Results of the whole GALLEX experiment

M Cribier,W Hampel,G Heusser,J Kiko,T Kirsten,M Laubenstein,E Pernicka, W Rau,U Ronn, C Schlosser, M Wojcik, R V Ammon,K H Ebert,T Fritsch, D Heidt,E Henrich,L Stieglitz,F Weirich, M Balata,F Hartmann,M Sann,E Bellotti, C Cattadori,O Cremonesi, N Ferrari, E Fiorini, L Zanotti,M Altmann,F V Feilitzsch, R Moβbauer, S Waenninger, G Berthomieu,Evry Schatzman,I Carmi,I Dostrovsky, C Bacci,P Belli,R Bernabei,S Dangelo, L Paoluzi,A Bevilacqua, L Gosset,J Rich,M Spiro,C Tao,D Vignaud, J Boger,R L Hahn,J K Rowley,R W Stoenner,J Weneser

Nuclear Physics B - Proceedings Supplements（1999）

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摘要

After 5.5 years of data taking, GALLEX ended its experimental phase. The solar neutrino production rate, 76.4 ± 8 SNU, represents about 55% of the predicted rate. The As tests prove, at the 1% level, the reliability of the technique and the detection of 51Cr neutrino, with the nominal efficiency (93.0±8%), control the response of the detector to neutrinos in the solar energy range.

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关键词

solar neutrinos,data processing,solar energy,radiation detector

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