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AbstractAbstract
[en] The GALLEX experiment, installed in the Gran Sasso Underground Laboratory, has measured the rate of production of 71Ge from 71Ga by solar neutrinos, using 30.3 tons of gallium in the form of gallium chloride solution. 14 measurements carried out in one year of operation give, after corrections for side reactions and other backgrounds, an average value of (83±19(stat.)±8(syst.)) SNU (1σ) due to solar neutrinos. This result, two standard deviations below the predictions of solar model calculations (122--132 SNU), constitutes the first observation of solar pp-neutrinos. The possible deficit is interpreted, together with those of the chlorine and Kamiokande experiments, in terms either of astrophysics or of neutrino oscillations (MSW effect)
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ICHEP-26: 26. International Union of Pure and Applied Physics (IUPAP) conference on high energy physics; Dallas, TX (United States); 6-12 Aug 1992; CONF-920837--
Record Type
Journal Article
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Conference
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BARYON-BARYON INTERACTIONS, BETA DECAY RADIOISOTOPES, DAYS LIVING RADIOISOTOPES, ELECTRON CAPTURE RADIOISOTOPES, ELEMENTARY PARTICLES, EVEN-ODD NUCLEI, FERMIONS, FIELD THEORIES, GALLIUM ISOTOPES, GERMANIUM ISOTOPES, GRAND UNIFIED THEORY, HADRON-HADRON INTERACTIONS, INTERACTIONS, INTERMEDIATE MASS NUCLEI, ISOTOPES, LEPTON-BARYON INTERACTIONS, LEPTON-HADRON INTERACTIONS, LEPTON-NUCLEON INTERACTIONS, LEPTONS, MASSLESS PARTICLES, MATHEMATICAL MODELS, NEUTRINOS, NUCLEI, NUCLEON-NUCLEON INTERACTIONS, ODD-EVEN NUCLEI, PARTICLE INTERACTIONS, PARTICLE MODELS, PROTON-NUCLEON INTERACTIONS, QUANTUM FIELD THEORY, RADIATIONS, RADIOISOTOPES, SOLAR PARTICLES, SOLAR RADIATION, SPECTRA, STABLE ISOTOPES, STELLAR RADIATION, UNIFIED GAUGE MODELS
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