Neutrinos for TeV Neutralinos
ORAL
Abstract
Dark matter remains one of the biggest open questions in particle physics. We focus on a particularly well motivated candidate to explain dark matter: the lightest neutralinos in a split supersymmetry model, and explore the signal possible from production of neutrinos in dark matter annihilations near the galactic center. Depending on the properties of the neutralino dark matter, such signals may be visible in current IceCube data, or in future neutrino telescopes.
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Presenters
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Benjamin J Sheff
University of Utah
Authors
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Benjamin J Sheff
University of Utah
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Pearl Sandick
University of Utah
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Carsten Rott
University of Utah, Sungkyunkwan University, Suwon, Korea