TY - JOUR
T1 - Solar neutrino results and future prospects with the Borexino detector
AU - The Borexino Collaboration
AU - Miramonti, L.
AU - Agostini, M.
AU - Altenmüller, K.
AU - Appel, S.
AU - Atroshchenko, V.
AU - Bagdasarian, Z.
AU - Basilico, D.
AU - Bellini, G.
AU - Benziger, J.
AU - Bick, D.
AU - Bonfini, G.
AU - Bravo, D.
AU - Caccianiga, B.
AU - Calaprice, F.
AU - Caminata, A.
AU - Cappelli, L.
AU - Cavalcante, P.
AU - Cavanna, F.
AU - Chepurnov, A.
AU - Choi, K.
AU - D'Angelo, D.
AU - Davini, S.
AU - Derbin, A.
AU - Di Giacinto, A.
AU - Di Marcello, V.
AU - Ding, X. F.
AU - Di Ludovico, A.
AU - Di Noto, L.
AU - Drachnev, I.
AU - Formozov, A.
AU - Franco, D.
AU - Gabriele, F.
AU - Galbiati, C.
AU - Gschwender, M.
AU - Ghiano, C.
AU - Giammarchi, M.
AU - Goretti, A.
AU - Gromov, M.
AU - Guffanti, D.
AU - Hagner, C.
AU - Hungerford, E.
AU - Ianni, Aldo
AU - Ianni, Andrea
AU - Jany, A.
AU - Jeschke, D.
AU - Kumaran, S.
AU - Kobychev, V.
AU - Korga, G.
AU - Lachenmaier, T.
AU - Laubenstein, M.
N1 - Publisher Copyright:
© 2012 IEEE Computer Society. All rights reserved.
PY - 2021/1/23
Y1 - 2021/1/23
N2 - Neutrinos coming from the Sun have played a crucial role in the discovery of neutrino oscillations and they still are proving to be a unique and powerful tool in the investigation of the fusion reactions that power the stars, as well as representing a probe to study the basic neutrino properties. The Borexino detector has started its data acquisition in 2007 in the underground Gran Sasso National Laboratories (LNGS) in Italy. The main goal of Borexino is the real-time study of low energy neutrinos with an energy threshold as low as about 50 keV. A first phase named Borexino Phase-I started in 2007 and ended in 2010, then after a purification campaign, data-taking resumed in 2011 with the so-called Borexino Phase-II. I will present the recent results of Borexino for the measurement of the four main solar neutrino components of the pp fusion chain (pp, pep, 7Be, 8B), and the upper limits on the remaining two solar neutrino fluxes (CNO and hep).
AB - Neutrinos coming from the Sun have played a crucial role in the discovery of neutrino oscillations and they still are proving to be a unique and powerful tool in the investigation of the fusion reactions that power the stars, as well as representing a probe to study the basic neutrino properties. The Borexino detector has started its data acquisition in 2007 in the underground Gran Sasso National Laboratories (LNGS) in Italy. The main goal of Borexino is the real-time study of low energy neutrinos with an energy threshold as low as about 50 keV. A first phase named Borexino Phase-I started in 2007 and ended in 2010, then after a purification campaign, data-taking resumed in 2011 with the so-called Borexino Phase-II. I will present the recent results of Borexino for the measurement of the four main solar neutrino components of the pp fusion chain (pp, pep, 7Be, 8B), and the upper limits on the remaining two solar neutrino fluxes (CNO and hep).
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U2 - 10.1088/1742-6596/1766/1/012006
DO - 10.1088/1742-6596/1766/1/012006
M3 - Conference article
AN - SCOPUS:85104230706
SN - 1742-6588
VL - 1766
JO - Journal of Physics: Conference Series
JF - Journal of Physics: Conference Series
IS - 1
M1 - 012006
T2 - 10th International Conference on High Energy and Astroparticle Physics, TIC-HEAP 2019
Y2 - 19 October 2019 through 21 October 2019
ER -