Update on testing of air-shower modelling using combined data of the Pierre Auger Observatory and phenomenological consequences
Jakub V\'icha (for the Pierre Auger Collaboration)

TL;DR
This paper evaluates current air-shower models using Pierre Auger Observatory data, revealing significant discrepancies in predictions of shower depth and muon content, and discusses implications for cosmic ray composition and model adjustments.
Contribution
It provides updated constraints on hadronic interaction models by analyzing combined fluorescence and surface detector data, highlighting the need for model modifications.
Findings
Models cannot accurately predict $X_{max}$ and ground signals at >5σ level.
Deeper $X_{max}$ scales suggest a heavier cosmic ray composition.
Phenomenological implications for energy spectrum and muon discrepancy are discussed.
Abstract
The combined data of Fluorescence and Surface Detectors of the Pierre Auger Observatory has recently provided the strongest constraints on the validity of predictions from current models of hadronic interactions. The unmodified predictions of these models on the depth of shower maximum () and the hadronic part of the ground signal are unable to accurately describe the measured data at a level of more than 5 in the energy range 3-10 EeV. This inconsistency has been shown to originate not only from the predicted amount of muons at the ground level, but also from the predicted scale of , which must be adjusted to better match the observed data. The resulting deeper scales of the models imply a heavier mass composition to be interpreted from the measurements. We show the results of the test with an updated data set of the…
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Taxonomy
TopicsAstrophysics and Cosmic Phenomena · Insects and Parasite Interactions · Particle Detector Development and Performance
