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@ARTICLE{Agostini:863235,
      author       = {Agostini, M. and Altenmüller, K. and Appel, S. and
                      Atroshchenko, V. and Bagdasarian, Zara 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 Caprioli, S. and Carlini, M. and
                      Cavalcante, P. and Chepurnov, A. and Choi, K. and Collica,
                      L. and D’Angelo, D. and Davini, S. and Derbin, A. 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 Ghiano, C. and
                      Giammarchi, M. and Goretti, A. and Gromov, M. and Guffanti,
                      D. and Hagner, C. and Houdy, T. and Hungerford, E. and
                      Ianni, Aldo and Ianni, Andrea and Jany, A. and Jeschke, D.
                      and Kobychev, V. and Korablev, D. and Korga, G. and Kryn, D.
                      and Laubenstein, M. and Litvinovich, E. and Lombardi, F. and
                      Lombardi, P. and Ludhova, Livia and Lukyanchenko, G. and
                      Lukyanchenko, L. and Machulin, I. and Manuzio, G. and
                      Marcocci, S. and Martyn, J. and Meroni, E. and Meyer, M. and
                      Miramonti, L. and Misiaszek, M. and Muratova, V. and
                      Neumair, B. and Oberauer, L. and Opitz, B. and Orekhov, V.
                      and Ortica, F. and Pallavicini, M. and Papp, L. and Penek,
                      Ömer and Pilipenko, N. and Pocar, A. and Porcelli, A. and
                      Raikov, G. and Ranucci, G. and Razeto, A. and Re, A. and
                      Redchuk, Mariia and Romani, A. and Roncin, R. and Rossi, N.
                      and Schönert, S. and Semenov, D. and Skorokhvatov, M. and
                      Smirnov, O. and Sotnikov, A. and Stokes, L. F. F. and
                      Suvorov, Y. and Tartaglia, R. and Testera, G. and Thurn, J.
                      and Toropova, M. and Unzhakov, E. and Villante, F. L. and
                      Vishneva, A. and Vogelaar, R. B. and von Feilitzsch, F. and
                      Wang, H. and Weinz, S. and Wojcik, M. and Wurm, M. and
                      Yokley, Z. and Zaimidoroga, O. and Zavatarelli, S. and
                      Zuber, K. and Zuzel, G.},
      title        = {{C}omprehensive measurement of pp-chain solar neutrinos},
      journal      = {Nature},
      volume       = {562},
      issn         = {0028-0836},
      address      = {London [u.a.]},
      publisher    = {Nature Publ. Group},
      reportid     = {FZJ-2019-03325},
      pages        = {505 - 510},
      year         = {2018},
      abstract     = {About 99 per cent of solar energy is produced through
                      sequences of nuclear reactions that convert hydrogen into
                      helium, starting from the fusion of two protons (the pp
                      chain). The neutrinos emitted by five of these reactions
                      represent a unique probe of the Sun’s internal working
                      and, at the same time, offer an intense natural neutrino
                      beam for fundamental physics. Here we report a complete
                      study of the pp chain. We measure the neutrino–electron
                      elastic-scattering rates for neutrinos produced by four
                      reactions of the chain: the initial proton–proton fusion,
                      the electron-capture decay of beryllium-7, the three-body
                      proton–electron–proton (pep) fusion, here measured with
                      the highest precision so far achieved, and the boron-8 beta
                      decay, measured with the lowest energy threshold. We also
                      set a limit on the neutrino flux produced by the
                      3He–proton fusion (hep). These measurements provide a
                      direct determination of the relative intensity of the two
                      primary terminations of the pp chain (pp-I and pp-II) and an
                      indication that the temperature profile in the Sun is more
                      compatible with solar models that assume high surface
                      metallicity. We also determine the survival probability of
                      solar electron neutrinos at different energies, thus probing
                      simultaneously and with high precision the neutrino
                      flavour-conversion paradigm, both in vacuum and in
                      matter-dominated regimes.},
      cin          = {IKP-2 / JARA-HPC},
      ddc          = {500},
      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 $(jikp20_20180501)$},
      pid          = {G:(DE-HGF)POF3-612 / $G:(DE-Juel1)jikp20_20180501$},
      typ          = {PUB:(DE-HGF)16},
      pubmed       = {pmid:30356186},
      UT           = {WOS:000448277800043},
      doi          = {10.1038/s41586-018-0624-y},
      url          = {https://juser.fz-juelich.de/record/863235},
}