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Matter Effects in Active-Sterile Solar Neutrino Oscillations

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arxiv 0910.5856 v2 pith:MGYI3VSX submitted 2009-10-30 hep-ph

classification hep-ph
keywords neutrinomixingoscillationssolareffectsmattersquared-massactive-sterile
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The matter effects for solar neutrino oscillations are studied in a general scheme with an arbitrary number of sterile neutrinos, without any constraint on the mixing, assuming only a realistic hierarchy of neutrino squared-mass differences in which the smallest squared-mass difference is effective in solar neutrino oscillations. The validity of the analytic results are illustrated with a numerical solution of the evolution equation in three examples of the possible mixing matrix in the simplest case of four-neutrino mixing.

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Cited by 1 Pith paper

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  1. Effective Matter Flavor Conversion Mediated by Pseudo-Sterile States as the Possible Origin of Neutrino Oscillation Anomalies

    hep-ph 2026-05 conditional novelty 6.0 of 10

    A sterile neutrino with a novel density-dependent matter potential Vs resolves multiple oscillation anomalies when Vs is negative and mixing angles are small.

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