Long-wavelength vacuum neutrino oscillations and the solar-neutrino deficit

Details Long-wavelength vacuum neutrino oscillations and the solar-neutrino deficit Long-wavelength vacuum neutrino oscillations and the solar-neutrino deficit

Dec 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990phrvl..65.3084b&link_type=abstract

Physical Review Letters (ISSN 0031-9007), vol. 65, Dec. 17, 1990, p. 3084-3087.

Physics

37

Long Wave Radiation, Oscillations, Particle Energy, Solar Neutrinos, Annual Variations, Earth Orbits, Relativistic Theory

Scientific paper

Vacuum neutrino oscillations with very long wavelength, comparable to the radius of the earth's orbit, can simultaneously explain both the Homestake and Kamiokande-II solar-neutrino counting rates. They imply approximately a 50 percent reduction of the nu(e) flux from the p-p process, and seasonal variations in the nu-e scattering rates for Be-7 and pep neutrinos, which distinguish this scenario from alternative explanations.

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