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Solar-neutrino results from SAGE
Authors:J N Abdurashitov  V N Gavrin  S V Girin  V V Gorbachev  T V Ibragimova  A V Kalikhov  N G Khairnasov  T V Knodel  I N Mirmov  A A Shikhin  E P Veretenkin  V M Vermul  V E Yants  G T Zatsepin  T J Bowles  W A Teasdale  D L Wark  J S Nico  M L Cherry  B T Cleveland  R Davis Jr  K Lande  P S Wildenhain  S R Elliott  J F Wilkerson
Institution:(1) Institute for Nuclear Research, Russian Academy of Sciences, pr. Shestidesyatiletiya Oktyabrya 7a, Moscow, 117312, Russia;(2) Los Alamos National Laboratory, Los Alamos, NM 87545, USA;(3) Department of Particle and Nuclear Physics, Oxford University, Keble Road, Oxford, OX1 3RH, UK;(4) National Institute of Standards and Technology, Gaithersburg, MD 20899, USA;(5) Louisiana State University, Baton Rouge, LA 70803, USA;(6) University of Pennsylvania, Philadelphia, PA 19104, USA;(7) University of Washington, Seattle, WA 98195, USA
Abstract:The solar-neutrino-capture rate measured by the Russian-American Gallium Experiment on metallic gallium during the period from January 1990 to December 1997 is (67.2 ?7.0?3.0 +7.2+3.5 ) SNU, where the uncertainties are statistical and systematic, respectively. This result represents a 7σ depression in the neutrino flux in relation to the predicted standard-solar-model rates. The experimental procedures used and data analysis are presented.
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