Axino dark matter with low reheating temperature
Leszek Roszkowski, Sebastian Trojanowski, Krzysztof Turzynski

TL;DR
This paper investigates axino dark matter production in low reheating temperature scenarios, considering non-instantaneous reheating and entropy effects, and derives new bounds on axino mass and reheating temperature consistent with cosmological and collider data.
Contribution
It provides a comprehensive analysis of axino dark matter in low T_R regimes, including non-thermal production and entropy effects, updating previous bounds on axino mass and reheating temperature.
Findings
Upper axino mass bound depends on T_R, peaking at ~100 GeV.
Reheating temperature lower limit of ~10 GeV for wino or higgsino LSP.
Entropy production during reheating significantly alters axino mass and T_R constraints.
Abstract
We examine axino dark matter in the regime of a low reheating temperature T_R after inflation and taking into account that reheating is a non-instantaneous process. This can have a significant effect on the dark matter abundance, mainly due to entropy production in inflaton decays. We study both thermal and non-thermal production of axinos in the context of the MSSM with ten free parameters. We identify the ranges of the axino mass and the reheating temperature allowed by the LHC and other particle physics data in different models of axino interactions. We confront these limits with cosmological constraints coming the observed dark matter density, large structures formation and big bang nucleosynthesis. We find a number of differences in the phenomenologically acceptable values of the axino mass and the reheating temperature relative to previous studies. In particular, an upper bound on…
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