Matter Effects in Active-Sterile Solar Neutrino Oscillations

Details Matter Effects in Active-Sterile Solar Neutrino Oscillations Matter Effects in Active-Sterile Solar Neutrino Oscillations

2009-10-30

arxiv.org/abs/0910.5856v2

Phys.Rev.D80:113007,2009

Physics

High Energy Physics

High Energy Physics - Phenomenology

26 pages. Final version published in Phys. Rev. D80 (2009) 113007

Scientific paper

10.1103/PhysRevD.80.113007

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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