Probing a Supersymmetric Model for Neutrino Masses at Ultrahigh Energy Neutrino Telescopes

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dc.creatorHirsch, M.
dc.creatorRoy, D. P.
dc.creatorValle, J. W. F.
dc.date2007-12-11
dc.date2008-02-28
dc.date.accessioned2026-07-07T11:39:19Z
dc.date.available2026-07-07T11:39:19Z
dc.descriptionA 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.
dc.description11 pages pdf including 2 figures. Discussion added. Final version to appear in Physics Letters B
dc.identifierhttps://arxiv.org/abs/0712.1711
dc.identifierhttp://arxiv.org/abs/0712.1711
dc.identifierPhys.Lett.B662:185-189,2008
dc.identifierdoi:10.1016/j.physletb.2008.02.065
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/199875
dc.subjectHigh Energy Physics - Phenomenology
dc.titleProbing a Supersymmetric Model for Neutrino Masses at Ultrahigh Energy Neutrino Telescopes
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