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18 April 2024

» arxiv » hep-ex/0504037

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Complete results for five years of GNO solar neutrino observations
GNO COLLABORATION: M. Altmann ; M. Balata ; P. Belli ; E. Bellotti ; R. Bernabei ; E. Burkert ; C. Cattadori ; R. Cerulli ; M. Chiarini ; M. Cribier ; S. d’Angelo ; G. Del Re ; K. H. Ebert ; F. v. Feilitzsch ; N. Ferrari ; W. Hampel ; F. X. Hartmann ; E. Henrich ; G. Heusser ; F. Kaether ; J. Kiko ; T. Kirsten ; T. Lachenmaier ; J. Lanfranchi ; M. Laubenstein ; K. Luetzenkirchen ; K. Mayer ; P. Moegel ; D. Motta ; S. Nisi ; J. Oehm ; L. Pandola ; F. Petricca ; W. Potzel ; H. Richter ; S. Schoenert ; M. Wallenius ; M. Wojcik ; L. Zanotti ;
Date:	19 Apr 2005
Journal:	Phys.Lett. B616 (2005) 174-190
Subject:	hep-ex astro-ph
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 + 9.9 - 9.3 (stat.)+- 2.3 (syst.)] SNU (1 sigma) or [54.3 + 10.2 - 9.6 (incl. syst.)] SNU (1 sigma) with errors combined. The GNO experiment is now terminated after altogether 58 solar exposure runs that were performed between May 20, 1998 and April 9, 2003. The combined result for GNO (I+II+III) is [62.9 + 5.5 - 5.3 (stat.) +- 2.5 (syst.)] SNU (1 sigma) or [62.9 + 6.0 - 5.9] SNU (1 sigma) with errors combined in quadrature. Overall, gallium based solar observations at LNGS (first in GALLEX, later in GNO) lasted from May 14, 1991 through April 9, 2003. The joint result from 123 runs in GNO and GALLEX is [69.3 +- 5.5 (incl. syst.)] SNU (1 sigma). The distribution of the individual run results is consistent with the hypothesis of a neutrino flux that is constant in time. Implications from the data in particle- and astrophysics are reiterated.
Source:	arXiv, hep-ex/0504037
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