Abstract
We investigate the prospects of indirect searches for the supersymmetric neutralino dark matter with high energy neutrinos produced from neutralino annihilations in the Sun. Muon neutrinos of this origin can be seen in large detectors like the AMANDA, the IceCube, and the ANTARES. We make realistic estimates for the indirect detection rates including effects of the muon detection threshold, quark hadronization, and solar absorption. In the minimal supersymmetric model and supergravity unified models, we find good prospects for detection of neutralinos with mass above 200 GeV.
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