A Unique Oscillation Solution to the Solar Neutrino Problem?

Preprint

8 February 2002

preprint
Published by arXiv in arXiv

https://doi.org/10.48550/arXiv.hep-ex/0202020

Abstract

A global two-neutrino oscillation fit combining Super-Kamiokande solar neutrino data with the solar neutrino rates measured by Homestake, Gallex/GNO, SAGE and SNO prefers a single allowed area, the Large Mixing Angle solution, at about 95% confidence level. The mass^2 difference between the two mass eigenstates is Delta m^2 approx 3-25 x 10^-5 eV^2, the mixing angle theta is tan^2 theta approx 0.21-0.67.

Keywords

OSCILLATION SOLUTION
UNIQUE OSCILLATION
NEUTRINO PROBLEM
SOLAR NEUTRINO
MIXING ANGLE
TWO NEUTRINO
GLOBAL TWO

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Version 1, 2002-02-08, ArXiv

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