Flavor Neutrino Oscillations and Time-Energy Uncertainty Relation
arXiv:hep-ph/0605228 · doi:10.1088/0031-8949/2006/T127/003
Abstract
We consider neutrino oscillations as non stationary phenomenon based on Schrodinger evolution equation and mixed states of neutrinos with definite flavors. We show that time-energy uncertainty relation plays a crucial role in neutrino oscillations. We compare neutrino oscillations with oscillations.
arXiv commentA report at the 2nd Scandinavian Neutrino Workshop, SNOW 2006, Stockholm, May 2-6, 2006
References in corpus (7)
- Evidence for oscillation of atmospheric neutrinos
- Solar 8B and hep Neutrino Measurements from 1258 Days of Super-Kamiokande Data
- Indications of Neutrino Oscillation in a 250 km Long-baseline Experiment
- Neutrino Masses and Mixing: Evidence and Implications
- Solar models and solar neutrino oscillations
- What is coherent in neutrino oscillations
- Neutrino mass bounds from cosmology
Cited by in corpus (6)
- Time-energy uncertainty relation for neutrino oscillations in curved spacetime
- Flavor Energy uncertainty relations for neutrino oscillations in quantum field theory
- Some non-trivial aspects of Poincaré and CPT invariance of flavor vacuum
- On the flavor/mass dichotomy for mixed neutrinos: a phenomenologically motivated analysis based on lepton charge conservation in neutron decay
- Time-energy uncertainty relation for neutrino oscillations: historical development, applications and future prospects
- Neutrino Oscillations in Finite Time Path Out-of-Equilibrium Thermal Field Theory