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Upward muon signals at neutrino detectors as a probe of dark matter properties
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Upward muon signals at neutrino detectors as a probe of dark matter properties
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We study upward muon flux at neutrino detectors such as Super-Kamiokande resulting from high-energy neutrinos produced by the dark matter annihilation/decay at the Galactic center. In particular, we distinguish showering and non-showering muons as their energy loss processes inside the detector, and show that this information is useful for discriminating dark matter models.
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Constraining primordial black holes and primordial curvature power spectrum with extragalactic muon neutrino
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