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Upper limit on the solar antineutrino flux according to LSD data

  • Gravity, Astrophysics
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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).

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Authors and Affiliations

  1. Instituto di Cosmogeofisica del C.N.R., 10133, Turin, Italy

    M. Aglietta, S. Vernetto, C. Vigorito, A. Castellina, L. Perliale, G. C. Trinchero, W. Fulgione, P. Galeotti, C. Castagnoli & O. Saavedra

  2. Instituto di Fisica Generale dell’Universita di Turino, 10133, Turin, Italy

    P. Galeotti, C. Castagnoli & O. Saavedra

  3. Institute of Nuclear Research, Russian Academy of Sciences, 117312, Moscow, Russia

    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

Authors
  1. M. Aglietta
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  2. S. Vernetto
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  3. C. Vigorito
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  4. A. Castellina
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  5. L. Perliale
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  6. G. C. Trinchero
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  7. W. Fulgione
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  8. P. Galeotti
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  9. C. Castagnoli
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  10. O. Saavedra
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  11. V. L. Dadykin
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  12. G. T. Zatsepin
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  13. E. V. Korolkova
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  14. P. V. Kortchaguin
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  15. V. B. Kortchaguin
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  16. V. A. Kudryavtsev
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  17. A. S. Malguin
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  18. O. G. Ryazhskaya
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  19. V. G. Ryasny
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  20. F. F. Khal’chukov
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  21. V. F. Yakushev
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Additional information

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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Aglietta, M., Vernetto, S., Vigorito, C. et al. Upper limit on the solar antineutrino flux according to LSD data. Jetp Lett. 63, 791–795 (1996). https://doi.org/10.1134/1.567091

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  • DOI: https://doi.org/10.1134/1.567091

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