Authors

A. I. Abazov, Institute for Nuclear Research of the Russian Academy of Sciences
D. N. Abdurashitov, Institute for Nuclear Research of the Russian Academy of Sciences
O. L. Anosov, Institute for Nuclear Research of the Russian Academy of Sciences
L. A. Eroshkina, 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. 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
S. A. Mezentseva, Institute for Nuclear Research of the Russian Academy of Sciences
I. N. Mirmov, Institute for Nuclear Research of the Russian Academy of Sciences
A. I. Ostrinsky, Institute for Nuclear Research of the Russian Academy of Sciences
V. V. Petukhov, Institute for Nuclear Research of the Russian Academy of Sciences
A. M. Pshukov, Institute for Nuclear Research of the Russian Academy of Sciences
N. Ye Revzin, 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
Yu Zakharov, Institute for Nuclear Research of the Russian Academy of Sciences
G. T. Zatsepin, Institute for Nuclear Research of the Russian Academy of Sciences
V. I. Zhandarov, Institute for Nuclear Research of the Russian Academy of Sciences
T. J. Bowles, Los Alamos National Laboratory
B. T. Cleveland, Los Alamos National Laboratory
S. R. Elliott, Los Alamos National Laboratory
H. A. O'Brien, Los Alamos National Laboratory
D. L. Wark, Los Alamos National Laboratory
J. F. Wilkerson, Los Alamos National Laboratory
R. Davis, University of Pennsylvania
K. Lande, University of Pennsylvania
M. L. Cherry, Louisiana State University
R. T. Kouzes, Princeton University

Document Type

Article

Publication Date

1-1-1991

Abstract

The Soviet-American Gallium Experiment is the first experiment able to measure the dominant flux of low energy p-p solar neutrinos. Four extractions made during January to May 1990 from 30 tons of gallium have been counted and indicate that the flux is consistent with 0 SNU and is less than 72 SNU (68% CL) and less than 138 SNU (95% CL). This is to be compared with the flux of 132 SNU predicted by the Standard Solar Model. © 1991.

Publication Source (Journal or Book title)

Nuclear Physics B (Proceedings Supplements)

First Page

84

Last Page

93

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