Describing analytically the MSW effect for solar neutrinos in the presence of solar density perturbations

Details Describing analytically the MSW effect for solar neutrinos in the presence of solar density perturbations Describing analytically the MSW effect for solar neutrinos in the presence of solar density perturbations

Apr 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992phlb..279..153a&link_type=abstract

Physics Letters B, Volume 279, Issue 1-2, p. 153-160.

Physics

8

Scientific paper

We derive a simple analytic expression for the average probability of two-neutrino matter-enhanced transitions of solar neutrinos in the sun in the case of existence of a thin layer in the interior of the sun in which the density changes much faster (but continuously) than is predicted by the standard solar model.
Permanent address: Institute of Nuclear Research and Nuclear Energy, Bulgarian Academy of Sciences, 1784 Sofia, Bulgaria.

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