FIRST RESULTS FROM THE CR-51 NEUTRINO SOURCE EXPERIMENT WITH THE GALLEX DETECTOR

The radiochemical GALLEX experiment, which has been measuring the solar neutrino flux since May 1991, has performed an investigation with an intense man-made Cr-51 neutrino source (61.9 +/- 1.2 PBq). The source, produced via neutron irradiation of approximate to 36 kg of chromium enriched in Cr-50, primarily emits 746 keV neutrinos. It was placed for a period of 3.5 months in the reentrant tube in the GALLEX tank, to expose the gallium chloride target to a known neutrino Bur. This experiment provides the ratio, R, of the production rate of Cr-produced Ge-71 measured in these source exposures to the rate expected from the known source activity: R = 1.04 +/- 0.12. This result not only constitutes the first observation of low-energy neutrinos from a terrestrial source, but also (a) provides an overall check of GALLEX, indicating that there are no significant experimental artifacts or unknown errors at the 10% level that are comparable to the 40% deficit in observed solar neutrino signal, and (b) directly demonstrates for the first time, using a man-made neutrino source, the validity of the basic principles of radiochemical methods used to detect rare events (at the level of 10 atoms or less). Because of the close similarity in neutrino energy spectra from Cr-51 and from the solar Be-7 branch, this source experiment also shows that the gallium detector is sensitive to Be-7 neutrinos with full efficiency.