Physics – High Energy Physics – High Energy Physics - Phenomenology
Scientific paper
1998-12-07
Phys.Rev.D59:093007,1999
Physics
High Energy Physics
High Energy Physics - Phenomenology
Revtex, 31 pages, uses epsf.sty, 14 postscript figures. Version to be published in Phys. Rev. D
Scientific paper
10.1103/PhysRevD.59.093007
We determine the three-neutrino mixing and mass parameters that are allowed by the solar and atmospheric neutrino data when vacuum oscillations are responsible for both phenomena. The global fit does not appreciably change the allowed regions for the parameters obtained from effective two-neutrino fits. We discuss how measurements of the solar electron energy spectrum below 6.5 GeV in Super-Kamiokande and seasonal variations in the Super-Kamiokande, $^{71}$Ga, and BOREXINO experiments can distinguish the different solar vacuum solutions.
Barger Vernon
Whisnant Kerry
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