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Main Authors: Ostapchenko, Sergey, Sigl, Günter
Format: Preprint
Published: 2025
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Online Access:https://arxiv.org/abs/2508.12095
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author Ostapchenko, Sergey
Sigl, Günter
author_facet Ostapchenko, Sergey
Sigl, Günter
contents The treatment of charmed hadron production in the framework of the QGSJET-III Monte Carlo generator is developed, including both perturbative and nonperturbative contributions. For the former, a leading order (LO) perturbative formalism is employed. The so-called $K$-factor designed to take effectively into account higher order corrections, which controls the magnitude of the LO perturbative contribution, is fixed based on a comparison with experimental data on $D$ meson production at the Large Hadron Collider. For the nonperturbative intrinsic charm, a phenomenological Regge-based treatment is developed, with the corresponding normalization being chosen based on measurements of the spectra of $Λ_c$ baryons at large values of Feynman $x$. The model is applied for a calculation of the prompt atmospheric muon neutrino flux in the $10-100$ TeV and $1-10$ PeV energy intervals.
format Preprint
id arxiv_https___arxiv_org_abs_2508_12095
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle Charmed hadron production in the QGSJET-III model: relevance to calculations of the prompt atmospheric neutrino background
Ostapchenko, Sergey
Sigl, Günter
High Energy Physics - Phenomenology
The treatment of charmed hadron production in the framework of the QGSJET-III Monte Carlo generator is developed, including both perturbative and nonperturbative contributions. For the former, a leading order (LO) perturbative formalism is employed. The so-called $K$-factor designed to take effectively into account higher order corrections, which controls the magnitude of the LO perturbative contribution, is fixed based on a comparison with experimental data on $D$ meson production at the Large Hadron Collider. For the nonperturbative intrinsic charm, a phenomenological Regge-based treatment is developed, with the corresponding normalization being chosen based on measurements of the spectra of $Λ_c$ baryons at large values of Feynman $x$. The model is applied for a calculation of the prompt atmospheric muon neutrino flux in the $10-100$ TeV and $1-10$ PeV energy intervals.
title Charmed hadron production in the QGSJET-III model: relevance to calculations of the prompt atmospheric neutrino background
topic High Energy Physics - Phenomenology
url https://arxiv.org/abs/2508.12095