Gravitino dark matter and baryon asymmetry from Q-ball decay in gauge mediation
Shinta Kasuya, Masahiro Kawasaki

TL;DR
This paper explores how Q-ball decay in gauge-mediated SUSY breaking can produce the observed baryon asymmetry and dark matter without conflicting with cosmological constraints, by analyzing decay channels and charge conditions.
Contribution
It provides a detailed analysis of Q-ball decay channels and conditions that yield correct baryon asymmetry and dark matter abundance while avoiding cosmological constraints.
Findings
Q-balls decay mainly into nucleons and gravitinos.
Decay channels are controlled by Q-ball charge size.
The model evades constraints from big bang nucleosynthesis.
Abstract
We investigate the Q-ball decay in the gauge-mediated SUSY breaking. Q balls decay mainly into nucleons, and partially into gravitinos, while they are kinematically forbidden to decay into sparticles which would be cosmologically harmful. This is achieved by the Q-ball charge small enough to be unstable for the decay, and large enough to be protected kinematically from unwanted decay channel. We can then have right amounts of the baryon asymmetry and the dark matter of the universe, evading any astrophysical and cosmological observational constraints such as the big bang nucleosynthesis, which has not been treated properly in the literatures.
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