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First calculated results with the new HIJING++ are presented for identified hadron production in high-energy heavy ion collisions. The recently developed HIJING++ version is based on the latest version of PYTHIA8 and contains all the…

The simulation analysis of the Extensive Air Showers (EAS) was executed by exploring the longitudinal development employing the AIRES system (version 19.04.00) for several hadronic interaction models (SIBYLL, QGSJET, and EPOS) for high…

High Energy Physics - Experiment · Physics 2022-02-21 Kadhom F. Fadhel , A. A. Al-Rubaiee

Extensive Air Showers are still the only source of information on primary cosmic rays and their interactions at energies above PeV. However, this information is hidden inside the multiplicative character of the cascading process. Inspite of…

High Energy Physics - Phenomenology · Physics 2008-11-26 A. D. Erlykin

Current simulations of air showers produced by ultra-high energy cosmic rays (UHECRs) do not satisfactorily describe recent experimental data, particularly when looking at the muonic shower component relative to the electromagnetic one.…

High Energy Astrophysical Phenomena · Physics 2023-09-12 Felix Riehn , Ralph Engel , Anatoli Fedynitch

We report on simulation studies comparing various hadronic shower packages. Results show that predictions from different models vary significantly, illustrating the necessity of testbeam data to resolve the situation.

Instrumentation and Detectors · Physics 2007-05-23 G. Mavromanolakis , D. Ward

Since a number of years the QGSJET model has been successfully used by different groups in the field of high energy cosmic rays. Current work is devoted to the first general update of the model. The key improvement is connected to an…

High Energy Physics - Phenomenology · Physics 2015-06-25 S. Ostapchenko

Hadronic cross sections at ultra-high energy have a significant impact on the development of extensive air shower cascades. Therefore the interpretation of air shower data depends critically on hadronic interaction models that extrapolate…

High Energy Astrophysical Phenomena · Physics 2009-12-08 Ralf Ulrich , Ralph Engel , Steffen Müller , Fabian Schüssler , Michael Unger

The bulk of air showers initiated by very high energy cosmic rays exhibits a longitudinal development in depth with a single well-defined shower maximum. However, a small fraction of showers has a profile that differs considerably from this…

High Energy Astrophysical Phenomena · Physics 2015-06-03 Colin Baus , Ralph Engel , Tanguy Pierog , Ralf Ulrich , Michael Unger

Underlying events dominate most of the hadronic activity in p$-$p collisions and are spanned from perturbative to non-perturbative QCD, having a sensitivity ranging from the multi-scale to very low-x scale physics. A detailed understanding…

High Energy Physics - Phenomenology · Physics 2022-09-07 Krishna Kumar , Sadhana Dash

Monte Carlo Event Generators are tools for simulating outcomes of high-energy collisions and particle production in High Energy Physics (HEP), such as those conducted at the Large Hadron Collider (LHC). Two of the most widely used…

High Energy Physics - Experiment · Physics 2025-11-05 Saliha Bashir , Agnieszka Obłąkowska-Mucha , Gloria Corti

Accurately simulating coupled physical processes under uncertainty is essential for reliable modeling and design in performance-critical applications such as combustion systems. Ablative heat shield design, as a specific example of this…

Computational Physics · Physics 2025-10-07 Diba Behnoudfar , Kyle E. Niemeyer

Recently, with the upgradation of LHC, it is realized that study of heavy-flavored hadrons, namely $\Lambda_{c}^{+}$ and $\rm{D}^{0}$ in hadronic collisions, could reveal the possibility of thermalization of charm quarks. With this…

High Energy Physics - Phenomenology · Physics 2024-12-13 Bhagyarathi Sahoo , Suman Deb , Raghunath Sahoo

The objective of this work is to report on the influence of muon interactions on the development of air showers initiated by astroparticles. We make a comparative study of the different theoretical approaches to muon bremsstrahlung and…

Astrophysics · Physics 2009-10-31 A. N. Cillis , S. J. Sciutto

Recently an essential progress in development of physical models for cosmic ray induced ionization in the atmosphere is achieved. Basically, the models are full target, i.e. based on Monte Carlo simulation of an electromagnetic-muon-nucleon…

High Energy Astrophysical Phenomena · Physics 2014-09-29 A. Mishev , P. I. Y. Velinov

The results of high energy simulated experiments where a given hadronic particle impacts on a given target are statistically analyzed. The energy range of the projectiles goes from below the LHC scale up to the highest cosmic ray energies.…

High Energy Physics - Phenomenology · Physics 2018-10-17 L. Calcagni , C. A. García Canal , S. J. Sciutto , T. Tarutina

We discuss simplified models for photo-meson production in cosmic accelerators, such as Active Galactic Nuclei and Gamma-Ray Bursts. Our self-consistent models are directly based on the underlying physics used in the SOPHIA software, and…

High Energy Astrophysical Phenomena · Physics 2014-11-20 Svenja Hümmer , Michael Rüger , Felix Spanier , Walter Winter

The hardness of the energy spectrum of neutral pions produced in proton-air interactions at ultra-high energies, above $10^{18}$ eV, is constrained by the steepness of the shower-to-shower distribution of the number of muons in…

High Energy Astrophysical Phenomena · Physics 2024-11-26 Lorenzo Cazon , Ruben Conceição , Miguel Alexandre Martins , Felix Riehn

Models with large extra dimensions as well as unparticle models could give rise to new phenomena at collider experiments due to real emission or virtual exchange of gravitons or unparticles. In this paper we present the common…

High Energy Physics - Phenomenology · Physics 2011-03-17 S. Ask , I. V. Akin , L. Benucci , A. De Roeck , M. Goebel , J. Haller

KASCADE-Grande, the extension of the multi-detector setup of KASCADE, was devoted to measure the properties of extensive air showers initiated by high-energy cosmic rays in the primary energy range of 1 PeV up to 1 EeV. The observations of…

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