%0 Conference Paper
%A Agostini, M.
%A Altenmüller, K.
%A Appel, S.
%A Atroshchenko, V.
%A Bagdasarian, Z.
%A Basilico, D.
%A Bellini, G.
%A Benziger, J.
%A Bick, D.
%A Bonfini, G.
%A Bravo, D.
%A Caccianiga, B.
%A Calaprice, F.
%A Caminata, A.
%A Cappelli, L.
%A Cavalcante, P.
%A Cavanna, F.
%A Chepurnov, A.
%A Choi, K.
%A D'Angelo, D.
%A Davini, S.
%A Derbin, A.
%A Di Giacinto, A.
%A Di Marcello, V.
%A Ding, X. F.
%A Di Lüdovico, A.
%A Di Noto, L.
%A Drachnev, I.
%A Formozov, A.
%A Franco, D.
%A Gabriele, F.
%A Galbiati, C.
%A Gschwender, M.
%A Ghiano, C.
%A Giammarchi, M.
%A Goretti, A.
%A Gromov, M.
%A Güffanti, D.
%A Hagner, C.
%A Hungerford, E.
%A Ianni, Aldo
%A Ianni, Andrea
%A Jany, A.
%A Jeschke, D.
%A Kumaran, Sindhujha
%A Kobychev, V.
%A Korga, G.
%A Lachenmaier, T.
%A Laubenstein, M.
%A Litvinovich, E.
%A Lombardi, P.
%A Lomskaya, I.
%A Ludhova, Livia
%A Lukyanchenko, G.
%A Lukyanchenko, L.
%A Machulin, I.
%A Manuzio, G.
%A Marcocci, S.
%A Maricic, J.
%A Martyn, J.
%A Meroni, E.
%A Meyer, M.
%A Miramonti, L.
%A Misiaszek, M.
%A Muratova, V.
%A Neumair, B.
%A Nieslony, M.
%A Oberauer, L.
%A Orekhov, V.
%A Ortica, F.
%A Pallavicini, M.
%A Papp, L.
%A Penek, Ömer
%A Pietrofaccia, L.
%A Pilipenko, N.
%A Pocar, A.
%A Raikov, G.
%A Ranalli, M. T.
%A Ranucci, G.
%A Razeto, A.
%A Re, A.
%A Redchuk, Mariia
%A Romani, A.
%A Rossi, N.
%A Rottenanger, S.
%A Schönert, S.
%A Semenov, D.
%A Skorokhvatov, M.
%A Smirnov, O.
%A Sotnikov, A.
%A Suvorov, Y.
%A Tartaglia, R.
%A Testera, G.
%A Thurn, J.
%A Unzhakov, E.
%A Vishneva, A.
%A Vogelaar, R. B.
%A von Feilitzsch, F.
%A Wojcik, M.
%A Wurm, M.
%A Zaimidoroga, O.
%A Zavatarelli, S.
%A Zuber and G. Zuzel, K.
%A Zavatarelli, S.
%T The study of solar neutrinos and of non-standard neutrino interactions with Borexino
%J Journal of physics / Conference Series
%V 1468
%N 1
%@ 1742-6588
%C Bristol
%I IOP Publ.
%M FZJ-2020-01796
%P 012192
%D 2020
%X The Borexino liquid scintillator neutrino observatory has a unique capability toperform high-precision solar neutrino observations thanks to its exceptional radiopurity andgood energy resolution (5% at 1 MeV). A comprehensive study of the pp-chain neutrinos waspresented that includes the direct measurements of 7Be, pp and pep neutrino fluxes with thehighest precision ever achieved (down to 2.8% in the 7Be component), the 8B with the lowestenergy threshold, the best limit on CNO neutrinos and the first Borexino limit on hep neutrinos.These results are important to validate the MSW-LMA oscillation paradigm across the full solarenergy range and to exclude possible Non-Standard neutrino Interactions (NSIs). In particularthe effects of neutrino-flavor-diagonal Neutral-Current (NC) interactions that modify the νeeand ντ e couplings while preserving their chiral and flavor structures, have been investigated. Atdetection, the shape of the electron-recoil spectrum is affected by changes in the νee and ντ ecouplings, quantified by the parameters εL/Re and εL/Rτ . New bounds to all four parameters wereobtained, quite stringent compared to the global ones. In particular, the best constraint to-dateon εLe was achieved. A comprehensive summary of all the recent results on solar neutrinos fromBorexino is reported in the present paper.
%B 16th International Conference on Topics in Astroparticle and Underground physics
%C 9 Sep 2019 - 13 Sep 2019, Toyama (Japan)
Y2 9 Sep 2019 - 13 Sep 2019
M2 Toyama, Japan
%F PUB:(DE-HGF)16 ; PUB:(DE-HGF)8
%9 Journal ArticleContribution to a conference proceedings
%U <Go to ISI:>//WOS:000539995300191
%R 10.1088/1742-6596/1468/1/012192
%U https://juser.fz-juelich.de/record/875087