作者: F. Kaether , W. Hampel , G. Heusser , J. Kiko , T. Kirsten
DOI: 10.1016/J.PHYSLETB.2010.01.030
关键词: Pulse shape analysis 、 Rate measurement 、 High rate 、 GALLEX 、 Flux 、 Physics 、 Nuclear physics 、 Solar neutrino 、 Neutrino 、 Calibration
摘要: Abstract After the completion of gallium solar neutrino experiments at Laboratori Nazionali del Gran Sasso ( Gallex : 1991–1997; GNO: 1998–2003) we have retrospectively updated results with help new technical data that were impossible to acquire for principle reasons before low rate measurement phase (that is, end GNO runs). Subsequent high allowed calibration absolute internal counter efficiencies and an advanced pulse shape analysis background discrimination. The overall result (only) is 73.4 − 7.3 + 7.1 SNU . This 5.3% below old value 77.5 7.8 7.5 Collaboration, W. Hampel et al., 1999 [1] ), a substantially reduced error. A similar reduction obtained from reanalysis 51Cr source 1994/1995.