Fingerprints of freeze-in dark matter in an early matter-dominated era

We study the impact of an alternate cosmological history with an early matter-dominated epoch on the freeze-in production of dark matter. Such early matter domination is triggered by a meta-stable matter field dissipating into radiation. In general, the dissipation rate has a non-trivial temperat...

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Main Author: Avik Banerjee, Debtosh Chowdhury
Format: Article
Language:English
Published: SciPost 2022-08-01
Series:SciPost Physics
Online Access:https://scipost.org/SciPostPhys.13.2.022
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author Avik Banerjee, Debtosh Chowdhury
author_facet Avik Banerjee, Debtosh Chowdhury
author_sort Avik Banerjee, Debtosh Chowdhury
collection DOAJ
description We study the impact of an alternate cosmological history with an early matter-dominated epoch on the freeze-in production of dark matter. Such early matter domination is triggered by a meta-stable matter field dissipating into radiation. In general, the dissipation rate has a non-trivial temperature and scale factor dependence. Compared to the usual case of dark matter production via the freeze-in mechanism in a radiation-dominated universe, in this scenario, orders of magnitude larger coupling between the visible and the dark sector can be accommodated. Finally, as a proof of principle, we consider a specific model where the dark matter is produced by a sub-GeV dark photon having a kinetic mixing with the Standard Model photon. We point out that the parameter space of this model can be probed by the experiments in the presence of an early matter-dominated era.
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spelling doaj.art-f23d2d91f1c7497988ae710c891426652022-12-22T03:44:21ZengSciPostSciPost Physics2542-46532022-08-0113202210.21468/SciPostPhys.13.2.022Fingerprints of freeze-in dark matter in an early matter-dominated eraAvik Banerjee, Debtosh ChowdhuryWe study the impact of an alternate cosmological history with an early matter-dominated epoch on the freeze-in production of dark matter. Such early matter domination is triggered by a meta-stable matter field dissipating into radiation. In general, the dissipation rate has a non-trivial temperature and scale factor dependence. Compared to the usual case of dark matter production via the freeze-in mechanism in a radiation-dominated universe, in this scenario, orders of magnitude larger coupling between the visible and the dark sector can be accommodated. Finally, as a proof of principle, we consider a specific model where the dark matter is produced by a sub-GeV dark photon having a kinetic mixing with the Standard Model photon. We point out that the parameter space of this model can be probed by the experiments in the presence of an early matter-dominated era.https://scipost.org/SciPostPhys.13.2.022
spellingShingle Avik Banerjee, Debtosh Chowdhury
Fingerprints of freeze-in dark matter in an early matter-dominated era
SciPost Physics
title Fingerprints of freeze-in dark matter in an early matter-dominated era
title_full Fingerprints of freeze-in dark matter in an early matter-dominated era
title_fullStr Fingerprints of freeze-in dark matter in an early matter-dominated era
title_full_unstemmed Fingerprints of freeze-in dark matter in an early matter-dominated era
title_short Fingerprints of freeze-in dark matter in an early matter-dominated era
title_sort fingerprints of freeze in dark matter in an early matter dominated era
url https://scipost.org/SciPostPhys.13.2.022
work_keys_str_mv AT avikbanerjeedebtoshchowdhury fingerprintsoffreezeindarkmatterinanearlymatterdominatedera