Refining the Greisen Profile for Low-Energy Cosmic Gamma-Rays: Quantifying Deviations Across Altitudes and Zenith Angles

Fuente: arXiv
Saved in:
Bibliographic Details
Main Authors: Valdivieso, Constanza, Gutierrez, Bárbara, M, Nicolás Viaux, Mendizabal, Sebastián, R, Raquel Pezoa, Tapia, Sebastián
Format: Preprint
Published: 2025
Subjects:
Online Access:
Tags: Add Tag
No Tags, Be the first to tag this record!
_version_ 1866916054424354816
author Valdivieso, Constanza
Gutierrez, Bárbara
M, Nicolás Viaux
Mendizabal, Sebastián
R, Raquel Pezoa
Tapia, Sebastián
author_facet Valdivieso, Constanza
Gutierrez, Bárbara
M, Nicolás Viaux
Mendizabal, Sebastián
R, Raquel Pezoa
Tapia, Sebastián
contents This study refines the Greisen formalism by comparing the classical Greisen profile and a modified Greisen profile, which incorporates an empirical correction to the shower age parameter with zenith-angle dependence, aiming to better describe low-energy cascades against CORSIKA simulations of cosmic gamma-ray showers (20-800 GeV). Fittings across altitudes of 5000-5900 m and zenith angles from 0 to 40 degrees quantify deviations in particle numbers, showing that the modified profile yields deviations below 4.7%, compared to up to 12.5% for the classical profile. These improvements address low-energy ionization losses, atmospheric density variations, and zenith-angle effects, enhancing accuracy for high-altitude observatories like HAWC and the proposed CONDOR array. The modified profile offers a computationally efficient alternative, providing precise particle number predictions to advance gamma-ray astrophysics and cosmic-ray research.
format Preprint
id arxiv_https___arxiv_org_abs_2509_16847
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle Refining the Greisen Profile for Low-Energy Cosmic Gamma-Rays: Quantifying Deviations Across Altitudes and Zenith Angles
Valdivieso, Constanza
Gutierrez, Bárbara
M, Nicolás Viaux
Mendizabal, Sebastián
R, Raquel Pezoa
Tapia, Sebastián
High Energy Astrophysical Phenomena
High Energy Physics - Phenomenology
This study refines the Greisen formalism by comparing the classical Greisen profile and a modified Greisen profile, which incorporates an empirical correction to the shower age parameter with zenith-angle dependence, aiming to better describe low-energy cascades against CORSIKA simulations of cosmic gamma-ray showers (20-800 GeV). Fittings across altitudes of 5000-5900 m and zenith angles from 0 to 40 degrees quantify deviations in particle numbers, showing that the modified profile yields deviations below 4.7%, compared to up to 12.5% for the classical profile. These improvements address low-energy ionization losses, atmospheric density variations, and zenith-angle effects, enhancing accuracy for high-altitude observatories like HAWC and the proposed CONDOR array. The modified profile offers a computationally efficient alternative, providing precise particle number predictions to advance gamma-ray astrophysics and cosmic-ray research.
title Refining the Greisen Profile for Low-Energy Cosmic Gamma-Rays: Quantifying Deviations Across Altitudes and Zenith Angles
topic High Energy Astrophysical Phenomena
High Energy Physics - Phenomenology
url https://arxiv.org/abs/2509.16847