Standard Solar Model and Electron-Neutrino Oscillations

Details Standard Solar Model and Electron-Neutrino Oscillations Standard Solar Model and Electron-Neutrino Oscillations

Aug 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001icrc....3.1193s&link_type=abstract

Proceedings of the 27th International Cosmic Ray Conference. 07-15 August, 2001. Hamburg, Germany. Under the auspices of the Int

Physics

Scientific paper

The deficiency in the experimental measurements [1-5] as compared to the theoretical predictions about the solar neutrino flux made by using the standard solar model [6-8] is called the solar neutrino problem. Attempts to explain all these results by using high or low flux parameters based on standard solar models have not been successful. Wolfenstein suggested [9] that the problem could be solved in principle by assuming that at least one of the neutrinos was massive and oscillations occurred between neutrinos of almost degenerate masses. The results were explained by taking neutrinos as massive and making use of MSW mechanism based on neutrino oscillations. However, all the terrestrial experiments [10], except the LSD experiment [11] whose results have not yet transcended the limits of statistical errors, performed to detect the flavour transformation of neutrinos due to their oscillations do not give any evidence for oscillations.

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