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@ARTICLE{Kampmann:888818,
      author       = {Kampmann, Philipp and Cheng, Yaping and Ludhova, Livia},
      title        = {{A} semi-analytical energy response model for low-energy
                      events in {JUNO}},
      journal      = {Journal of Instrumentation},
      volume       = {15},
      number       = {10},
      issn         = {1748-0221},
      address      = {London},
      publisher    = {Inst. of Physics},
      reportid     = {FZJ-2020-05232},
      pages        = {P10007 - P10007},
      year         = {2020},
      abstract     = {The Jiangmen Underground Neutrino Observatory (JUNO) is a
                      next-generation neutrino experiment under construction in
                      China expected to be completed in 2022. As the main goal it
                      aims to determine the neutrino mass ordering with 3–4 σ
                      significance using a 20 kton liquid scintillator detector.
                      It will measure the oscillated energy spectrum of electron
                      anti-neutrinos from two nuclear power plants at about 53 km
                      baseline with an unprecedented energy resolution of $3\%$ at
                      1 MeV . A requirement of the JUNO experiment is the
                      knowledge of the energy non-linearity of the detector with a
                      sub-percent precision. As the light yield of the liquid
                      scintillator is not fully linear to the energy of the
                      detected particle and dependent on the particle type, a
                      model for this light yield is presented in this paper. Based
                      on an energy non-linearity model of electrons, this article
                      provides the conversion to the more complex energy response
                      of positrons and gammas. This conversion uses a fast and
                      simple algorithm to calculate the spectrum of secondary
                      electrons generated by a gamma, which is introduced here and
                      made open access to potential users. It is also discussed
                      how the positron non-linearity can be obtained from the
                      detector calibration with gamma sources using the results
                      presented in this article.},
      cin          = {IKP-2},
      ddc          = {610},
      cid          = {I:(DE-Juel1)IKP-2-20111104},
      pnm          = {612 - Cosmic Matter in the Laboratory (POF3-612)},
      pid          = {G:(DE-HGF)POF3-612},
      typ          = {PUB:(DE-HGF)16},
      UT           = {WOS:000577278000007},
      doi          = {10.1088/1748-0221/15/10/P10007},
      url          = {https://juser.fz-juelich.de/record/888818},
}