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@INPROCEEDINGS{Penek:890009,
      author       = {Penek, Ömer and et al. {Borexino Collaboration}},
      title        = {{B}orexino {S}ensitivity {S}tudies towards {D}etection of
                      {S}olar {N}eutrinos from the {CNO} {F}usion {C}ycle},
      school       = {RWTH Aachen},
      reportid     = {FZJ-2021-00603},
      year         = {2020},
      abstract     = {The Borexino detector, located at the Laboratori Nazionali
                      del Gran Sasso in Italy, is a liquid scintillator detector
                      with a primary goal to measure solar neutrinos. The *pp*
                      fusion chain has been measured in Borexino with an
                      outstanding precision through the detection of *pp*, *pep*,
                      $^{7}$Be, and $^{8}$B neutrinos. It is well motivated by
                      standard solar models that around 1 per cent of the solar
                      energy is fueled by the so-called Carbon-Nitrogen-Oxygen
                      (CNO) cycle. A direct measurement of the CNO cycle is
                      difficult due to the high spectral correlation with the
                      background isotope $^{210}$Bi and *pep* neutrinos. The
                      sensitivity to CNO neutrinos was evaluated through a
                      likelihood-ratio test, based on thousands of
                      pseudo-experiments analyzed with a counting analysis as well
                      as spectral fit. This poster presents the resulting
                      discovery potential of Borexino towards the CNO cycle in the
                      Sun.},
      month         = {Jun},
      date          = {2020-06-22},
      organization  = {The XXIX International Conference on
                       Neutrino Physics and Astrophysics,
                       Chicago (USA), 22 Jun 2020 - 2 Jul
                       2020},
      subtyp        = {Other},
      cin          = {IKP-2},
      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)24},
      doi          = {10.5281/ZENODO.4401808},
      url          = {https://juser.fz-juelich.de/record/890009},
}