Measurement of the solar 8B neutrino rate with a liquid scintillator target and 3 MeV energy threshold in the Borexino detector

By G. Bellini, Jay B. Benziger, M. Avanzini, B. Caccianiga, L. Cadonati, F. Calaprice, C. Carraro, A. Chavarria, F. Dalnoki-Veress, D. D’Angelo and 77 more. 2010

199 citations recorded by the source corpus.

Subfields: Nuclear and High Energy Physics

View Paper: https://www.semanticscholar.org/paper/a6ac5eef83f6588710574e674b240b5debbbf4d3

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Citations in the corpus

Updated fit to three neutrino mixing: status of leptonic CP violation (2014, methodology): “tion given in their combined analysis [26] which amount to 7 data points. We also include the main set of the 740.7 days of Borexino data [27] as well as their high-energy spectrum from 246 live days [28]. In the analysis of solar neutrino data we use the GS98 version of the solar standard model [29”
The fate of hints: updated global analysis of three-flavor neutrino oscillations (2020, unknown): “• Borexino Phase-I 246-day high-energy data [45], 6 data points.”
Sterile neutrino oscillations: the global picture (2013, background): “7 days of Borexino data [136] as well as their high-energy spectrum from 246 live days [137].”
Updated fit to three neutrino mixing: exploring the accelerator-reactor complementarity (2016, background): “y energy spectrum [22], 24 data points. SNO combined analysis [23], 7 data points. { 25 { Borexino Phase-I 740.7-day low-energy data [24], 33 data points. Borexino Phase-I 246-day high-energy data [25], 6 data points. Borexino Phase-II 408-day low-energy data [26], 42 data points. Atmospheric experi”
Solar Neutrinos: Status and Prospects (2012, result): “A ES rate for 8B neutrinos, based on a integration above 3 MeV, corre- sponding to an equivalent flux of φES(8B) = (2.4 ± 0.4 ± 0.1) × 106/cm2s (Borexino Collaboration, G. Bellini et al. 2010), less precise than but in good agreement with SNO and Super-Kamiokande results.”
SOLAR MODELS WITH ACCRETION. I. APPLICATION TO THE SOLAR ABUNDANCE PROBLEM (2011, unknown): “The luminosity constraint and the 7Be measurement by Borexino combine to produce the small uncertainties in these fluxes (about 1% and 1.5%, respectively).”
Determination of matter potential from global analysis of neutrino oscillation data (2013, methodology): “f the 1097-day energy spectrum and day-night asymmetry of SK4 [64]. We { 7 { also include the main set of the 740.7 days of Borexino data [65] as well as their high-energy spectrum from 246 live days [66]. The results of the three phases of SNO are included in two dierent forms. First, we perform ou”