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Indirect Search for Neutralino Dark Matter with High Energy Neutrinos
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We investigate the prospects of indirect searches for supersymmetric neutralino dark matter. Relic neutralinos gravitationally accumulate in the Sun and their annihilations produce high energy neutrinos. Muon neutrinos of this origin can be seen in large detectors like AMANDA, IceCube and ANTARES. We evaluate the relic density and the detection rate in several models---the minimal supersymmetric model, minimal supergravity, and supergravity with non-universal Higgs boson masses at the grand unification scale. We make realistic estimates for the indirect detection rates including effects of the muon detection threshold, quark hadronization, and solar absorption. We find good prospects for detection of neutralinos with mass above 200 GeV.
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Cited by 2 Pith papers
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Asteroseismological constraints on--and hints of--dark matter interactions
Dark matter heat transport can erase convective cores in solar-mass stars, yielding asteroseismic constraints on dark matter-nucleon scattering and a 4 sigma hint of dark matter-electron scattering in KIC 8228742 that...
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Searching for dark matter annihilation in the Sun with the IceCube Upgrade
Projected IceCube Upgrade sensitivity could set the strongest spin-dependent dark matter limits for masses from about 5 to 1700 GeV when dark matter annihilates to taus or neutrinos.
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