Title

Results from SAGE (The Russian-American gallium solar neutrino experiment)

Authors

J. N. Abdurashitov, Institute for Nuclear Research of the Russian Academy of Sciences
E. L. Faizov, Institute for Nuclear Research of the Russian Academy of Sciences
V. N. Gavrin, Institute for Nuclear Research of the Russian Academy of Sciences
A. O. Gusev, Institute for Nuclear Research of the Russian Academy of Sciences
A. V. Kalikhov, Institute for Nuclear Research of the Russian Academy of Sciences
T. V. Knodel, Institute for Nuclear Research of the Russian Academy of Sciences
I. I. Knyshenko, Institute for Nuclear Research of the Russian Academy of Sciences
V. N. Kornoukhov, Institute for Nuclear Research of the Russian Academy of Sciences
I. N. Mirmov, Institute for Nuclear Research of the Russian Academy of Sciences
A. M. Pshukov, Institute for Nuclear Research of the Russian Academy of Sciences
A. M. Shalagin, Institute for Nuclear Research of the Russian Academy of Sciences
A. A. Shikhin, Institute for Nuclear Research of the Russian Academy of Sciences
P. V. Timofeyev, Institute for Nuclear Research of the Russian Academy of Sciences
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
G. T. Zatsepin, Institute for Nuclear Research of the Russian Academy of Sciences
T. J. Bowles, Los Alamos National Laboratory
J. S. Nico, Los Alamos National Laboratory
W. A. Teasdale, Los Alamos National Laboratory
D. L. Wark, Los Alamos National Laboratory
J. F. Wilkerson, Los Alamos National Laboratory
B. T. Cleveland, University of Pennsylvania
T. Daily, University of Pennsylvania
R. Davis, University of Pennsylvania
K. Lande, University of Pennsylvania
C. K. Lee, University of Pennsylvania
P. W. Wildenhain, University of Pennsylvania
S. R. Elliott, Lawrence Livermore National Laboratory
M. L. Cherry, Louisiana State University
R. T. Kouzes, Princeton University

Document Type

Article

Publication Date

5-26-1994

Abstract

Fifteen measurements of the solar neutrino flux have been made in a radiochemical 71Ga-71Ge experiment employing initially 30 t and later 57 t of liquid metallic gallium at the Baksan Neutrino Observatory between January 1990 and May 1992. This provides an integral measurement of the flux of solar neutrinos and in particular is sensitive to the dominant, low-energy p-p solar neutrinos. SAGE observed the capture rate to be 73-16+18 (stat.)-7+5 (syst.) SNU. This represents only 56%-60% of the capture rate predicted by different Standard Solar Models. © 1994.

Publication Source (Journal or Book title)

Physics Letters B

First Page

234

Last Page

248

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