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@ARTICLE{Agarwalla:890649,
      author       = {Agarwalla, S. K. and 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
                      Ludovico, A. and Di Noto, L. and Drachnev, I. and Fomenko,
                      K. 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 Guffanti,
                      D. and Hagner, C. and Hungerford, E. and Ianni, Aldo and
                      Ianni, Andrea and Jany, A. and Jeschke, D. and Kumaran, S.
                      and Kobychev, V. and Korga, G. and Lachenmaier, T. and
                      Laubenstein, M. and Litvinovich, E. and Lombardi, P. and
                      Ludhova, L. 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, Ö. and Pietrofaccia, L. and Pilipenko, N. and Pocar,
                      A. and Raikov, G. and Ranucci, G. and Razeto, A. and Re, A.
                      and Redchuk, M. 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 Sun,
                      C. and Suvorov, Y. and Takeuchi, T. 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, K. and Zuzel, G.},
      title        = {{C}onstraints on flavor-diagonal non-standard neutrino
                      interactions from {B}orexino {P}hase-{II}},
      journal      = {Journal of high energy physics},
      volume       = {2020},
      number       = {2},
      issn         = {1029-8479},
      address      = {[Trieste]},
      publisher    = {SISSA},
      reportid     = {FZJ-2021-01097},
      pages        = {38},
      year         = {2020},
      abstract     = {The Borexino detector measures solar neutrino fluxes via
                      neutrino-electron elastic scattering. Observed spectra are
                      determined by the solar-νe survival probability Pee(E), and
                      the chiral couplings of the neutrino and electron. Some
                      theories of physics beyond the Standard Model postulate the
                      existence of Non-Standard Interactions (NSI’s) which
                      modify the chiral couplings and Pee(E). In this paper, we
                      search for such NSI’s, in particular, flavor-diagonal
                      neutral current interactions that modify the νee and ντe
                      couplings using Borexino Phase II data. Standard Solar Model
                      predictions of the solar neutrino fluxes for both high- and
                      low-metallicity assumptions are considered. No indication of
                      new physics is found at the level of sensitivity of the
                      detector and constraints on the parameters of the NSI’s
                      are placed. In addition, with the same dataset the value of
                      sin2θW is obtained with a precision comparable to that
                      achieved in reactor antineutrino experiments},
      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},
      UT           = {WOS:000520506100001},
      doi          = {10.1007/JHEP02(2020)038},
      url          = {https://juser.fz-juelich.de/record/890649},
}