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@INPROCEEDINGS{Fogli:308160,
      author       = {Fogli, G. L. and Lisi, E. and Marrone, A. and Montanino, D.
                      and Palazzo, A. and Rotunno, A. M.},
      title        = {{N}eutrino oscillations: {A} {G}lobal analysis},
      reportid     = {PUBDB-2016-03511, hep-ph/0310012. PIC-2003-THAT05},
      pages        = {49-64},
      year         = {2003},
      abstract     = {We review the status of the neutrino oscillation physics
                      (as of June 2003), with a particular emphasis on the present
                      knowledge of the neutrino mass-mixing parameters in a three
                      generation approach. We consider first the $nu_mu-->nu_tau$
                      flavor transitions of atmospheric neutrinos. It is found
                      that standard oscillations provide the best description of
                      the SK+K2K data, and that the associated mass-mixing
                      parameters are determined at 1 sigma (and dof=1) as: Delta
                      $m^2=(2.6$ +-0.4) x $10^-3$ $eV^2$ and
                      $sin^2(2theta)=1.00+0.00-0.05.$ Such indications, presently
                      dominated by SK, could be strengthened by further K2K data.
                      Then we analyze the energy spectrum of reactor neutrino
                      events recently observed at KamLAND and combine them with
                      solar and terrestrial neutrino data. We find that the
                      solution to the solar neutrino problem at large mixing angle
                      (LMA) is basically split into two sub-regions, that we
                      denote as LMA-I and LMA-II. The LMA-I solution,
                      characterized by lower values of the squared neutrino mass
                      gap, is favored by the global data fit. Finally, we briefly
                      illustrate how prospective data from the SNO and KamLAND can
                      increase our confidence in the occurrence of standard matter
                      effects in the Sun, which are starting to emerge from
                      current data.},
      month         = {Jun},
      date          = {2003-06-26},
      organization  = {23rd International Conference on
                       Physics in Collision, Zeuthen
                       (Germany), 26 Jun 2003 - 28 Jun 2003},
      keywords     = {talk: Zeuthen 2003/06/26 (INSPIRE) / review (INSPIRE) /
                      neutrino: oscillation (INSPIRE) / neutrino: mass (INSPIRE) /
                      neutrino: mixing angle (INSPIRE) / neutrino: flavor
                      (INSPIRE) / flavor: 2 (INSPIRE) / flavor: 3 (INSPIRE) /
                      neutrino: cosmic radiation (INSPIRE) / neutrino: solar
                      (INSPIRE) / neutrino: particle source (INSPIRE) / neutrino:
                      mass difference (INSPIRE) / model: solar (INSPIRE) / matter:
                      effect (INSPIRE) / statistical analysis (INSPIRE) /
                      numerical calculations: interpretation of experiments
                      (INSPIRE) / bibliography (INSPIRE)},
      cin          = {L},
      cid          = {I:(DE-H253)L-20120731},
      pnm          = {899 - ohne Topic (POF3-899)},
      pid          = {G:(DE-HGF)POF3-899},
      experiment   = {EXP:(DE-H253)HERA(machine)-20150101},
      typ          = {PUB:(DE-HGF)29 / PUB:(DE-HGF)8},
      url          = {https://bib-pubdb1.desy.de/record/308160},
}