Status report on the GALLEX experiment

P. Anselmann,W. Hampel,G. Heusser,J. Kiko,T. Kirsten,E. Pernicka, R. Plaga,U. Rönn,M. Sann,C. Schlosser,R. Wink,M. Wojcik,R. Von Ammon, K. Ebert,T. Fritsch,K. Hellriegel,E. Henrich,L. Stieglitz, F. Weyrich,M. Balata,E. Bellotti,N. Ferrari,H. Lalla,T. Stolarczyk,C. Cattadori,O. Cremonesi,E. Fiorini,S. Pezzoni,L. Zanotti,F. Von Feilitzsch, R. Möβbauer,U. Schanda,G. Berthomieu,E. Schatzman,I. CaRmi,I. Dostrovsky,C. Bacci,P. Belli,R. Bernabei,S. D’Angelo,L. Paoluzi,S. Charbit,M. Cribier, G. Du Pont,L. Gösset,J. Rich,M. Spiro,C. Tao,D. Vignaud,R. L. Hahn,F. X. Hartmann,J. K. Rowley,R. W. Stoenner,J. Weneser, GALLEX Collaboration

Il Nuovo Cimento C（1992）

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摘要

The GALLEX collaboration is performing an experiment for the detection of neutrinos coming principally from the p-p fusion reaction in the Sun, via the reaction ve +71Ga →71Ge + e-. The experiment is running in the Gran Sasso Underground Laboratory of INFN, using as a target 30.3 tons of gallium in the form of 8.13 molar aqueous GaCl3 solution.

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关键词

96.60.Kx,Solar interior (including neutrino problem),12.15,Models of electroweak interactions

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