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Electroweak resummation of neutralino dark-matter annihilation into high-energy photons

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arxiv 2211.14341 v1 pith:D7XXS5LM submitted 2022-11-25 hep-ph astro-ph.COastro-ph.HE

classification hep-phastro-ph.COastro-ph.HE
keywords photonsresummationannihilationelectroweakhigh-energymassesminimalneutralino
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abstract

We consider the resummation of large electroweak Sudakov logarithms for the annihilation of neutralino DM with $\mathcal{O}$(TeV) mass to high-energy photons in the minimal supersymmetric standard model, extending previous work on the minimal wino and Higgsino models. We find that NLL resummation reduces the yield of photons by about $20\%$ for Higgsino-dominated DM at masses around 1~TeV, and up to $45\%$ for neutralinos with larger wino admixture at heavier masses near 3~TeV. This sizable effect is relevant when observations or exclusion limits are translated into MSSM parameter-space constraints.

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    CTAO-North, using high-zenith-angle observations, could discover 1.1 TeV thermal higgsino dark matter by 2030 for several plausible Galactic Center density profiles, earlier than CTAO-South.

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