantum Cosmology
url https://arxiv.org/abs/1906.06790