Neutrinos in Stochastic Media: From Sun to Core-Collapse Supernovae

Details Neutrinos in Stochastic Media: From Sun to Core-Collapse Supernovae Neutrinos in Stochastic Media: From Sun to Core-Collapse Supernovae

2001-09-18

arxiv.org/abs/hep-ph/0109163v1

AIPConf.Proc.610:969-972,2002

Physics

High Energy Physics

High Energy Physics - Phenomenology

4 pages, to be published in the proceedings of the International Nuclear Physics Conference (INPC 2001): Nuclear Physics And T

Scientific paper

10.1063/1.1470265

Recent work on neutrino propagation in stochastic media and its implications for the Sun and core-collapse supernovae are reviewed. It is shown that recent results from Sudbury Neutrino Observatory and SuperKamiokande combined with a best global fit value of $\delta m^2= 5\times 10^{-5}$ eV$^2$ and $\tan^2 \theta = 0.3$ rule out solar electron density fluctuations of a few percent or more. It is argued that solar neutrino experiments may be able to rule out even smaller fluctuations in the near future.

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