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arXiv · hep-ph/0001101

Four--Neutrino Oscillation Solutions of the Solar Neutrino Problem

C. Giunti·M. C. Gonzalez-Garcia·C. Peña-Garay
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Abstract

We present an analysis of the neutrino oscillation solutions of the solar neutrino problem in the framework of four-neutrino mixing where a sterile neutrino is added to the three standard ones. We perform a fit to the full data set corresponding to the 825-day Super-Kamiokande data sample as well as to Chlorine, GALLEX and SAGE and Kamiokande experiments. In our analysis we use all measured total event rates as well as all Super-Kamiokande data on the zenith angle dependence and the recoil electron energy spectrum. We consider both transitions via the Mikheyev-Smirnov-Wolfenstein (MSW) mechanism as well as oscillations in vacuum (just-so) and find the allowed solutions for different values of the additional mixing angles. This framework permits transitions into active or sterile neutrinos controlled by the additional parameter $\cos^2(\vartheta_{23}) \cos^2(\vartheta_{24})$ . We discuss the maximum allowed values of this additional mixing parameter for the different solutions.

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C. Giunti, M. C. Gonzalez-Garcia, C. Peña-Garay. 2000-02-18. Four--Neutrino Oscillation Solutions of the Solar Neutrino Problem. https://doi.org/10.1103/physrevd.62.013005

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