Title

Measurement of the solar neutrino capture rate by SAGE and implications for neutrino oscillations in vacuum

Authors

J. N. Abdurashitov, 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
V. N. Gavrin, Institute for Nuclear Research of the Russian Academy of Sciences
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, 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
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. Zatsep, Institute for Nuclear Research of the Russian Academy of Sciences

Document Type

Article

Publication Date

1-1-1999

Abstract

The Russian-American solar neutrino experiment has measured the capture rate of neutrinos on metallic gallium in a radiochemical experiment at the Baksan Neutrino Observatory. Eight years of measurement give the result 67.2-7.0-3.0+7.2+3.5solar neutrino units, where the uncertainties are statistical and systematic, respectively. The restrictions these results impose on vacuum neutrino oscillation parameters are given. © 1999 The American Physical Society.

Publication Source (Journal or Book title)

Physical Review Letters

First Page

4686

Last Page

4689

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