Dark Matter Freeze-out During Matter Domination

Fuente: arXiv
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Main Authors: Hamdan, Saleh, Unwin, James
Format: Preprint
Published: 2017
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author Hamdan, Saleh
Unwin, James
author_facet Hamdan, Saleh
Unwin, James
contents We highlight the general scenario of dark matter freeze-out whilst the energy density of the universe is dominated by a decoupled non-relativistic species. Decoupling during matter domination changes the freeze-out dynamics, since the Hubble rate is parametrically different for matter and radiation domination. Furthermore, for successful Big Bang Nucleosynthesis the state dominating the early universe energy density must decay, this dilutes (or repopulates) the dark matter. As a result, the masses and couplings required to reproduce the observed dark matter relic density can differ significantly from radiation dominated freeze-out.
format Preprint
id arxiv_https___arxiv_org_abs_1710_03758
institution arXiv
publishDate 2017
record_format arxiv
spellingShingle Dark Matter Freeze-out During Matter Domination
Hamdan, Saleh
Unwin, James
High Energy Physics - Phenomenology
Cosmology and Nongalactic Astrophysics
We highlight the general scenario of dark matter freeze-out whilst the energy density of the universe is dominated by a decoupled non-relativistic species. Decoupling during matter domination changes the freeze-out dynamics, since the Hubble rate is parametrically different for matter and radiation domination. Furthermore, for successful Big Bang Nucleosynthesis the state dominating the early universe energy density must decay, this dilutes (or repopulates) the dark matter. As a result, the masses and couplings required to reproduce the observed dark matter relic density can differ significantly from radiation dominated freeze-out.
title Dark Matter Freeze-out During Matter Domination
topic High Energy Physics - Phenomenology
Cosmology and Nongalactic Astrophysics
url https://arxiv.org/abs/1710.03758