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The GALLEX Project

Published online by Cambridge University Press:  12 April 2016

T. Kirsten ,
M. Breitenbach ,
W. Hampel ,
G. Heusser ,
J. Kiko ,
T. Kirsten ,
H. Lalla ,
A. Lenzing ,
E. Pernicka  and
R. Plaga
...Show all authors
T. Kirsten
Affiliation:
Max-Planck-Institut für Kernphysik,P.O.Box 103980, 6900 Heidelberg
M. Breitenbach
Affiliation:
Max-Planck-Institut für Kernphysik, Heidelberg
W. Hampel
Affiliation:
Max-Planck-Institut für Kernphysik, Heidelberg
G. Heusser
Affiliation:
Max-Planck-Institut für Kernphysik, Heidelberg
J. Kiko
Affiliation:
Max-Planck-Institut für Kernphysik, Heidelberg
T. Kirsten
Affiliation:
Max-Planck-Institut für Kernphysik, Heidelberg
H. Lalla
Affiliation:
Max-Planck-Institut für Kernphysik, Heidelberg
A. Lenzing
Affiliation:
Max-Planck-Institut für Kernphysik, Heidelberg
E. Pernicka
Affiliation:
Max-Planck-Institut für Kernphysik, Heidelberg
R. Plaga
Affiliation:
Max-Planck-Institut für Kernphysik, Heidelberg
B. Povh
Affiliation:
Max-Planck-Institut für Kernphysik, Heidelberg
C. Schlosser
Affiliation:
Max-Planck-Institut für Kernphysik, Heidelberg
H. Völk
Affiliation:
Max-Planck-Institut für Kernphysik, Heidelberg
R. Wink
Affiliation:
Max-Planck-Institut für Kernphysik, Heidelberg
K. Zuber
Affiliation:
Max-Planck-Institut für Kernphysik, Heidelberg
R.v. Ammon
Affiliation:
Kernforschungszentrum Karlsruhe-KFK
K. Ebert
Affiliation:
Kernforschungszentrum Karlsruhe-KFK
E. Henrich
Affiliation:
Kernforschungszentrum Karlsruhe-KFK
L. Stieglitz
Affiliation:
Kernforschungszentrum Karlsruhe-KFK
E. Bellotti
Affiliation:
Dip.di Fisica dell’Università, Milano and Laboratori Nazionali del Gran Sasso-INFN
O. Cremonesi
Affiliation:
Dip.di Fisica dell’Università, Milano
E. Fiorini
Affiliation:
Dip.di Fisica dell’Università, Milano
C. Liguori
Affiliation:
Dip.di Fisica dell’Università, Milano
S. Ragazzi
Affiliation:
Dip.di Fisica dell’Università, Milano
L. Zanotti
Affiliation:
Dip.di Fisica dell’Università, Milano
R. Mössbauer
Affiliation:
Physik Dept. E15, Technische Universität München
A. Urban
Affiliation:
Physik Dept. E15, Technische Universität München
G. Berthomieu
Affiliation:
Université de Nice-Observatoire
E. Schatzman
Affiliation:
Université de Nice-Observatoire
S. d’Angelo
Affiliation:
II-Universita di Roma-INFN
C. Bacci
Affiliation:
II-Universita di Roma-INFN
P. Belli
Affiliation:
II-Universita di Roma-INFN
R. Bernabei
Affiliation:
II-Universita di Roma-INFN
L. Paoluzi
Affiliation:
II-Universita di Roma-INFN
R. Santonico
Affiliation:
II-Universita di Roma-INFN
M. Cribier
Affiliation:
Centre d’Etudes Nucléaires de Saclay, Gif-sur Yvette
G. Dupont
Affiliation:
Centre d’Etudes Nucléaires de Saclay, Gif-sur Yvette
B. Pichard
Affiliation:
Centre d’Etudes Nucléaires de Saclay, Gif-sur Yvette
J. Rich
Affiliation:
Centre d’Etudes Nucléaires de Saclay, Gif-sur Yvette
M. Spiro
Affiliation:
Centre d’Etudes Nucléaires de Saclay, Gif-sur Yvette
T. Stolarczyk
Affiliation:
Centre d’Etudes Nucléaires de Saclay, Gif-sur Yvette
C. Tao
Affiliation:
Centre d’Etudes Nucléaires de Saclay, Gif-sur Yvette
D. Vignaud
Affiliation:
Centre d’Etudes Nucléaires de Saclay, Gif-sur Yvette
I. Dostrovsky
Affiliation:
Weizmann Institute of Sciences, Rehovot
G. Friedlander
Affiliation:
Brookhaven National Laboratory, Upton, N.Y.
R.L. Hahn
Affiliation:
Brookhaven National Laboratory, Upton, N.Y.
J.K. Rowley
Affiliation:
Brookhaven National Laboratory, Upton, N.Y.
R.W. Stoenner
Affiliation:
Brookhaven National Laboratory, Upton, N.Y.
J. Weneser
Affiliation:
Brookhaven National Laboratory, Upton, N.Y.

Abstract

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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.

Type
Part 2: Neutrinos
Information
International Astronomical Union Colloquium , Volume 121: Inside the Sun , 1990 , pp. 187 - 199
Copyright
Copyright © Kluwer 1990

References

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