Measurement of the solar neutrino capture rate with gallium metal. III:2002-2007
By J. N. Abdurashitov, V. Gavrin, S. V. Girin, V. Gorbachev, T. Ibragimova, A. Kalikhov, N. G. Khairnasov, T. Knodel, I. Mirmov, A. Shikhin and 15 more. 2009
346 citations recorded by the source corpus.
Subfields: Nuclear and High Energy Physics
View Paper: https://www.semanticscholar.org/paper/262c94bd6390c5204c16396f3e10c083da56b7b0
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In Nuclear and High Energy Physics
- C. Giunti
- G. Mart'inez-Pinedo
- K. Langanke
- Julien Lesgourgues
- P. Krastev
- C. Buck
- S. Boser
- A. Y. Smirnov
Citations in the corpus
- Nuclear weak-interaction processes in stars (2002, background): “…for example, for 37Cl (Aufderheide et al., 1994a), 40Ar (Ormand et al., 1995) and 71Ga (Haxton, 1998), the detector material in the Homestake (Cleveland et al., 1998), ICARUS4, and GALLEX/SAGE/GNO detectors (Abdurashitov et al., 1999; Altmann et al., 2000; Hampel et al., 1999), respectively.”
- Solar neutrinos: Global analysis and implications for SNO (2001, methodology): “The allowed regions at dierentcondencelevelsarepresentedforneutrinooscillationmodelsthattthetotalratesmeasuredinthechlorine[8]andgallium[ 4 ,5,7]solarneutrinosexperiments, as well as the electron recoil energy spectrum measured by the Super-Kamiokande collaboration[6]duringthedayandthespectrummeasur”