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@INPROCEEDINGS{Ludhova:1018460,
      author       = {Ludhova, Livia},
      title        = {{JUNO} {S}tatus and {P}hysics {P}otential},
      publisher    = {MDPI Basel Switzerland},
      reportid     = {FZJ-2023-04823},
      pages        = {8(1), 25},
      year         = {2023},
      abstract     = {The Jiangmen Underground Neutrino Observatory (JUNO) is a
                      neutrino experiment under construction in an underground
                      laboratory with a 650 m rock overburden near Jiangmen in
                      southern China. The detector’s main component will be 20
                      kton of liquid scintillator held in a spherical acrylic
                      vessel. The experiment is designed for the determination of
                      neutrino mass ordering, one of the key open questions in
                      neutrino physics. This measurement will be based on
                      observations of the vacuum oscillation pattern of
                      antineutrinos from two nuclear power plants at a baseline of
                      53 km. The estimated sensitivity is 3𝜎 in about six years
                      with 26.6 GW$_{\rm th}$ of reactor power. A key ingredient
                      for the success is an excellent and extremely challenging
                      energy resolution of 3\% at 1 MeV. The light produced by the
                      scintillator will be seen by 17,612 large twenty-inch PMTs
                      and 25,600 small three-inch PMTs. The OSIRIS detector will
                      monitor the radio purity of the liquid scintillator during
                      the months-long filling process of the main detector. The
                      unoscillated antineutrino spectrum from one reactor core
                      will be measured with unprecedented precision by the Taishan
                      Antineutrino Observatory (TAO), located at a baseline of
                      about 30 m. JUNO is expected to substantially improve the
                      precision of sin$^2$$2𝜃_{12}$, $Δ𝑚^2_{21}$, and
                      $Δ𝑚^2_{31}$ neutrino oscillation parameters.
                      Astrophysical measurements of solar, geo-, supernova, DSNB,
                      and atmospheric neutrinos, as well as searching for proton
                      decay and dark matter, are integral parts of the vast JUNO
                      physics program. This contribution reviews the physics goals
                      and current status of the JUNO project.},
      month         = {Jul},
      date          = {2022-07-31},
      organization  = {NuFACT 2022, Salt Lake City (USA), 31
                       Jul 2022 - 6 Aug 2022},
      cin          = {IKP-2},
      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)8},
      doi          = {10.3390/psf2023008025},
      url          = {https://juser.fz-juelich.de/record/1018460},
}