Sommerfeld enhancement for puffy self-interacting dark matter

Journal of High Energy Physics(2024)

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Abstract
bstract 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 χ (radius of a puffy dark matter particle) and 1/ m ϕ (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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Cosmology of Theories BSM,Particle Nature of Dark Matter
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