Majorana Neutrino Mixing

Abstract

The most plausible see-saw explanation of the smallness of the neutrino masses is based on the assumption that total lepton number is violated at a large scale and neutrinos with definite masses are Majorana particles. In this review we consider in details difference between Dirac and Majorana neutrino mixing and possibilities of revealing Majorana nature of neutrinos with definite masses.

References in corpus (12)

• Measurement of Neutrino Oscillation with KamLAND: Evidence of Spectral Distortion
• Final Results from phase II of the Mainz Neutrino Mass Search in Tritium $\beta$ Decay
• Evidence for an oscillatory signature in atmospheric neutrino oscillation
• Search for neutrinoless double beta decay with enriched 76Ge in Gran Sasso 1990-2003
• Evidence for muon neutrino oscillation in an accelerator-based experiment
• Double Beta Decay
• Models of Neutrino Masses and Mixings
• A New Limit on the Neutrinoless DBD of 130Te
• Neutrinoless Double Beta Decay and Future Neutrino Oscillation Precision Experiments
• The Majorana neutrino masses, neutrinoless double beta decay and nuclear matrix elements
• Models of Neutrino Masses and Mixings
• Neutrinoless double beta decay and neutrino mass hierarchies

Cited by in corpus (6)

• Heavy Neutral Leptons at Muon Colliders
• From Generalized Dirac Equations to a Candidate for Dark Energy
• Teaching Theoretical Physics: the cases of Enrico Fermi and Ettore Majorana
• $\Delta L=2$ hyperon semileptonic decays
• Neutrino Mass Squared Differences in the Exact Solution of a 3-3-1 Gauge Model without Exotic Electric Charges
• Neutrino Helicity Reversal and Fundamental Symmetries