Dark Matter from Eternity

Fuente: arXiv
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Autores principales: Franciolini, G., Peloso, M., Riotto, A.
Formato: Preprint
Publicado: 2026
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author Franciolini, G.
Peloso, M.
Riotto, A.
author_facet Franciolini, G.
Peloso, M.
Riotto, A.
contents We propose that the totality of dark matter in the universe might ascribe its origin to one of the key properties of cosmological inflation, that it may be eternal: regions that at the end of the primordial accelerated expansion of the universe never reheated, but keep eternally inflating, manifest themselves as primordial black holes in our observable universe. This mechanism can provide a primordial black hole abundance which is larger than the standard one due to the gravitational collapse of sizeable overdensities in the radiation phase. It also predicts a broad spectrum for the curvature perturbation and a flat stochastic gravitational wave background at a level of $Ω_\text{GW} h^2 \simeq 10^{-10}$ up to the mHz.
format Preprint
id arxiv_https___arxiv_org_abs_2602_08338
institution arXiv
publishDate 2026
record_format arxiv
spellingShingle Dark Matter from Eternity
Franciolini, G.
Peloso, M.
Riotto, A.
Cosmology and Nongalactic Astrophysics
General Relativity and Quantum Cosmology
High Energy Physics - Phenomenology
We propose that the totality of dark matter in the universe might ascribe its origin to one of the key properties of cosmological inflation, that it may be eternal: regions that at the end of the primordial accelerated expansion of the universe never reheated, but keep eternally inflating, manifest themselves as primordial black holes in our observable universe. This mechanism can provide a primordial black hole abundance which is larger than the standard one due to the gravitational collapse of sizeable overdensities in the radiation phase. It also predicts a broad spectrum for the curvature perturbation and a flat stochastic gravitational wave background at a level of $Ω_\text{GW} h^2 \simeq 10^{-10}$ up to the mHz.
title Dark Matter from Eternity
topic Cosmology and Nongalactic Astrophysics
General Relativity and Quantum Cosmology
High Energy Physics - Phenomenology
url https://arxiv.org/abs/2602.08338