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Gravitino dark matter and baryon asymmetry from Q-ball decay in gauge mediation

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arxiv 1107.0403 v3 pith:LZDWOIYB submitted 2011-07-02 hep-ph astro-ph.CO

classification hep-phastro-ph.CO
keywords decayq-ballasymmetrybaryondarkenoughkinematicallymatter
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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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  1. Q-ball perturbations with more details: linear analysis vs lattice

    hep-ph 2024-12 conditional novelty 6.0 of 10

    Q-ball perturbation theory is shown to remain valid for wavepacket amplitudes below about 10^-2 of the Q-ball background, and the analysis is extended to two-field FLS Q-balls.

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