An explanation of the muon puzzle of ultrahigh-energy cosmic rays and the role of the Forward Physics Facility for model improvement

• DOI: 10.1016/j.jheap.2022.03.004
• Publication Date: 2022-03-25T16:15:36Z
• Authors: Luis A. Anchordoqui; Carlos García Canal; Felix Kling; Sergio J. Sciutto; Jorge F. Soriano
• Keywords: air; toy model; FOS: Physical sciences; anomaly; model: phase space; 01 natural sciences; High Energy Physics - Phenomenology (hep-ph); ALICE; muon; 0103 physical sciences; hadron hadron, interaction; cosmic radiation: UHE; info:eu-repo/classification/ddc/530; hadron hadron: interaction; showers, atmosphere; showers: atmosphere; model, phase space; cosmic radiation, UHE; parametrization; sensitivity; strangeness, production; High Energy Physics - Phenomenology; neutrino: detector; CERN LHC Coll; rapidity; strangeness, enhancement; strangeness: production; strangeness: enhancement; neutrino, detector

We investigate the observed muon deficit in air shower simulations when compared to ultrahigh-energy cosmic ray (UHECR) data. Based upon the observed enhancement of strangeness production in high-energy hadronic collisions reported by the ALICE Collaboration, the concomitant $\pi \leftrightarrow K$ swap is considered as the keystone to resolve the muon anomaly through its corresponding impact on the shower development. We construct a toy model in terms of the $\pi \leftrightarrow K$ swapping probability $F_s$. We present a parametrization of $F_s$ in terms of the pseudorapidity that can accommodate the UHECR data. Looking to the future, we explore potential strategies for model improvement using the massive amounts of data to be collected by LHC neutrino detectors, such as FASER$\nu$ and experiments at the Forward Physics Facility. We calculate the corresponding sensitivity to $F_s$ and show that these experiments will be able to probe the model phase space.