Can the Super-Kamiokande Atmospheric Data Predict the Solar Neutrino Deficit ?

Details Can the Super-Kamiokande Atmospheric Data Predict the Solar Neutrino Deficit ? Can the Super-Kamiokande Atmospheric Data Predict the Solar Neutrino Deficit ?

1999-03-31

arxiv.org/abs/hep-ph/9903552v1

Mod.Phys.Lett.A14:689-700,1999

Physics

High Energy Physics

High Energy Physics - Phenomenology

LaTeX, 12 pages with 4 figures (EPS)

Scientific paper

10.1142/S0217732399000730

In this Letter we show that the evidence for neutrino oscillations from the Super-Kamiokande atmospheric neutrino data fully determines the 3x3 neutrino-oscillations mixing matrix and predicts an energy independent solar neutrino deficit at the level of 45%. This corresponds to a ratio of measured to predicted neutrino flux of R_e^{Solar} = 0.55, in good agreement with the experimental results. We achieve this result within the framework of a minimal, three-generations neutrino mixing, with mass squared differences of dM^2 = 0.45 eV^2 and dm^2 = O(10^-3) eV^2. The mixing matrix derived here is characterized by the mixing angles theta = 35.1, beta = 5.5, and psi = 23.3, and a vanishing CP-violating phase, delta = 0.

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