TY - JOUR
T1 - Seasonal modulation of the 7Be solar neutrino rate in Borexino
AU - The Borexino Collaboration
AU - Agostini, M.
AU - Altenmüller, K.
AU - Appel, S.
AU - Atroshchenko, V.
AU - Basilico, D.
AU - Bellini, G.
AU - Benziger, Jay Burton
AU - Bick, D.
AU - Bonfini, G.
AU - Borodikhina, L.
AU - Bravo, D.
AU - Caccianiga, B.
AU - Calaprice, F.
AU - Caminata, A.
AU - Caprioli, S.
AU - Carlini, M.
AU - Cavalcante, P.
AU - Chepurnov, A.
AU - Choi, K.
AU - D'Angelo, D.
AU - Davini, S.
AU - Derbin, A.
AU - Ding, X. F.
AU - Di Noto, L.
AU - Drachnev, I.
AU - Fomenko, K.
AU - Franco, D.
AU - Froborg, F.
AU - Gabriele, F.
AU - Galbiati, Cristiano
AU - Ghiano, C.
AU - Giammarchi, M.
AU - Goeger-Neff, M.
AU - Goretti, A.
AU - Gromov, M.
AU - Hagner, C.
AU - Houdy, T.
AU - Hungerford, E.
AU - Ianni, Aldo
AU - Ianni, Andrea
AU - Jany, A.
AU - Jeschke, D.
AU - Kobychev, V.
AU - Korablev, D.
AU - Korga, G.
AU - Kryn, D.
AU - Laubenstein, M.
AU - Lehnert, B.
AU - Litvinovich, E.
AU - Lombardi, F.
N1 - Publisher Copyright:
© 2017 Elsevier B.V.
PY - 2017/6
Y1 - 2017/6
N2 - We present the evidence for the seasonal modulation of the 7Be neutrino interaction rate with the Borexino detector at the Laboratori Nazionali del Gran Sasso in Italy. The period, amplitude, and phase of the observed time evolution of the signal are consistent with its solar origin, and the absence of an annual modulation is rejected at 99.99% C.L. The data are analyzed using three methods: the analytical fit to event rate, the Lomb-Scargle and the Empirical Mode Decomposition techniques, which all yield results in excellent agreement.
AB - We present the evidence for the seasonal modulation of the 7Be neutrino interaction rate with the Borexino detector at the Laboratori Nazionali del Gran Sasso in Italy. The period, amplitude, and phase of the observed time evolution of the signal are consistent with its solar origin, and the absence of an annual modulation is rejected at 99.99% C.L. The data are analyzed using three methods: the analytical fit to event rate, the Lomb-Scargle and the Empirical Mode Decomposition techniques, which all yield results in excellent agreement.
KW - Liquid scintillators detectors
KW - Low background detectors
KW - Neutrino oscillations
KW - Solar neutrinos
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U2 - 10.1016/j.astropartphys.2017.04.004
DO - 10.1016/j.astropartphys.2017.04.004
M3 - Article
AN - SCOPUS:85033216793
SN - 0927-6505
VL - 92
SP - 21
EP - 29
JO - Astroparticle Physics
JF - Astroparticle Physics
ER -