The GALLEX Project

The GALLEX Project

T. Kirsten,M. Breitenbach,W. Hampel,G. Heusser,J. Kiko,H. Lalla,A. Lenzing,E. Pernicka,R. Plaga,B. Povh,C. Schlosser,H. Völk,R. Wink,K. Zuber,R.V. Ammon,K. Ebert,E. Henrich,L. Stieglitz,E. Bellotti,O. Cremonesi,E. Fiorini,C. Liguori,S. Ragazzi,L. Zanotti,R. Mössbauer,A. Urban,G. Berthomieu,E. Schatzman,S. D’Angelo,C. Bacci,P. Belli,R. Bernabei,L. Paoluzi,R. Santonico,M. Cribier,G. Dupont,B. Pichard,J. Rich,M. Spiro,T. Stolarczyk,C. Tao,D. Vignaud,I. Dostrovsky,G. Friedlander,R.L. Hahn,J.K. Rowley,R.W. Stoenner,J. Weneser;T. Kirsten;M. Breitenbach;W. Hampel;G. Heusser;J. Kiko;H. Lalla;A. Lenzing;E. Pernicka;R. Plaga;B. Povh;C. Schlosser;H. Völk;R. Wink;K. Zuber;R.V. Ammon;K. Ebert;E. Henrich;L. Stieglitz;E. Bellotti;O. Cremonesi;E. Fiorini;C. Liguori;S. Ragazzi;L. Zanotti;R. Mössbauer;A. Urban;G. Berthomieu;E. Schatzman;S. D’Angelo;C. Bacci;P. Belli;R. Bernabei;L. Paoluzi;R. Santonico;M. Cribier;G. Dupont;B. Pichard;J. Rich;M. Spiro;T. Stolarczyk;C. Tao;D. Vignaud;I. Dostrovsky;G. Friedlander;R.L. Hahn;J.K. Rowley;R.W. Stoenner;J. Weneser;
International Astronomical Union Colloquium 1990 Vol. 121 pp. 187-199
151
weneser1990internationalthe

Abstract

The GALLEX collaboration aims at the detection of solar neutrinos in a radiochemical experiment employing 30 tons of Gallium in form of concentrated aqueous Gallium-chloride solution. The detector is primarily sensitive to the otherwise inaccessible pp-neutrinos. Details of the experiment have been repeatedly described before [1-7]. Here we report the present status of implementation in the Laboratori Nazionali del Gran Sasso (Italy). So far, 12.2 tons of Gallium are at hand. The present status of development allows to start the first full scale run at the time when 30 tons of Gallium become available. This date is expected to be January, 1990.

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