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Sommerfeld enhancement for puffy self-interacting dark matter

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arxiv 2308.02170 v1 pith:RUQDEAU3 submitted 2023-08-04 hep-ph astro-ph.HEhep-th

classification hep-phastro-ph.HEhep-th
keywords enhancementpuffydarkmattersommerfeldeffectfactorfind
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abstract

We examine the Sommerfeld enhancement effect for the puffy self-interacting dark matter. We find out two new parameters to classify the self-scattering cross section into the Born, the resonance and the classical regimes for the puffy dark matter. Then we observe that the resonance peaks for the puffy dark matter self-scattering and for the Sommerfeld enhancement effect have the same locations. Further, we find that for a large ratio between $R_{\chi}$ (radius of a puffy dark matter particle) and $1/m_{\phi}$ (force range), the Sommerfeld enhancement factor approaches to 1 (no enhancement). Finally, for the puffy SIDM scenario to solve the small-scale problems, the values of the Sommerfeld enhancement factor are displayed in the allowed parameter regions.

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  1. Searching for dark matter annihilating into light long-lived mediators from stars inside dwarf spheroidal galaxies

    astro-ph.HE 2025-01 conditional novelty 5.0 of 10

    Fermi-LAT observations of ten dwarf spheroidals place upper limits on dark matter-nucleon scattering by modeling stellar capture and annihilation through long-lived mediators.

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