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@ARTICLE{He:911312,
      author       = {He, Miao and Göttel, Alexandre and Kampmann, Philipp and
                      Liu, Runxuan and Ludhova, Livia and Pelicci, Luca and Rifai,
                      Mariam and Schever, Michaela and Settanta, Giulio and
                      Vollbrecht, Moritz Cornelius},
      title        = {{S}ub-percent {P}recision {M}easurement of {N}eutrino
                      {O}scillation {P}arameters with {JUNO}},
      journal      = {Chinese physics / C},
      volume       = {46},
      issn         = {0254-3052},
      address      = {Bristol [u.a.]},
      publisher    = {IOP Publ.},
      reportid     = {FZJ-2022-04605},
      pages        = {123001},
      year         = {2022},
      abstract     = {JUNO is a multi-purpose neutrino observatory under
                      construction in the south of China. This publication
                      presents new sensitivity estimates for the measurement of
                      the ∆m$^2_{31}$, ∆m$^2_{21}$, sin$^2θ_{12}$, and
                      sin$^2θ_{13}$ oscillation parameters using reactor
                      antineutrinos, which is one of the primary physics goals of
                      the experiment. The sensitivities are obtained using the
                      best knowledge available to date on the location and
                      overburden of the experimental site, the nuclear reactors in
                      the surrounding area and beyond, the detector response
                      uncertainties, and the reactor antineutrino spectral shape
                      constraints expected from the TAO satellite detector. It is
                      found that the ∆m$^2_{21}$ and sin$^2θ_{12}$ oscillation
                      parameters will be determined to better than 0.5\% precision
                      in six years of data collection. In the same period, the
                      ∆m$^2_{31}$ parameter willbe determined to about 0.2\%
                      precision for each mass ordering hypothesis. The new
                      precision represents approximately an order of magnitude
                      improvement over existing constraints for these three
                      parameters.},
      cin          = {IKP-2},
      ddc          = {530},
      cid          = {I:(DE-Juel1)IKP-2-20111104},
      pnm          = {612 - Cosmic Matter in the Laboratory (POF4-612)},
      pid          = {G:(DE-HGF)POF4-612},
      typ          = {PUB:(DE-HGF)16},
      UT           = {WOS:000928183400001},
      doi          = {10.1088/1674-1137/ac8bc9},
      url          = {https://juser.fz-juelich.de/record/911312},
}