Complete results for five years of GNO solar neutrino observations

Altmann, M.; Balata, M.; Belli, P.; Bellotti, E.; Bernabei, R.; Burkert, E.; Cattadori, C.; Cerulli, R.; Chiarini, Marco; Cribier, M.; d’Angelo, S.; Del Re, G.; Ebert, Klaus; von Feilitzsch, F.; Ferrari, N.; Hampel, W.; Hartmann, F.; Henrich, E.; Heusser, G.; Kaether, F.; Kiko, J.; Kirsten, T.; Lachenmaier, T.; L. Lanfranchi, J.; Laubenstein, M.; Lützenkirchen, Klaus; Mayer, Klaus; Moegel, P.; Motta, D.; Nisi, S.; Oehm, J.; Pandola, L.; Petricca, F.; Potzel, W.; Richter, H.; Schoenert, S.; Wallenius, Maria; Wójcik, M.; Zanotti, L.

doi:10.1016/j.physletb.2005.04.068

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Complete results for five years of GNO solar neutrino observations

Published in Physics Letters B • May 11, 2005

Authors:

M. Altmann

M. Balata

P. Belli

Abstract

We report the complete GNO solar neutrino results for the measuring periods GNO III, GNO II, and GNO I. The result for GNO III (last 15 solar runs) is [54.3−9.3+9.9(stat)±2.3(syst)]SNU (1σ) or [54.3−9.6+10.2(incl. syst)]SNU (1σ) with errors combined. The GNO experiment is now terminated after altoge...

Subject

Solar neutrino

Physics

Neutrino

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