Reinterpreting the development of extensive air showers initiated by nuclei and photons
Manlio De Domenico, Mariangela Settimo, Simone Riggi, Eric Bertin

TL;DR
This paper introduces an empirical model using the generalized Gumbel distribution to describe the $ ext{X}_{ ext{max}}$ distribution in extensive air showers caused by nuclei and photons at ultra-high energies, aiding cosmic ray composition analysis.
Contribution
The paper presents a novel analytical model for $ ext{X}_{ ext{max}}$ distribution in EAS, incorporating the impact of hadronic interaction models and extending to ultra-high energies.
Findings
The model accurately describes $ ext{X}_{ ext{max}}$ distributions across a wide energy range.
It highlights the influence of hadronic interaction models on $ ext{X}_{ ext{max}}$ predictions.
Application to experimental data demonstrates the model's utility in cosmic ray studies.
Abstract
Ultra-high energy cosmic rays (UHECRs) interacting with the atmosphere generate extensive air showers (EAS) of secondary particles. The depth corresponding to the maximum development of the shower, , is a well-known observable for determining the nature of the primary cosmic ray which initiated the cascade process. In this paper, we present an empirical model to describe the distribution of for EAS initiated by nuclei, in the energy range from eV up to eV, and by photons, in the energy range from eV up to eV. Our model adopts the generalized Gumbel distribution motivated by the relationship between the generalized Gumbel statistics and the distribution of the sum of non-identically distributed variables in dissipative stochastic systems. We provide an analytical expression for describing the distribution for photons and…
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