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@INPROCEEDINGS{Agostini:875087,
      author       = {Agostini, M. and Altenmüller, K. and Appel, S. and
                      Atroshchenko, V. and Bagdasarian, Z. and Basilico, D. and
                      Bellini, G. and Benziger, J. and Bick, D. and Bonfini, G.
                      and Bravo, D. and Caccianiga, B. and Calaprice, F. and
                      Caminata, A. and Cappelli, L. and Cavalcante, P. and
                      Cavanna, F. and Chepurnov, A. and Choi, K. and D'Angelo, D.
                      and Davini, S. and Derbin, A. and Di Giacinto, A. and Di
                      Marcello, V. and Ding, X. F. and Di Lüdovico, A. and Di
                      Noto, L. and Drachnev, I. and Formozov, A. and Franco, D.
                      and Gabriele, F. and Galbiati, C. and Gschwender, M. and
                      Ghiano, C. and Giammarchi, M. and Goretti, A. and Gromov, M.
                      and Güffanti, D. and Hagner, C. and Hungerford, E. and
                      Ianni, Aldo and Ianni, Andrea and Jany, A. and Jeschke, D.
                      and Kumaran, Sindhujha and Kobychev, V. and Korga, G. and
                      Lachenmaier, T. and Laubenstein, M. and Litvinovich, E. and
                      Lombardi, P. and Lomskaya, I. and Ludhova, Livia and
                      Lukyanchenko, G. and Lukyanchenko, L. and Machulin, I. and
                      Manuzio, G. and Marcocci, S. and Maricic, J. and Martyn, J.
                      and Meroni, E. and Meyer, M. and Miramonti, L. and
                      Misiaszek, M. and Muratova, V. and Neumair, B. and Nieslony,
                      M. and Oberauer, L. and Orekhov, V. and Ortica, F. and
                      Pallavicini, M. and Papp, L. and Penek, Ömer and
                      Pietrofaccia, L. and Pilipenko, N. and Pocar, A. and Raikov,
                      G. and Ranalli, M. T. and Ranucci, G. and Razeto, A. and Re,
                      A. and Redchuk, Mariia and Romani, A. and Rossi, N. and
                      Rottenanger, S. and Schönert, S. and Semenov, D. and
                      Skorokhvatov, M. and Smirnov, O. and Sotnikov, A. and
                      Suvorov, Y. and Tartaglia, R. and Testera, G. and Thurn, J.
                      and Unzhakov, E. and Vishneva, A. and Vogelaar, R. B. and
                      von Feilitzsch, F. and Wojcik, M. and Wurm, M. and
                      Zaimidoroga, O. and Zavatarelli, S. and Zuber and G. Zuzel,
                      K. and Zavatarelli, S.},
      title        = {{T}he study of solar neutrinos and of non-standard neutrino
                      interactions with {B}orexino},
      journal      = {Journal of physics / Conference Series},
      volume       = {1468},
      number       = {1},
      issn         = {1742-6588},
      address      = {Bristol},
      publisher    = {IOP Publ.},
      reportid     = {FZJ-2020-01796},
      pages        = {012192},
      year         = {2020},
      abstract     = {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.},
      month         = {Sep},
      date          = {2019-09-09},
      organization  = {16th International Conference on
                       Topics in Astroparticle and Underground
                       physics, Toyama (Japan), 9 Sep 2019 -
                       13 Sep 2019},
      cin          = {IKP-2},
      ddc          = {530},
      cid          = {I:(DE-Juel1)IKP-2-20111104},
      pnm          = {612 - Cosmic Matter in the Laboratory (POF3-612)},
      pid          = {G:(DE-HGF)POF3-612},
      typ          = {PUB:(DE-HGF)16 / PUB:(DE-HGF)8},
      UT           = {WOS:000539995300191},
      doi          = {10.1088/1742-6596/1468/1/012192},
      url          = {https://juser.fz-juelich.de/record/875087},
}