Seesaw mechanism in three flavors
arXiv:hep-ph/0103147 · doi:10.1103/PhysRevD.65.013002
Abstract
We advance a method used to analyse the neutrino properties (masses and mixing) in the seesaw mechanism. Assuming the hierarchical Dirac and light neutrino masses we establish rather simple relations between the light and the heavy neutrino parameters in the favored region of the solar and the atmospheric neutrino experiments. A empirical condition satisfied by the RH mixing angles is obtained.
arXiv comment19 pages. Acceptted by Phys. Rev. D The part about the neutrino experiments is selected as a single section. The mistakes in spelling and grammer are corrected. Also, some equations are neewly numbered
References in corpus (18)
- Evidence for oscillation of atmospheric neutrinos
- Limits on Neutrino Oscillations from the CHOOZ Experiment
- Measurements of the Solar Neutrino Flux from Super-Kamiokande's First 300 Days
- Mass and Flavor Mixing Schemes of Quarks and Leptons
- Where do we stand with solar neutrino oscillations?
- Updated Estimate of Running Quark Masses
- See-saw Enhancement of Lepton Mixing
- Large Neutrino Mixing from Small Quark and Lepton Mixings
- Neutrinos in Physics and Astrophysics
- Stability of the Lepton-Flavor Mixing Matrix Against Quantum Corrections
- Neutrino masses and mixing with seesaw mechanism and universal breaking of extended democracy
- Linking solar and long baseline terrestrial neutrino experiments
- See-saw Enhancement of Neutrino Mixing due to the Right-handed Phases
- Neutrino Mass Texture with Large Mixing
- Mass Hierarchies and the Seesaw Neutrino Mixing
- Seesaw model and its Lorentz group formulation
- Neutrino masses and mixings in a seesaw framework
- Natural Neutrino Mass Matrix