Constraining Primordial Black Hole Formation from Single-Field Inflation

Fuente: arXiv
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Autores principales: Kristiano, Jason, Yokoyama, Jun'ichi
Formato: Preprint
Publicado: 2022
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author Kristiano, Jason
Yokoyama, Jun'ichi
author_facet Kristiano, Jason
Yokoyama, Jun'ichi
contents The most widely studied formation mechanism of a primordial black hole is collapse of large-amplitude perturbation on small scales generated in single-field inflation. In this Letter, we calculate one-loop correction to the large-scale power spectrum in a model with sharp transition of the second slow-roll parameter. We find that models producing an appreciable amount of primordial black holes induce nonperturbative coupling on a large scale probed by cosmic microwave background radiation. Our result implies that a small-scale power spectrum can be constrained by large-scale cosmological observations.
format Preprint
id arxiv_https___arxiv_org_abs_2211_03395
institution arXiv
publishDate 2022
record_format arxiv
spellingShingle Constraining Primordial Black Hole Formation from Single-Field Inflation
Kristiano, Jason
Yokoyama, Jun'ichi
High Energy Physics - Theory
Cosmology and Nongalactic Astrophysics
The most widely studied formation mechanism of a primordial black hole is collapse of large-amplitude perturbation on small scales generated in single-field inflation. In this Letter, we calculate one-loop correction to the large-scale power spectrum in a model with sharp transition of the second slow-roll parameter. We find that models producing an appreciable amount of primordial black holes induce nonperturbative coupling on a large scale probed by cosmic microwave background radiation. Our result implies that a small-scale power spectrum can be constrained by large-scale cosmological observations.
title Constraining Primordial Black Hole Formation from Single-Field Inflation
topic High Energy Physics - Theory
Cosmology and Nongalactic Astrophysics
url https://arxiv.org/abs/2211.03395