Neutrino Anomalies and Quasi-Dirac neutrinos
arXiv:hep-ph/0110272 · doi:10.1103/PhysRevD.65.073025
Abstract
We discuss possibility of describing solar, atmospheric and LSND results with four neutrinos forming two quasi-degenerate pairs. The simplest versions of this 2+2 scheme with either or mixing exclusively with sterile neutrino is disfavored by the SNO and atmospheric neutrino results respectively. A generalized scheme with sterile state participating in both the solar and atmospheric oscillations is still allowed. We show thasolar and atmospheric oscillations is still allowed. We show that the complex pattern of mixing needed for this purpose follows from a simple L_e+L_μ-L_τ-L_s symmetry. Specific form of L_e+L_μ-L_τ-L_s symmetric mass matrix is determined from experimental results. Two theoretical schemes which lead to this form and a proper breaking of L_e+L_μ-L_τ-L_s symmetry are discussed.
15 pages, LATEX, minor corrections; addition of few references
References in corpus (12)
- Measurement of the rate of nu_e + d --> p + p + e^- interactions produced by 8B solar neutrinos at the Sudbury Neutrino Observatory
- Constraints on Neutrino Oscillations Using 1258 Days of Super-Kamiokande Solar Neutrino Data
- Global Analysis of Solar Neutrino Oscillations Including SNO CC Measurement
- Softly broken lepton numbers and maximal neutrino mixing
- Unknowns after the SNO Charged-Current Measurement
- Impact of the first SNO results on Neutrino Mass and Mixing
- 4-Neutrino mass schemes and the likelihood of (3+1)-mass spectra
- Connecting bimaximal neutrino mixing to a light sterile neutrino
- Cornering (3+1) sterile neutrino schemes
- Bayesian View Of Solar Neutrino Oscillations
- L_e + L_μ- L_τ- L_s Symmetry and a Mixed 2+2 Scenario for Neutrino Oscillations
- Neutrino anomalies and large extra dimensions
Cited by in corpus (5)
- Status of four-neutrino mass schemes: a global and unified approach to current neutrino oscillation data
- Constraining Mass Spectra with Sterile Neutrinos from Neutrinoless Double Beta Decay, Tritium Beta Decay and Cosmology
- Quasi Dirac neutrino oscillations
- Three Generation Neutrino Oscillation Parameters after SNO
- Quasi-Dirac neutrino oscillations at DUNE and JUNO