Excited dark matter that is stable in vacuum can decay near Earth into two fast muons, giving neutrino telescopes a nearly background-free signal.
Sensitivity Projections for Low-Mass Dark Matter Annihilation with the IceCube Upgrade
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abstract
The IceCube Upgrade, an extension designed to enhance the IceCube Neutrino Observatory's detection of neutrinos with energies between 1 GeV and 500 GeV, will markedly improve IceCube's sensitivity to low-mass dark matter scenarios. In this study, we present sensitivity projections for the IceCube Upgrade to neutrino fluxes arising from dark matter annihilation. In particular, we consider dark matter with masses between 3 GeV to 500 GeV from both the core of the Sun and the Galactic Center. These projections indicate that the IceCube Upgrade will enable stringent limits on dark matter in this parameter space, achieving leading sensitivities to some dark matter models with only three years of data taking.
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Novel Signatures of Matter-Induced Dark Matter Decay in Large-Volume Neutrino Telescopes
Excited dark matter that is stable in vacuum can decay near Earth into two fast muons, giving neutrino telescopes a nearly background-free signal.