Physics – High Energy Physics – High Energy Physics - Phenomenology
Scientific paper
2000-09-15
Phys.Lett.B511:119-128,2001
Physics
High Energy Physics
High Energy Physics - Phenomenology
10 pages, 4 figures
Scientific paper
10.1016/S0370-2693(01)00629-3
Accumulation and annihilation of weakly interacting massive particles (WIMPs) in the earth and the sun may be observed by the resulting neutrino signal. We demonstrate that, for certain parts of the SUSY parameter space, present and future neutrino telescopes can expect a higher rate of events due to tau-neutrinos than of events due to muon-neutrinos. We show how $\nu_{\tau}\leftrightarrow\nu_{\mu}$ oscillations, and in the case of the sun also scattering, absorption and regeneration, modify the signal expectation. We find that most currently proposed neutralino models predict equal or increased muon fluxes if $\nu_{\tau}\leftrightarrow\nu_{\mu}$ oscillations are included.
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