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

TL;DR

This paper addresses the muon deficit in ultrahigh-energy cosmic ray air showers by proposing a strangeness production enhancement mechanism, and discusses how future LHC neutrino detectors can help refine the models.

Contribution

It introduces a toy model with a $_s$ parameter to explain the muon puzzle and explores how upcoming experiments can test this model.

Findings

The $_s$ swap impacts shower development and can fit UHECR data.

FASER$ u$ and Forward Physics Facility experiments can probe the $_s$ parameter space.

The model provides a potential solution to the muon deficit problem.

Abstract

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.