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The MSW effect in a fluctuating matter density

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arxiv astro-ph/9604061 v1 pith:YF4SEUIR submitted 1996-04-11 astro-ph hep-phnucl-th

A. B. Balantekin , J. M. Fetter , F. N. Loreti This is my paper
classification astro-phhep-phnucl-th
keywords densityneutrinodistributioneffectfluctuatingfluctuationsmattersolar
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We consider the effect on matter-enhanced neutrino flavor transformation of a randomly fluctuating, delta-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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Cited by 1 Pith paper

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  1. Estimating amplitude of matter density fluctuations in solar and supernova models using neutrino flavor evolution

    astro-ph.HE 2026-07 conditional novelty 5.0 of 10

    SDA recovers density-fluctuation amplitudes from boundary neutrino flavor data in simplified solar and CCSN models, more reliably for the Sun and at high noise in CCSN.

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