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Solar neutrino results and present status
Authors:V V Gorbachev  J N Abdurashitov  T J Bowles  M L Cherry  B T Cleveland  R Davis Jr  S R Elliott  V N Gavrin  S V Girin  P P Gurkina  T V Ibragimova  A V Kalikhov  N G Khairnasov  T V Knodel  K Lande  I N Mirmov  J S Nico  A A Shikhin  W A Teasdale  E P Veretenkin  V M Vermul  D L Wark  P S Wildenhain  J F Wilkerson  V E Yants  G T Zatsepin
Institution:(1) Los Alamos National Laboratory, Los Alamos, NM, USA;(2) Louisiana State University, Baton Rouge, LA 70803, USA;(3) University of Washington, Seattle, WA 98195, USA;(4) University of Pennsylvania, Philadelphia, PA 19104, USA;(5) National Institute of Standards and Technology, Gaithersburg, MD, USA;(6) Department of Particle and Nuclear Physics, Oxford University, Oxford, UK;(7) Institute for Nuclear Research, Russian Academy of Sciences, pr. Shestidesyatiletiya Oktyabrya 7a, Moscow, 117312, Russia
Abstract:The solar neutrino capture rate measured by the Russian-American Gallium Experiment on a metallic gallium target SAGE during the time from January 1990 through December 2000 is 77.0 ?6.2 ?3.0 +6.2 +3.5 SNU, where the uncertainties are statistical and systematic, respectively. The experimental procedures and data analysis are presented.
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