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We consider the effect on matter-enhanced neutrino flavor transformation of a randomly fluctuating, δ-correlated matter density. The fluctuations will produce a distribution of neutrino survival probabilities. We find the mean and variance of the distribution for the case of solar neutrinos, and discuss the possibility of placing a limit on solar density fluctuations using neutrino data.
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Balantekin et al. (1996) studied this question.
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