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Limits on Kaluza-Klein dark matter annihilation in the Sun from recent IceCube results

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arxiv 1912.04585 v1 pith:JYBMFLH4 submitted 2019-12-10 astro-ph.HE hep-ex

classification astro-ph.HEhep-ex
keywords resultsicecubekaluza-kleinannihilationdarklimitsmassesmatter
verification ladder T0 review T1 audit T2 compute T3 formal
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abstract

We interpret recent IceCube results on searches for dark matter accumulated in the sun in terms of the lightest Kaluza-Klein excitation (assumed here to be the Kaluza-Klein photon, $B^1$), obtaining improved limits on the annihilation rate in the Sun, the resulting neutrino flux at the Earth and on the $B^1$-proton cross-sections, for $B^1$ masses in the range 30--3000 GeV. These results improve previous results from IceCube in its 22-string configuration by up to an order of magnitude, depending on mass, but also extend the results to $B^1$ masses as low as 30 GeV.

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  1. Revisiting Universal Extra-Dimension Model with Gravity Mediated Decays

    hep-ph 2024-12 conditional novelty 5.0 of 10

    Existing LHC data exclude fat-brane mUED compactification scales below about 3 TeV, and ML-tagged searches at 500 fb^-1 could extend the reach to roughly 3.2 to 3.4 TeV.

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