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.

Hampel, W., Heusser, G., Kiko, J., Kirsten, T., Laubenstein, M., Pernicka, E., et al. (1999). Results of the whole GALLEX experiment. NUCLEAR PHYSICS B-PROCEEDINGS SUPPLEMENTS, 70(1-3), 284-291 [10.1016/S0920-5632(98)00438-1].

Results of the whole GALLEX experiment

BERNABEI, RITA;D'ANGELO, SILIO;PAOLUZI, LUCIANO;
1999-01-01

Abstract

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.
1999
Pubblicato
Rilevanza internazionale
Articolo
Sì, ma tipo non specificato
Settore FIS/04 - FISICA NUCLEARE E SUBNUCLEARE
Settore FIS/01 - FISICA SPERIMENTALE
English
Con Impact Factor ISI
Solar Neutrinos, Detectors, GALLEX
http://www.sciencedirect.com/science/article/pii/S0920563298004381
Hampel, W., Heusser, G., Kiko, J., Kirsten, T., Laubenstein, M., Pernicka, E., et al. (1999). Results of the whole GALLEX experiment. NUCLEAR PHYSICS B-PROCEEDINGS SUPPLEMENTS, 70(1-3), 284-291 [10.1016/S0920-5632(98)00438-1].
Hampel, W; Heusser, G; Kiko, J; Kirsten, T; Laubenstein, M; Pernicka, E; Rau, W; Rönn, U; Schlosser, C; Wójcik, M; Ammon, R; Ebert, K; Fritsch, T; H...espandi
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/2108/18415
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