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Gravitino Cosmology Helped by a Right Handed (S)Neutrino

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arxiv 2104.02958 v2 pith:R3PBOUM6 submitted 2021-04-07 hep-ph astro-ph.CO

classification hep-phastro-ph.CO
keywords gravitinoneutrinoright-handedcasedarkdecaydecayinglightest
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abstract

In this paper, we discuss interesting scenarios resulting from the interplay between the gravitino and the lightest right-handed (s)neutrino. We consider two gravitino mass regimes vastly separated, that is, $m_{3/2}=\mathcal{O}(100){\rm eV}$ and $m_{3/2}\simeq100{\rm GeV}$. For the former case, a significant amount of the entropy production in the cosmological history to dilute the gravitino relic abundance is unavoidable for consistency with the number of satellite galaxies in the Milky way. We will show that the right-handed (s)neutrino can play the role of the heavy particle whose late time decay provides such an additional radiation. For the later case, the gravitino of $m_{3/2}\simeq100{\rm GeV}$ may resolve the $S_{8}$ tension as a decaying dark matter. We will show how the lightest right-handed neutrino and its superpartner can help the gravitino decaying dark matter be equipped with a long enough life time and mass degeneracy with a massive decay product to address the $S_{8}$ tension.

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  1. A frequentist view on the two-body decaying dark matter model

    astro-ph.CO 2025-05 conditional novelty 6.0 of 10

    A frequentist reanalysis of Planck and KiDS-1000 data shows that a two-body decaying dark matter model can produce S8 values consistent with weak lensing surveys, and that prior choices dominated earlier Bayesian exclusions.

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