Seismic constraints on neutrino oscillation parameters

Details Seismic constraints on neutrino oscillation parameters Seismic constraints on neutrino oscillation parameters

Jan 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001esasp.464..519g&link_type=abstract

In: Proceedings of the SOHO 10/GONG 2000 Workshop: Helio- and asteroseismology at the dawn of the millennium, 2-6 October 2000,

Computer Science

Sun: Oscillations, Solar Neutrinos, Sun: Interior

Scientific paper

The neutrino fluxes calculated using a seismically inferred solar model are compared with measured fluxes from the three solar neutrino experiments. Treating the neutrino fluxes from seismic model as theoretical predictions, the latest solar neutrino data is analyzed assuming vacuum oscillation of neutrinos. The best-fit values of the neutrino mixing angle and mass squared difference are found and the allowed regions are determined.

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