Effects of magnetohydrodynamics matter density fluctuations on the solar neutrino resonant spin-flavor precession

Reggiani, N.; Guzzo, M. M.; Colonia, J.H.; Holanda, P. C. de

doi:10.1590/s0103-97332000000300018

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2002

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Cited by 3 publications

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“…Even though this limit is not appropriate to the solar fluctuations it may be applicable to a number of other astrophysical situations where neutrinos play a role. Similar conclusions were reached by other authors [16,17,18,19,20,21,22,23,24,25,26,27,28,29]. Recent reviews were given in Refs.…”

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confidence: 82%

Neutrinos in stochastic media: From sun to core-collapse supernovae

Balantekin

2002

AIP Conference Proceedings

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Recent work on neutrino propagation in stochastic media and its implications for the Sun and corecollapse supernovae are reviewed. It is shown that recent results from Sudbury Neutrino Observatory and SuperKamiokande combined with a best global fit value of δm 2 = 5 × 10 −5 eV 2 and tan 2 θ = 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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