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Astroparticle Physics with the Forward Physics Facility at the High-Luminosity LHC

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arxiv 2308.09079 v1 pith:5WJ2WVTP submitted 2023-08-17 hep-ex astro-ph.HE

classification hep-exastro-ph.HE
keywords physicswillhigh-energyastroparticleexperimentsforwardatmospherecollisions
verification ladder T0 review T1 audit T2 compute T3 formal
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High-energy collisions at the High-Luminosity Large Hadron Collider (HL-LHC) will produce an enormous flux of particles along the beam collision axis that is not accessible by existing LHC experiments. Multi-particle production in the far-forward region is of particular interest for astroparticle physics. High-energy cosmic rays produce large particle cascades in the atmosphere, extensive air showers (EAS), which are driven by hadron-ion collisions under low momentum transfer in the non-perturbative regime of QCD. Thus, the understanding of high-energy hadronic interactions in the forward region is crucial for the interpretation of EAS data and for the estimation of backgrounds for searches of astrophysical neutrinos. The Forward Physics Facility (FPF) is a proposal to build a new underground cavern at the HL-LHC which will host a variety of far-forward experiments to detect particles outside the acceptance of the existing LHC experiments. We will present the current status of plans for the FPF and highlight the synergies with astroparticle physics. In particular, we will discuss how measurements at the FPF will improve the modeling of high-energy hadronic interactions in the atmosphere and thereby reduce the associated uncertainties of measurements in the context of multi-messenger astrophysics.

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Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. The Forward Physics Facility at the HL-LHC and its Synergies with Astroparticle Physics

    astro-ph.HE 2024-12 unverdicted novelty 2.0 of 10

    A proceedings review of the Forward Physics Facility, arguing that its planned far-forward hadron and neutrino measurements would reduce model uncertainties in ultra-high-energy cosmic-ray and neutrino astrophysics.

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