Ultra-high-energy hadronic physics at the Pierre Auger Observatory: muon measurements

TL;DR

This paper discusses measurements of muons in ultra-high-energy cosmic ray air showers at the Pierre Auger Observatory, revealing discrepancies between observed data and simulation predictions, and exploring the implications for hadronic interaction models.

Contribution

It presents a comprehensive analysis of muon measurements and model-data discrepancies, incorporating hybrid detection methods and recent upgrades to the Observatory.

Findings

Discrepancy between muon counts in data and simulations.

Complex disagreement involving shower maximum depths.

Good agreement in shower-to-shower fluctuations.

Abstract

The Pierre Auger Observatory, the world's largest observatory of ultra-high-energy cosmic rays (UHECR), offers a unique insight into the properties of hadronic interactions occurring in air showers at energies well above those reached at human-made accelerators. The key probe into the hadronic interactions has, for a long time, been the number of muons arriving at the ground, which can be directly measured at Auger for energies up to 10 EeV using dedicated underground muon detectors or estimated through the observation of highly inclined showers using the surface detector of the Observatory. Further information can be obtained using the hybrid character of the Observatory, which allows the simultaneous observation of the longitudinal development of the shower with the fluorescence (and lately also radio) detector and the ground signal with the surface detector. Several different analyses using hybrid data show a discrepancy between the predictions of simulations based on the latest hadronic interaction models and data. This discrepancy has been long interpreted as a deficit in the number of muons predicted by the simulations with respect to the data. A new analysis using a global fit of the data on selected hybrid showers has shown that the disagreement between models and data is more complex and also involves the predictions for the depths of the maxima of the longitudinal shower development. At the same time, measurements of shower-to-shower fluctuations using inclined hybrid events show good agreement with the predictions, suggesting that the observed muon discrepancy is rather the result of a gradual accumulation of small changes during the shower development than of a major change in the properties of the first interaction. Recently, the Observatory has undergone an upgrade, which includes several components aimed at a significant improvement ...