Solar neutrino observations and neutrino oscillations

Details Solar neutrino observations and neutrino oscillations Solar neutrino observations and neutrino oscillations

Jun 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990phrvd..41.3842k&link_type=abstract

Physical Review D (Particles and Fields), Volume 41, Issue 12, 15 June 1990, pp.3842-3845

Physics

3

Scientific paper

The results of recent Kamiokande-II and 37Cl solar-neutrino experiments are quantitatively analyzed assuming the Mikheyev-Smirnov-Wolfenstein solution to the solar-neutrino problem. It is found that the parameter region known as the ``large mass'' solution to the solar-neutrino problem is disfavored by a little more than 1 σ while the ``small mass'' and ``large angle'' solutions are in good agreement at this level. The implications on this analysis from time variations in the data are discussed.

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