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Main Authors: Silva-Malpartida, Javier, Bernal, Nicolás, Jones-Pérez, Joel, Lineros, Roberto A.
Format: Preprint
Published: 2024
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Online Access:https://arxiv.org/abs/2408.08950
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author Silva-Malpartida, Javier
Bernal, Nicolás
Jones-Pérez, Joel
Lineros, Roberto A.
author_facet Silva-Malpartida, Javier
Bernal, Nicolás
Jones-Pérez, Joel
Lineros, Roberto A.
contents In the context of non-standard cosmologies, an early matter-dominated (EMD) era can significantly alter the conventional dark matter (DM) genesis. In this work, we reexamine the impact of an EMD on the weakly- and feebly-interacting massive particle (WIMP and FIMP) paradigms. EMD eras significantly modify the genesis of DM because of the change in the Hubble expansion rate and the injection of entropy. The WIMP paradigm can be realized with couplings much smaller than in the standard cosmological scenario, whereas much larger couplings are required in the FIMP case. Using the singlet-scalar DM model as a case study, we show that these results can lead to a continuous transition between the WIMP and FIMP scenarios, with results that are also applicable to other DM models. This broadens the parameter space consistent with observed DM levels and suggests that even elusive FIMP scenarios may be within the reach of future experimental searches.
format Preprint
id arxiv_https___arxiv_org_abs_2408_08950
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle From WIMPs to FIMPs: Impact of Early Matter Domination
Silva-Malpartida, Javier
Bernal, Nicolás
Jones-Pérez, Joel
Lineros, Roberto A.
High Energy Physics - Phenomenology
In the context of non-standard cosmologies, an early matter-dominated (EMD) era can significantly alter the conventional dark matter (DM) genesis. In this work, we reexamine the impact of an EMD on the weakly- and feebly-interacting massive particle (WIMP and FIMP) paradigms. EMD eras significantly modify the genesis of DM because of the change in the Hubble expansion rate and the injection of entropy. The WIMP paradigm can be realized with couplings much smaller than in the standard cosmological scenario, whereas much larger couplings are required in the FIMP case. Using the singlet-scalar DM model as a case study, we show that these results can lead to a continuous transition between the WIMP and FIMP scenarios, with results that are also applicable to other DM models. This broadens the parameter space consistent with observed DM levels and suggests that even elusive FIMP scenarios may be within the reach of future experimental searches.
title From WIMPs to FIMPs: Impact of Early Matter Domination
topic High Energy Physics - Phenomenology
url https://arxiv.org/abs/2408.08950