On the massless "just-so" solution to the solar neutrino problem

Physics – High Energy Physics – High Energy Physics - Phenomenology

Scientific paper

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4 pages, Latex, uses epsf

Scientific paper

10.1103/PhysRevD.64.097301

We study the effect of the non-resonant, vacuum oscillation-like neutrino flavor conversion induced by non-standard flavor changing and non-universal flavor diagonal neutrino interactions with electrons in the sun. We have found an acceptable fit for the combined analysis for the solar experiments total rates, the Super-Kamiokande (SK) energy spectrum and zenith angle dependence. Phenomenological constraints on non-standard flavor changing and non-universal flavor diagonal neutrino interactions are considered.

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