Interplay of Non-Relativistic and Relativistic Effects in Neutrino Oscillations
arXiv:hep-ph/9702308 · doi:10.1103/PhysRevD.56.1698
Abstract
A theoretical structure that involves neutrino mass eigenstates at non relativistic as well as relativistic energies is presented. Using this framework, we find that if the particle X, with mass 33.9 MeV, of the KARMEN collaboration anomaly is identified with the third neutrino mass eigenstate, then the present limit of 23 MeV upper bound on the tau neutrino mass implies |U_{τ3}| < 0.82.
Revtex 3.0, 12 pages
References in corpus (1)
Cited by in corpus (15)
- Oscillations of neutrinos and mesons in quantum field theory
- Heavy sterile neutrinos: Bounds from big-bang nucleosynthesis and SN 1987A
- Testing violations of special and general relativity through the energy dependence of nu_mu<--->nu_tau oscillations in the Super-Kamiokande atmospheric neutrino experiment
- L/E-Flatness of the Electron-Like Event Ratio in Super-Kamiokande and a Degeneracy in Neutrino Masses
- Cosmological and astrophysical bounds on a heavy sterile neutrino and the KARMEN anomaly
- Sterile neutrinos in tau lepton decays
- Interplay of gravitation and linear superposition of different mass eigenstates
- Multi-Angle Simulation of Flavor Evolution in the Neutrino Neutronization Burst From an O-Ne-Mg Core-Collapse Supernova
- Quantum Coherence of Relic Neutrinos
- Remarks upon the mass oscillation formulas
- Nuclear weak interaction rates in primordial nucleosynthesis
- Do non-relativistic neutrinos oscillate?
- Notes on the Kinematic Structure of the Three-Flavor Neutrino Oscillation Framework
- Can the Super-Kamiokande Atmospheric Data Predict the Solar Neutrino Deficit ?
- Quantum measurement schemes related to flavor-weighted energies