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

By The Borexino Collaboration. 2008

158 citations recorded by the source corpus.

G. Bellini, J. Benziger, S. Bonetti, M. Buizza Avanzini, B. Caccianiga, L. Cadonati, F. Calaprice, C. Carraro, A. Chavarria, A. Chepurnov, F. Dalnoki-Veress, D. D’Angelo, S. Davini, H. de Kerret, A. Derbin, A. Etenko, K. Fomenko, D. Franco, C. Galbiati, S. Gazzana, C. Ghiano, M. Giammarchi, M. Goeger-Neff, A. Goretti, E. Guardincerri, S. Hardy, Aldo Ianni, Andrea Ianni, M. Joyce, G. Korga, D. Kryn, M. Laubenstein, M. Leung, T. Lewke, E. Litvinovich, B. Loer, P. Lombardi, L. Ludhova, I. Machulin, S. Manecki, W. Maneschg, G. Manuzio, Q. Meindl, E. Meroni, L. Miramonti, M. Misiaszek, 11 D. Montanari, V. Muratova, L. Oberauer, M. Obolensky, F. Ortica, M. Pallavicini, L. Papp, L. Perasso, S. Perasso, A. Pocar, R.S. Raghavan, G. Ranucci, A. Razeto, A. Re, P. Risso, A. Romani, D. Rountree, A. Sabelnikov, R. Saldanha, C. Salvo, S. Schönert, H. Simgen, M. Skorokhvatov, O. Smirnov, A. Sotnikov, S. Sukhotin, Y. Suvorov, 9 R. Tartaglia, G. Testera, D. Vignaud, R.B. Vogelaar, F. von Feilitzsch, J. Winter, M. Wojcik, A. Wright, M. Wurm, J. Xu, O. Zaimidoroga, S. Zavatarelli, and G. Zuzel

Subfields: Nuclear and High Energy Physics

View Paper: https://www.semanticscholar.org/paper/a811a6fadd1e5e431396006c2fb8e219dc704da7

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Citations in the corpus

• 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 global analysis of neutrino oscillations in the presence of eV-scale sterile neutrinos (2018, unknown): “Borexino [46, 82, 83] 81 Phases I and II νe scattering on carbon (νe + 12C→ e− + 12N) (32)”
• A White Paper on keV sterile neutrino Dark Matter (2016, background): “In brief, at present we have observed neutrino oscillation effects in: • atmospheric neutrinos, in particular in the high-statistics results of Super-Kamiokande [90]; • event rates of solar neutrino radiochemical experiments Chlorine [91], GALLEX/GNO [92], and SAGE [93], as well as time- and energy-”
• Global analysis of three-flavour neutrino oscillations: synergies and tensions in the determination of θ23, δCP, and the mass ordering (2018, unknown): “• Borexino Phase-I 246-day high-energy data [66], 6 data points.”
• Neutrino oscillations (2013, unknown): “2MeV) [85] neutrino fluxes and to obtain an upper limit for the CNO neutrino flux [22].”
• Global Analyses of Neutrino Oscillation Experiments (2015, background): “In brief, at present we have observed neutrino oscillation effects in: • atmospheric neutrinos, in particular in the high-statistics results of Super-Kamiokande [4]; • event rates of solar neutrino radiochemical experiments Chlorine [5], Gallex/GNO [6] and SAGE [7], as well as time and energy depend”
• Neutrino Oscillations and Non-standard Interactions (2017, background): “Moreover, Borexino has also measured the solar (8)B rate with a very low energy threshold of 3 MeV [52] and it has also provided the first real–time observation of the very low energy pp neutrinos [53].”
• Evidence of $\theta_{13}$>0 from global neutrino data analysis (2011, methodology): “With respect to [26], we update the KamLAND results on reactor and geoneutrino data [16, 27], and include the Borexino total event rates of (7)Be [28] and (8)B [29] solar neutrinos.”
• Determination of matter potential from global analysis of neutrino oscillation data (2013, background): “7 days of Borexino data [65] as well as their high-energy spectrum from 246 live days [66].”
• Updated fit to three neutrino mixing: exploring the accelerator-reactor complementarity (2016, unknown): “• Borexino Phase-I 246-day high-energy data [25], 6 data points.”
• Updated fit to three neutrino mixing: status of leptonic CP violation (2014, background): “7 days of Borexino data [27] as well as their high-energy spectrum from 246 live days [28].”