Physics – High Energy Physics – High Energy Physics - Phenomenology
Scientific paper
2000-02-17
Phys.Rev.D62:031301,2000
Physics
High Energy Physics
High Energy Physics - Phenomenology
5 pages,latex file using RevTex. Two-layer aproximation for the Earth density replaced by numerical integration with PREM. Lat
Scientific paper
10.1103/PhysRevD.62.031301
We present an analysis of the MSW neutrino oscillation solutions of the solar neutrino problem in the framework of two-neutrino mixing in the enlarged parameter space $(\Delta m^2, \tan^2\theta)$ with $\theta \in (0,\frac{\pi}{2})$. Recently, it was pointed out that the allowed region of parameters from a fit to the measured total rates can extend to values $\theta \geq \frac{\pi}{4}$ (the so called ``dark side'') when higher confidence levels are allowed. The purpose of this letter is to reanalize the problem including all the solar neutrino data available, to discuss the dependence on the statistical criteria in the determination of the CL of the ``dark side'' and to extract the corresponding limits on the largest mixing allowed by the data. Our results show that when the Super-Kamiokande data on the zenith angle distribution of events and the spectrum information is included, the regions extend more into the dark side.
Gonzalez-Garcia M. C.
Pena-Garay Carlos
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