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April 4, 2026Particles0 citationsOpen Access

Current Status and Future Prospects of the LHCf Experiment

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OAO. AdrianiEBEugenio BertiPBP. Betti

Key Points

  • To investigate the production of neutral particles in high-energy hadronic collisions at the LHC and improve cosmic-ray interaction models.
  • Analyzed data from proton–proton collisions at energies up to 13.6 TeV.
  • Measured forward neutral particles like neutrons, photons, and η mesons.
  • Conducted comparisons between experimental results and predictions of hadronic interaction models.
  • Identified key measurements of forward neutron, photon, and η meson production during Run II at 13 TeV.
  • Provided essential calibration data for extensive air shower simulations initiated by cosmic rays.
  • Planned further analyses using Run III data at 13.6 TeV and in proton-oxygen collisions.

Abstract

The Large Hadron Collider forward (LHCf) experiment studies the production of neutral particles in the very forward region of high-energy hadronic collisions at the LHC. These measurements provide essential calibration data for hadronic interaction models used in simulations of extensive air showers initiated by ultra-high-energy cosmic rays. The LHCf experiment measures forward-produced neutral particles, such as neutrons, photons, π0, and η mesons, which play a key role in the development of extensive air showers. Proton–proton collisions at the LHC reach center-of-mass energies up to 13.6 TeV, corresponding in the fixed-target frame to cosmic-ray interactions at energies close to 1017 eV in the Earth’s atmosphere. LHCf has collected data in proton–proton collisions at several energies, as well as in proton–lead collisions, enabling detailed comparisons between experimental results and predictions of hadronic interaction models. This contribution reviews the most significant LHCf results, with emphasis on Run II proton–proton data at s=13TeV, including measurements of forward neutron, photon, and η meson production. Finally, future prospects are discussed, focusing on ongoing analyses of Run III proton–proton data at s=13.6TeV and on the final LHCf operation in proton-oxygen collisions at sNN=9.6TeV, which best reproduces cosmic-ray interactions with nuclei of the Earth’s atmosphere.

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Cite This Study

Adriani et al. (2026) studied this question.

synapsesocial.com/papers/69d0afb4659487ece0fa5b66https://doi.org/10.3390/particles9020034
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