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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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dc.contributor.author Hirsch, Martin
dc.contributor.author Roy, Durga Prasad
dc.contributor.author Furtado Valle, José Wagner
dc.date.accessioned 2014-08-25T09:22:16Z
dc.date.available 2014-08-25T09:22:16Z
dc.date.issued 2008
dc.identifier.citation 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
dc.identifier.uri http://hdl.handle.net/10550/37375
dc.description.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-km(3) size neutrino telescope.
dc.language.iso eng
dc.relation.ispartof Physics Letters B, 2008, vol. 662, num. 2, p. 185-189
dc.subject Física
dc.title Probing a supersymmetric model for neutrino masses at ultrahigh energy neutrino telescopes
dc.type journal article es_ES
dc.date.updated 2014-08-25T09:22:16Z
dc.identifier.doi 10.1016/j.physletb.2008.02.065
dc.identifier.idgrec 048296
dc.rights.accessRights open access es_ES

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