Attenuation Models for Extensive Air Showers Derived from Simulations
Fiona Ellwanger, Darko Veberi\v{c} (Institute for Astroparticle Physics, Karlsruhe Institute of Technology, Karlsruhe, Germany)

TL;DR
This paper develops and evaluates physics-based models for attenuation effects in extensive air showers caused by cosmic rays, improving energy estimation accuracy across different primary particles and energies.
Contribution
It introduces new functional forms for modeling attenuation in air showers and assesses their effectiveness using Monte Carlo simulations.
Findings
Functional forms accurately describe attenuation effects.
Calibration reduces systematic uncertainties.
Models are applicable across various primary particles.
Abstract
At ultra-high energies, the flux of cosmic rays is too low for direct measurements to be meaningful. When a cosmic ray enters the atmosphere, it initiates an extensive air shower, producing a cascade of secondary particles that propagate toward the ground. Large arrays of surface detectors are used to measure these secondary particles upon arrival. The signal detected at a specific reference distance from the shower core serves as a proxy for the shower size and, consequently, as a reliable estimator of the energy of primary cosmic ray. However, shower development is influenced by attenuation effects: measured signals at the ground depend on the amount of traversed atmospheric density (column density) through which the shower evolves. Since the column density varies with the inclination of the shower, it is important to account for these attenuation effects to ensure accurate energy…
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