G
G. T. Zatsepin
Researcher at Russian Academy of Sciences
Publications - 134
Citations - 3941
G. T. Zatsepin is an academic researcher from Russian Academy of Sciences. The author has contributed to research in topics: Neutrino & Solar neutrino. The author has an hindex of 25, co-authored 134 publications receiving 3669 citations. Previous affiliations of G. T. Zatsepin include Lebedev Physical Institute & Moscow State University.
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Journal ArticleDOI
Measurement of the solar neutrino capture rate with gallium metal. III: Results for the 2002--2007 data-taking period
J. N. Abdurashitov,V. N. Gavrin,V. V. Gorbachev,P. P. Gurkina,T. V. Ibragimova,A. V. Kalikhov,N. G. Khairnasov,T. V. Knodel,I. N. Mirmov,A. A. Shikhin,E. P. Veretenkin,V. E. Yants,G. T. Zatsepin,T. J. Bowles,S. R. Elliott,W. A. Teasdale,Jeffrey S. Nico,B. T. Cleveland,J. F. Wilkerson +18 more
TL;DR: In this paper, the authors presented the experimental improvements in SAGE since its last published data summary in December 2001, and combined analysis of 168 extractions through December 2007 gives a capture rate of solar neutrinos with energy more than 233 keV of $65.1$ SNU, where statistical and systematic uncertainties have been combined in quadrature.
Journal ArticleDOI
Cosmic rays at ultra high energies (neutrino
V.S. Beresinsky,G. T. Zatsepin +1 more
TL;DR: The neutrino spectrum produced by protons on microwave photons was calculated in this article, and it was shown that a spectrum of extensive air shower primaries can have no cut-off at an energy E > 3 × 1019 eV, if the neutrinos-nucleon total cross-section rises up to the geometrical one of a nucleon.
Journal ArticleDOI
Solar neutrino flux measurements by the Soviet-American gallium experiment (SAGE) for half the 22-year solar cycle
J. N. Abdurashitov,E. P. Veretenkin,V. M. Vermul,V. N. Gavrin,S. V. Girin,V. V. Gorbachev,P. P. Gurkina,G. T. Zatsepin,T. V. Ibragimova,A. V. Kalikhov,T. V. Knodel,I. N. Mirmov,N. G. Khairnasov,A. A. Shikhin,V. E. Yants,T. J. Bowles,W. A. Teasdale,Jeffrey S. Nico,J. F. Wilkerson,B. T. Cleveland,Steven Elliott +20 more
TL;DR: In this article, the authors present measurements of the solar neutrino capture rate on metallic gallium in the Soviet-American gallium experiment (SAGE) over a period of slightly more than half the 22-year solar cycle.
Journal ArticleDOI
Measurement of the response of a Ga solar neutrino experiment to neutrinos from a Ar37 source
J. N. Abdurashitov,V. N. Gavrin,S. V. Girin,V. V. Gorbachev,P. P. Gurkina,T. V. Ibragimova,A. V. Kalikhov,N. G. Khairnasov,T. V. Knodel,Viktor Matveev,I. N. Mirmov,A. A. Shikhin,E. P. Veretenkin,V. M. Vermul,V. E. Yants,G. T. Zatsepin,T. J. Bowles,S. R. Elliott,W. A. Teasdale,B. T. Cleveland,Wick Haxton,J. F. Wilkerson,Jeffrey S. Nico,A. Suzuki,K. Lande,Yu. S. Khomyakov,V. M. Poplavsky,V. V. Popov,O. V. Mishin,A. N. Petrov,B. A. Vasiliev,S. A. Voronov,A. I. Karpenko,V. V. Maltsev,N. N. Oshkanov,A. M. Tuchkov,V. I. Barsanov,A. A. Janelidze,A. V. Korenkova,N. A. Kotelnikov,S. Yu. Markov,V. V. Selin,Z. N. Shakirov,A. A. Zamyatina,S. B. Zlokazov +44 more
TL;DR: An intense source of gallium was produced by the $(n,\ensuremath{\alpha})$ reaction on $40}$ by irradiating 330 kg of calcium oxide in the fast neutron breeder reactor at Zarechny, Russia as discussed by the authors.
Journal ArticleDOI
On the Event Observed in the Mont Blanc Underground Neutrino Observatory during the Occurrence of Supernova 1987a
Marco Aglietta,Giovanni Badino,G. Bologna,C. Castagnoli,Antonella Castellina,V. L. Dadykin,W. Fulgione,P. Galeotti,F. F. Kalchukov,B. V. Kortchaguin,P. V. Kortchaguin,A. S. Malguin,V. G. Ryassny,O. G. Ryazhskaya,O. Saavedra,V. P. Talochkin,G. C. Trinchero,S. Vernetto,G. T. Zatsepin,V. F. Yakushev +19 more
TL;DR: In this article, the characteristics of the event detected in the Mont Blanc Underground Neutrino Observatory on February 23, 1987, consisting of 5 interactions recorded during 7s are discussed, and it is shown that the event can be explained in terms of detection of neutrinos emitted during the stellar collapse in the Large Magellanic Cloud.