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@ARTICLE{Ariga:640487,
      author       = {Ariga, Akitaka and Barwick, Steven and Boyd, Jamie and
                      Fieg, Max and Kling, Felix and Mäkelä, Toni and Vendeuvre,
                      Camille and Weyer, Benjamin},
      title        = {{D}etecting {LHC} neutrinos at surface level},
      journal      = {Journal of high energy physics},
      volume       = {2025},
      number       = {7},
      issn         = {1126-6708},
      address      = {Heidelberg},
      publisher    = {Springer},
      reportid     = {PUBDB-2025-04809, arXiv:2501.06142},
      pages        = {270},
      year         = {2025},
      note         = {cc-by},
      abstract     = {The first direct detection of neutrinos at the LHC not only
                      marks the beginning of a novel collider neutrino program at
                      CERN but also motivates considering additional neutrino
                      detectors to fully exploit the associated physics potential.
                      As the existing forward neutrino detectors are located
                      underground, it is interesting to investigate the
                      feasibility and physics potential of neutrino experiments
                      located at the surface-level. A topographic desk study is
                      performed to identify all points at which the LHC’s
                      neutrino beams exit the earth. The closest location lies
                      about 9 km east of the CMS interaction point, at the bottom
                      of Lake Geneva. Several detectors to be placed at this
                      location are considered, including a water Cherenkov
                      detector and an emulsion detector. The detector designs are
                      outlined at a conceptual level, and projections for their
                      contribution to the LHC forward neutrino program and
                      searches for dark sector particles are presented. However,
                      the dilution of the neutrino flux over distance reduces the
                      neutrino yield significantly, necessitating large and coarse
                      detector designs. We identify the experimental challenges to
                      be overcome by future research, and conclude that at present
                      the physics potential of surface-level detectors is limited
                      in comparison to ones closer to the interaction point,
                      including the proposed Forward Physics Facility.},
      keywords     = {Fixed Target Experiments (autogen) / Forward Physics
                      (autogen) / Electroweak Interaction (autogen) / Dark Matter
                      (autogen)},
      cin          = {T},
      ddc          = {530},
      cid          = {I:(DE-H253)T-20120731},
      pnm          = {611 - Fundamental Particles and Forces (POF4-611) / DFG
                      project G:(GEPRIS)390833306 - EXC 2121: Quantum Universe
                      (390833306) / FASERnu - Studying Neutrinos at the High
                      Energy Frontier (101002690)},
      pid          = {G:(DE-HGF)POF4-611 / G:(GEPRIS)390833306 /
                      G:(EU-Grant)101002690},
      experiment   = {EXP:(DE-MLZ)NOSPEC-20140101},
      typ          = {PUB:(DE-HGF)16},
      eprint       = {2501.06142},
      howpublished = {arXiv:2501.06142},
      archivePrefix = {arXiv},
      SLACcitation = {$\%\%CITATION$ = $arXiv:2501.06142;\%\%$},
      doi          = {10.1007/JHEP07(2025)270},
      url          = {https://bib-pubdb1.desy.de/record/640487},
}