Solar Neutrino Data, Solar Model Uncertainties and Neutrino Oscillations
arXiv:hep-ph/9210221 · doi:10.1016/0370-2693(93)90888-O
Abstract
We incorporate all existing solar neutrino flux measurements and take solar model flux uncertainties into account in deriving global fits to parameter space for the MSW and vacuum solutions of the solar neutrino problem.
10 pages, latex, 3 figures (not included)
References in corpus (1)
Cited by in corpus (23)
- Effects of neutrino mixing on high-energy cosmic neutrino flux
- See-saw Enhancement of Lepton Mixing
- Solar Model Uncertainties, MSW Analysis, and Future Solar Neutrino Experiments
- Coherence Effects in Neutrino Oscillations
- Astrophysical Solutions are Incompatible with the Solar Neutrino Data
- Quantifying uncertainties in primordial nucleosynthesis without Monte Carlo simulations
- Is Large Lepton Mixing Excluded?
- On The Vacuum Oscillation Solution of The Solar Neutrino Problem
- Neutrino masses from U(1) symmetries and the Super-Kamiokande data
- Testing the Vacuum Oscillation and the MSW Solutions of the Solar Neutrino Problem
- Short-baseline neutrino oscillations and neutrinoless double-beta decay in the framework of three neutrino mixing and a mass hierarchy
- Anomalous diffusion modifies solar neutrino fluxes
- Atmospheric Neutrino Problem in Maximally-Mixed Three Generations of Neutrinos
- The Earth Effect in the MSW Analysis of the Solar Neutrino Experiments
- Sterile Neutrinos and Future Solar Neutrino Experiments
- On the MSW transition solution of the solar neutrino problem
- Treating Solar Model Uncertainties: A Consistent Statistical Analysis of Solar Neutrino Models and Data
- Common Origin for the Solar and Atmospheric Neutrino Deficits
- Future Oscillation Experiments and Present Data
- Solar Neutrinos: What We Have Learned
- A Model Independent Analysis of Solar Neutrino Data
- Neutrinos Mass and Mixing
- Neutrino Mixing and Future Solar Neutrino Experiments