Probing a supersymmetric model for neutrino masses at ultrahigh energy neutrino telescopes
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Probing a supersymmetric model for neutrino masses at ultrahigh energy neutrino telescopes

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Probing a supersymmetric model for neutrino masses at ultrahigh energy neutrino telescopes

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Hirsch, Martin; Roy, Durga Prasad; Furtado Valle, José Wagner Perfil
Aquest document és un/a article, creat/da en: 2008
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-km(3) size neutrino telescope.

    Hirsch, Martin Roy, Durga Prasad Furtado Valle, José Wagner 2008 Probing a supersymmetric model for neutrino masses at ultrahigh energy neutrino telescopes Physics Letters B 662 2 185 189
http://dx.doi.org/10.1016/j.physletb.2008.02.065
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