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Upper limit on the solar antineutrino flux according to LSD data |
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| Authors: | M. Aglietta S. Vernetto C. Vigorito A. Castellina L. Perliale G. C. Trinchero W. Fulgione P. Galeotti C. Castagnoli O. Saavedra V. L. Dadykin G. T. Zatsepin E. V. Korolkova P. V. Kortchaguin V. B. Kortchaguin V. A. Kudryavtsev A. S. Malguin O. G. Ryazhskaya V. G. Ryasny F. F. Khal’chukov V. F. Yakushev |
| Affiliation: | (1) Instituto di Cosmogeofisica del C.N.R., 10133 Turin, Italy;(2) Instituto di Fisica Generale dell’Universita di Turino, 10133 Turin, Italy;(3) Institute of Nuclear Research, Russian Academy of Sciences, 117312 Moscow, Russia |
| Abstract: | The experimental data obtained on the liquid scintillation detector LSD are analyzed for the purpose of searching for the solar electron antineutrino flux predicted in the model of spin-flavor precession of the neutrino. The currently most accurate upper limit on the solar v̄e/v e flux ratio is established: Φv̄/Φv⩽1.7% (90% confidence range). Pis’ma Zh. éksp. Teor. Fiz. 63, No. 10, 753–757 (25 May 1996) The spelling of the authors names are presented here in English as requested by the Russian Editorial office. |
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