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Probing a supersymmetric model for neutrino masses at ultrahigh energy neutrino telescopes
Authors:M Hirsch  DP Roy  JWF Valle
Institution:1. AHEP Group, Instituto de Fisica Corpuscular (IFIC), CSIC-U. de Valencia, Edificio de Instituto de Paterna, Apartado de Correos 22085, E-46071 Valencia, Spain;2. Homi Bhabha Centre for Science Education, Tata Institute of Fundamental Research, Mumbai 400088, India
Abstract:A bilinear R-parity breaking SUSY model for neutrino mass and mixing predicts the lightest superparticle to decay mainly into a pair of tau leptons or b quarks along with a neutrino for relatively light SUSY spectra. This leads to a distinctive triple bang signature of SUSY events at ultrahigh energy neutrino telescopes like IceCube or Antares. While the expected signal size is only marginal at IceCube, it will be promising for a future multi-km3 size neutrino telescope.
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