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Reanalysis of the GALLEX solar neutrino flux and source experiments · Around

2010

Reanalysis of the GALLEX solar neutrino flux and source experiments

Kaether, F., Hampel, W., Heusser, G. et al.

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After the completion of the gallium solar neutrino experiments at the Laboratori Nazionali del Gran Sasso (GALLEX}: 1991-1997; GNO: 1998-2003) we have retrospectively updated the GALLEX results with the help of new technical data that were impossible to acquire for principle reasons before the completion of the low rate measurement phase (that is, before the end of the GNO solar runs).

Subsequent high rate experiments have allowed the calibration of absolute internal counter efficiencies and of an advanced pulse shape analysis for counter background discrimination.
The updated overall result for GALLEX (only) is (73.4 +7.1 -7.3) SNU.
This is 5.3% below the old value of (77.5 + 7.5 -7.8) SNU (PLB 447 (1999) 127-133) with a substantially reduced error.

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Then

F. Kaether, Master Thesis, Universität Heidelberg 2003
2003
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L. Pandola, Ph. D. Thesis, Università degli Studi dell’Aquila, 2004
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J. N. Bahcall, C. Pe n ~ \tilde{\rm n} a-Garay, New Journal of Physics 6 (2004) 63
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GNO Collaboration, M. Altmann et al., Physics Letters B 616 (2005) 174-190
2005
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F. Kaether, Ph. D. Thesis, Universität Heidelberg 2007
2007
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