Neutrino flavour relaxation or neutrino oscillations?
arXiv:hep-ph/0312146 · doi:10.1134/1.1759403
Abstract
We propose the new mechanism of neutrino flavour relaxation to explain the experimentally observed changes of initial neutrino flavour fluxes. The test of neutrino relaxation hypothesis is presented, using the data of modern reactor, solar and accelerator experiments. The final choice between the standard neutrino oscillations and the proposed neutrino flavour relaxation model can be done in future experiments.
References in corpus (9)
- Evidence for oscillation of atmospheric neutrinos
- Direct Evidence for Neutrino Flavor Transformation from Neutral-Current Interactions in the Sudbury Neutrino Observatory
- First Results from KamLAND: Evidence for Reactor Anti-Neutrino Disappearance
- Indications of Neutrino Oscillation in a 250 km Long-baseline Experiment
- Solar Models: current epoch and time dependences, neutrinos, and helioseismological properties
- Search for neutrino oscillations on a long base-line at the CHOOZ nuclear power station
- Measurement of the solar neutrino capture rate with gallium metal
- GNO Solar Neutrino Observations: Results for GNOI
- Matter Effects in Upward-Going Muons and Sterile Neutrino Oscillations