Sensitivity of the correlation between the depth of shower maximum and the muon shower size to the cosmic ray composition
Patrick Younk, Markus Risse

TL;DR
This study shows that the correlation between the depth of shower maximum and muon shower size can reveal the composition spread of ultra-high energy cosmic rays, aiding in distinguishing between pure and mixed primary beams.
Contribution
It introduces the correlation factor r as a robust observable to infer cosmic ray composition and quantifies the number of events needed for significant differentiation.
Findings
Correlation factor r can measure the spread of primary masses.
Approximately 200 events are needed for significant differentiation.
The method remains effective despite uncertainties in hadronic interaction models.
Abstract
The composition of ultra-high energy cosmic rays is an important issue in astroparticle physics research, and additional experimental results are required for further progress. Here we investigate what can be learned from the statistical correlation factor r between the depth of shower maximum and the muon shower size, when these observables are measured simultaneously for a set of air showers. The correlation factor r contains the lowest-order moment of a two-dimensional distribution taking both observables into account, and it is independent of systematic uncertainties of the absolute scales of the two observables. We find that, assuming realistic measurement uncertainties, the value of r can provide a measure of the spread of masses in the primary beam. Particularly, one can differentiate between a well-mixed composition (i.e., a beam that contains large fractions of both light and…
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