Document Type
Article
Publication Date
1-1-1996
Abstract
The solar neutrino capture rate measured by SAGE is well below that predicted by solar models. To check the overall experimental efficiency, we exposed 13 tonnes of Ga metal to a reactor-produced 517 kCi source of 51Cr. The ratio of the measured production rate to that predicted from the source activity is 0.95+/-0.11\(stat\)+0.05/-0.08\(syst\). This agreement verifies that the experimental efficiency is measured correctly, establishes that there are no unknown systematic errors at the 10% level, and provides considerable evidence for the reliability of the solar neutrino measurement. © 1996 The American Physical Society.
Publication Source (Journal or Book title)
Physical Review Letters
First Page
4708
Last Page
4711
Recommended Citation
Abdurashitov, J., Gavrin, V., Girin, S., Gorbachev, V., Ibragimova, T., Kalikhov, A., Khairnasov, N., Knodel, T., Kornoukhov, V., Mirmov, I., Shikhin, A., Veretenkin, E., Vermul, V., Yants, V., Zatsepin, G., Bowles, T., Nico, J., Teasdale, W., Wark, D., Cherry, M., Karaulov, V., Levitin, V., Maev, V., Nazarenko, P., Shkol-Nik, V., Skorikov, N., Cleveland, B., Daily, T., Davis, R., Lande, K., Lee, C., Wildenhain, P., & Khomyakov, Y. (1996). The russian-american gallium experiment (sage) cr neutrino source measurement. Physical Review Letters, 77 (23), 4708-4711. https://doi.org/10.1103/PhysRevLett.77.4708