Neutrino Flavor Mixing Constrained by Accelerator and Reactor Experiments and Solar Neutrino Observation

Details Neutrino Flavor Mixing Constrained by Accelerator and Reactor Experiments and Solar Neutrino Observation Neutrino Flavor Mixing Constrained by Accelerator and Reactor Experiments and Solar Neutrino Observation

1995-04-05

arxiv.org/abs/hep-ph/9504222v2

Phys.Lett.B356:61-67,1995

Physics

High Energy Physics

High Energy Physics - Phenomenology

13 pages, REVTeX, no figures, slightly revised with no change in conclusion

Scientific paper

10.1016/0370-2693(95)00788-M

We derive the constraints imposed on neutrino masses and mixing angles by performing a combined analysis of the data from the Los Alamos and the other terrestrial neutrino oscillation experiments with the assumption of the flavor-mixing solutions to the solar neutrino problem. In a three-flavor mixing scheme which ignores the possibility of sterile neutrinos, we obtain severe constraints on the pattern of masses and flavor mixing of neutrinos. For example, we show that in the standard Kobayashi-Maskawa type mixing matrix $s_{13}^2 \lsim 10^{-2}$ independent of the choice of the solar neutrino solutions. The constraint from the double $\beta$ decay is also discussed.

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