Title

Solar neutrino results from SAGE

Authors

V. N. Gavrin, Institute for Nuclear Research of the Russian Academy of Sciences
V. N. Gavrin, Institute for Nuclear Research of the Russian Academy of Sciences
J. N. Abdurashitovi, Institute for Nuclear Research of the Russian Academy of Sciences
T. J. Bowles, Los Alamos National Laboratory
M. L. Cherry, Louisiana State University
B. T. Cleveland, University of Pennsylvania
R. Davis, University of Pennsylvania
S. R. Elliott, University of Washington
S. V. Girin, Institute for Nuclear Research of the Russian Academy of Sciences
V. V. Gorbachev, Institute for Nuclear Research of the Russian Academy of Sciences
T. V. Ibragimova, Institute for Nuclear Research of the Russian Academy of Sciences
A. V. Kalikhov, Institute for Nuclear Research of the Russian Academy of Sciences
N. G. Khairnasov, Institute for Nuclear Research of the Russian Academy of Sciences
T. V. Knodel, Institute for Nuclear Research of the Russian Academy of Sciences
K. Lande, University of Pennsylvania
I. N. Mirmov, Institute for Nuclear Research of the Russian Academy of Sciences
J. S. Nico, National Institute of Standards and Technology
A. A. Shikhin, Institute for Nuclear Research of the Russian Academy of Sciences
W. A. Teasdale, Los Alamos National Laboratory
E. P. Veretenkin, Institute for Nuclear Research of the Russian Academy of Sciences
V. M. Vermul, Institute for Nuclear Research of the Russian Academy of Sciences
D. L. Wark, Los Alamos National Laboratory
P. S. Wildenhain, University of Pennsylvania
J. F. Wilkerson, University of Washington
V. E. Yants, Institute for Nuclear Research of the Russian Academy of Sciences
G. T. Zatsepin, Institute for Nuclear Research of the Russian Academy of Sciences

Document Type

Article

Publication Date

1-1-2001

Abstract

We report the results of ten years of solar neutrino observation by the Russian-American Gallium solar neutrino Experiment (SAGE). The overall result of 70 runs during the measurement period January 1990 to October 1999 is 75.4 +7.0/-6.8 (stat.) +3.5/-3.0 (syst.) SNU. This represents only slightly more than half of the predicted standard solar model rate of 129 SNU. The individual results of each run, and the results of combined analysis of all runs during each year, as well as the results of combined analysis of all runs during monthly and bimonthly periods are presented.

Publication Source (Journal or Book title)

Nuclear Physics B - Proceedings Supplements

First Page

36

Last Page

43

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