Solar Neutrinos with Three Flavor Mixings
arXiv:hep-ph/9208241 · doi:10.1103/PhysRevD.47.4059
Abstract
The recent 71Ga solar neutrino observation is combined with the 37Cl and Kamiokande-II observations in an analysis for neutrino masses and mixings. The allowed parameter region is found for matter enhanced mixings among all three neutrino flavors. Distortions of the solar neutrino spectrum unique to three flavors are possible and may be observed in continuing and next generation experiments.
August 1992 (Revised) PURD-TH-92-8
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- A Possible Violation of the Equivalence Principle by Neutrinos
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- Constraints on Three-Neutrino Mixing from Atmospheric and Reactor Data
- Neutrinos with Zee-Mass Matrix in Vacuum and Matter
- Common Origin for the Solar and Atmospheric Neutrino Deficits
- Possible Revelation of Seesaw Mass Pattern in Solar and Atmospheric Neutrino Data
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- Some consequences in weak processes of three generations mixing in the leptonic sector
- PEANUTS: a software for the automatic computation of solar neutrino flux and its propagation within Earth
- The Earth Regeneration Effect of Solar Neutrinos: a Numerical Treatment with Three Active Neutrino Flavors