Direct approach to resolve the solar-neutrino problem

Details Direct approach to resolve the solar-neutrino problem Direct approach to resolve the solar-neutrino problem

Sep 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985phrvl..55.1534c&link_type=abstract

Physical Review Letters (ISSN 0031-9007), vol. 55, Sept. 30, 1985, p. 1534-1536. DOE-NSF-supported research.

Physics

82

Flux Quantization, Neutrino Beams, Solar Neutrinos, Boron Isotopes, Cerenkov Counters, Heavy Water, Solar Physics

Scientific paper

A direct approach to resolve the solar-neutrino problem would be to observe neutrinos by use of both neutral-current and charged-current reactions. Then, the total neutrino flux and the electron-neutrino flux would be separately determined to provide independent tests of the neutrino-oscillation hypothesis and the standard solar model. A large heavy-water Cherenkov detector, sensitive to neutrinos from 8B decay via the neutral-current reaction ν+d→ν+p+n and the charged-current reaction νe+d→e-+p+p, is suggested for this purpose.

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