Journal
JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS
Volume -, Issue 3, Pages -Publisher
IOP Publishing Ltd
DOI: 10.1088/1475-7516/2022/03/016
Keywords
dark matter theory; inflation; physics of the early universe
Funding
- European Union [860881-HIDDeN]
- CNRS PICS MicroDark
- IN2P3 master project UCMN
- research grant The Dark Universe: A Synergic Multi-messenger Approach - Ministero dell'Istruzione, Universita e della Ricerca (MIUR) [2017X7X85K]
- Istituto Nazionale di Fisica Nucleare (INFN) through the Theoretical Astroparticle Physics (TAsP) project
- Spanish Agencia Estatal de Investigacion [FPA2015-65929-P, PGC2018095161-B-I00]
- IFT Centro de Excelencia Severo Ochoa [SEV-2016-0597]
- Red Consolider MultiDark [FPA2017-90566-REDC]
- MCIU (Spain) [PGC2018-096646-A-I00]
- DOE at the University of Minnesota [DE-SC0011842]
- JSPS Kakenhi [19H01899]
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This article investigates the production of dark matter during the process of reheating after inflation. By comparing perturbative and non-perturbative calculations of energy density and considering the instability of final state scalar products, the resulting relic density based on different approaches is compared. It is shown that the present-day cold dark matter density can be obtained through freeze-in from preheating for a large range of dark matter masses.
We consider the production of dark matter during the process of reheating after inflation. The relic density of dark matter from freeze-in depends on both the energy density and energy distribution of the inflaton scattering or decay products composing the radiation bath. We compare the perturbative and non-perturbative calculations of the energy density in radiation. We also consider the (likely) possibility that the final state scalar products are unstable. Assuming either thermal or non-thermal energy distribution functions, we compare the resulting relic density based on these different approaches. We show that the present-day cold dark matter density can be obtained through freeze-in from preheating for a large range of dark matter masses.
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