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@ARTICLE{Agostini:889009,
      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 Biondi, R. and Bravo, D.
                      and Caccianiga, B. and Calaprice, F. and Caminata, A. and
                      Cavalcante, P. and Chepurnov, A. 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 Formozov, A. and Franco, D.
                      and Galbiati, C. and Ghiano, C. and Giammarchi, M. and
                      Goretti, A. and Göttel, A. S. and Gromov, M. and Guffanti,
                      D. and Ianni, Aldo and Ianni, Andrea and Jany, A. and
                      Jeschke, D. and Kobychev, V. and Korga, G. and Kumaran, S.
                      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 Martyn, J. and Meroni,
                      E. and Meyer, M. and Miramonti, L. and Misiaszek, M. and
                      Muratova, V. and Neumair, B. and Nieslony, M. and Nugmanov,
                      R. 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 Ranalli, M. T. and Ranucci, G. and Razeto, A. and Re,
                      A. and Redchuk, Mariia and Romani, A. and Rossi, N. and
                      Schönert, S. and Semenov, D. and Settanta, G. 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 Villante, F. L. and Vishneva, A. and
                      Vogelaar, R. B. and Feilitzsch, F. von and Wojcik, M. and
                      Wurm, M. and Zavatarelli, S. and Zuber, K. and Zuzel, G.},
      title        = {{S}ensitivity to neutrinos from the solar {CNO} cycle in
                      {B}orexino},
      journal      = {The European physical journal / C},
      volume       = {80},
      number       = {11},
      issn         = {1434-6052},
      address      = {Heidelberg},
      publisher    = {Springer},
      reportid     = {FZJ-2020-05384},
      pages        = {1091},
      year         = {2020},
      abstract     = {Neutrinos emitted in the carbon, nitrogen, oxygen (CNO)
                      fusion cycle in the Sun are a sub-dominant, yet crucial
                      component of solar neutrinos whose flux has not been
                      measured yet. The Borexino experiment at the Laboratori
                      Nazionali del Gran Sasso (Italy) has a unique opportunity to
                      detect them directly thanks to the detector’s radiopurity
                      and the precise understanding of the detector backgrounds.
                      We discuss the sensitivity of Borexino to CNO neutrinos,
                      which is based on the strategies we adopted to constrain the
                      rates of the two most relevant background sources, $pep$
                      neutrinos from the solar pp-chain and $^{210}$Bi beta decays
                      originating in the intrinsic contamination of the liquid
                      scintillator with $^{210}$Pb. Assuming the CNO flux
                      predicted by the high-metallicity Standard Solar Model and
                      an exposure of 1000 days $\times $ 71.3 t, Borexino has a
                      median sensitivity to CNO neutrino higher than 3 $\sigma $.
                      With the same hypothesis the expected experimental
                      uncertainty on the CNO neutrino flux is 23\%, provided the
                      uncertainty on the independent estimate of the $^{210}\text
                      {Bi}$ interaction rate is 1.5 $\hbox {cpd}/100~\hbox
                      {ton}$. Finally, we evaluated the expected uncertainty of
                      the C and N abundances and the expected discrimination
                      significance between the high and low metallicity Standard
                      Solar Models (HZ and LZ) with future more precise
                      measurement of the CNO solar neutrino flux.},
      cin          = {IKP-2 / JARA-HPC},
      ddc          = {530},
      cid          = {I:(DE-Juel1)IKP-2-20111104 / $I:(DE-82)080012_20140620$},
      pnm          = {612 - Cosmic Matter in the Laboratory (POF3-612) / Solar
                      and Geo-neutrino Analysis with Borexino $(jikp20_20190501)$},
      pid          = {G:(DE-HGF)POF3-612 / $G:(DE-Juel1)jikp20_20190501$},
      typ          = {PUB:(DE-HGF)16},
      UT           = {WOS:000595779500001},
      doi          = {10.1140/epjc/s10052-020-08534-2},
      url          = {https://juser.fz-juelich.de/record/889009},
}