The MSW solution to the solar neutrino problem in the presence of random solar matter density perturbations

Details The MSW solution to the solar neutrino problem in the presence of random solar matter density perturbations The MSW solution to the solar neutrino problem in the presence of random solar matter density perturbations

1996-02-23

arxiv.org/abs/hep-ph/9602384v1

Nucl.Phys.Proc.Suppl. 48 (1996) 384-390

Physics

High Energy Physics

High Energy Physics - Phenomenology

Talk presented at TAUP95, Toledo, Sept. 1995, Latex file, 4 pages, including 3 figures

Scientific paper

10.1016/0920-5632(96)00277-0

We present the evolution equation describing MSW conversion, derived in the framework of the Schr\"odinger approach, in the presence of matter density fluctuations. Then we analyse the effect of such fluctuations in the MSW scenario as a solution to the solar neutrino problem. It is shown that the non-adiabatic MSW parameter region is rather stable (especially in $\delta m^2$) for matter density noise at the few percent level. We also discuss the possibility to probe solar matter density fluctuations at the future Borexino experiment.

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