Neutrino Masses at v^{3/2}
arXiv:hep-ph/0007001
Abstract
Theories in which neutrino masses are generated by a conventional see-saw mechanism generically yield masses which are O(v^2) in units where M_{Pl}=1, which is naively too small to explain the results from SuperKamiokande. In supersymmetric theories with gravity mediated supersymmetry breaking, the fundamental small parameter is not v/M_{Pl}, but m_I/M_{Pl}, where m_I is the scale of supersymmetry breaking in the hidden sector. We note that m_I^3/M_{Pl}^2 is only slightly too large to explain SuperKamiokande, and present two models that achieve neutrino masses at this order in m_I, one of which has an additional suppression lambda_tau^2, while the other has additional suppression arising from a loop factor. The latter model shares a great deal of phenomenology with a class of models previously explored, including the possibility of viable sneutrino dark matter.
arXiv commentMinor revisions, 4 pages, RevTeX
Cited by in corpus (10)
- Dark Energy from Mass Varying Neutrinos
- Asymmetric Sneutrino Dark Matter and the Omega(b)/Omega(DM) Puzzle
- Direct Detection of Leptophilic Dark Matter in a Model with Radiative Neutrino Masses
- R Symmetry and the Mu Problem
- Neutrino Mass, Sneutrino Dark Matter and Signals of Lepton Flavor Violation in the MRSSM
- Naturally Degenerate Right Handed Neutrinos
- Phenomenology of SUSY SU(5) GUT with neutrinophilic Higgs
- Bilarge neutrino mixing from supersymmetry with high-scale nonrenormalizable interactions
- Asymmetric Sneutrino Dark Matter
- Mixed Sneutrino Dark Matter and the Ratio Omega(b)/Omega(dm)