Maximal $ν_e \to ν_s$ solution to the solar neutrino problem: just-so, MSW or energy independent?

Details Maximal $ν_e \to ν_s$ solution to the solar neutrino problem: just-so, MSW or energy independent? Maximal $ν_e \to ν_s$ solution to the solar neutrino problem: just-so, MSW or energy independent?

1999-05-24

arxiv.org/abs/hep-ph/9905461v2

Phys.Lett. B465 (1999) 203-210

Physics

High Energy Physics

High Energy Physics - Phenomenology

minor changes to text and fig.4

Scientific paper

10.1016/S0370-2693(99)00969-7

We examine the maximal $\nu_e \to \nu_s$ solution to the solar neutrino problem. This solution can be motivated by the exact parity model and other theories. The $\nu_e$ survival probability exhibits one of three qualitatively different behaviours depending on the value of $\Delta m^2$, viz. approximately energy independent, just-so or MSW. By the last of these we mean an enhanced night-time event rate due to regeneration in the Earth. We study all of these possibilities in the context of the recent SuperKamiokande data.

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