Model of Four Light Neutrinos in the Light of All Present Data
arXiv:hep-ph/9504342 · doi:10.1103/PhysRevD.52.R4780
Abstract
Motivated by existing and recent data on possible neutrino oscillations, we propose a model of four light neutrinos ($ν_e, ν_μ, ν_Ï$, and a singlet $ν_S$) with a pattern of masses and mixing derivable from a $Z_5$ discrete symmetry and the seesaw mechanism. Atmospheric neutrino oscillations occur between $ν_μ$ and $ν_Ï$ as pseudo-Dirac partners; whereas solar neutrino oscillations occur between $ν_e$ and $ν_S$, a linear combination of which is massless. Additional oscillations may occur between $ν_e$ and $ν_μ$ to account for the recent observation of the LSND (Liquid Scintillator Neutrino Detector) experiment.
Title changed, new (penultimate) paragraph added, Ref.[7] expanded, 12 pages, no figure