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

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

2007-12-11

arxiv.org/abs/0712.1711v2

Phys.Lett.B662:185-189,2008

Physics

High Energy Physics

High Energy Physics - Phenomenology

11 pages pdf including 2 figures. Discussion added. Final version to appear in Physics Letters B

Scientific paper

10.1016/j.physletb.2008.02.065

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.

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