Constraints on neutrino-oscillation parameters from the Kamiokande-II solar-neutrino data

Details Constraints on neutrino-oscillation parameters from the Kamiokande-II solar-neutrino data Constraints on neutrino-oscillation parameters from the Kamiokande-II solar-neutrino data

Sep 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990phrvl..65.1301h&link_type=abstract

Physical Review Letters (ISSN 0031-9007), vol. 65, Sept. 10, 1990, p. 1301-1304. Research supported by MOESC, DOE, and Universit

Physics

119

Adiabatic Conditions, Electron Energy, Energy Spectra, Solar Neutrinos, Error Analysis, Signal Detectors, Solar Oscillations

Scientific paper

The solar neutrino data from the Kamiokande II detector have been
analyzed for compatibility with the different solutions in the
Mikheyev-Smirnov-Wolfenstein formalism. The measured recoil-electron
energy spectrum alone disfavors the region of the adiabatic solution at
the 90 percent confidence level.

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