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It is shown that statistical properties of developed hydrodynamic turbulence are characterized by an infinite set of independent anomalous exponents which describes the scaling behavior of hydrodynamic fields constructed from the second and…

chao-dyn · Physics 2008-02-03 Vladimir V. Lebedev , Victor S. L'vov

The development of extensive air showers at extreme energies is studied using a simulation model much simpler and cruder, but also more transparent and flexible, than existing sophisticated codes. Evidence for its satisfactory performance…

High Energy Astrophysical Phenomena · Physics 2015-06-04 Do Thi Hoai , Pham Ngoc Diep , Pierre Darriulat , Pham Tuan Anh , Pham Ngoc Dong , Nguyen Van Hiep , Pham Thi Tuyet Nhung , Nguyen Thi Thao

We have implemented ad-hoc modifications to the CORSIKA Monte-Carlo generator which allow us to simultaneously adjust the multiplicity, elasticity and cross-section of hadronic interactions with respect to the predictions of the Sibyll 2.3d…

High Energy Astrophysical Phenomena · Physics 2023-05-24 Jiri Blazek , Jan Ebr , Jakub Vicha , Tanguy Pierog , Petr Travnicek

The physics content of the QGSJET-III Monte Carlo model of high energy hadronic interactions is briefly described. The predictions of the model for extensive air shower characteristics are presented in comparison to the corresponding…

High Energy Physics - Phenomenology · Physics 2024-11-06 Sergey Ostapchenko

The interpretation of extensive air shower measurements, produced by ultra-high energy cosmic rays, relies on the correct modeling of the hadron-air interactions that occur during the shower development. The majority of hadronic particles…

Nuclear Experiment · Physics 2019-08-14 Alexander E. Hervé

Recently, the energy determination of extensive air showers using radio emission has been shown to be both precise and accurate. In particular, radio detection offers the opportunity for an independent measurement of the absolute energy of…

High Energy Astrophysical Phenomena · Physics 2017-08-17 Marvin Gottowik , Christian Glaser , Tim Huege , Julian Rautenberg

The nature and origin of ultra-high energy (UHE: reffering to > 10^19 eV) cosmic rays are great mysteries in modern astrophysics. The current theories for their explanation include the so-called "top-down" decay scenarios whose main…

Astrophysics · Physics 2009-11-07 H. P. Vankov , N. Inoue , K. Shinozaki

Air-showers measured by the Pierre Auger Observatory were analyzed in order to extract the depth of maximum (Xmax).The results allow the analysis of the Xmax distributions as a function of energy ($> 10^{17.8}$ eV). The Xmax distributions,…

High Energy Astrophysical Phenomena · Physics 2017-01-25 Vitor de Souza

The energy spectrum of muons produced in air showers depends not only on the properties of the primary particle, but also on the atmosphere. This is because of the competition between decay and interaction of the parent mesons, which…

High Energy Astrophysical Phenomena · Physics 2025-09-22 Stef Verpoest , Marisol Catalan Olais , Frank Schroeder

The analysis of high-energy air shower data allows one to study the proton-air cross section at energies beyond the reach of fixed target and collider experiments. The mean depth of the first interaction point and its fluctuations are a…

High Energy Astrophysical Phenomena · Physics 2009-07-22 Ralf Ulrich , Johannes Blümer , Ralph Engel , Fabian Schüssler , Michael Unger

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

The showers of cosmic rays entering the Earth's atmosphere are main sources of information on cosmic rays and are also believed to provide information on elementary interactions at energies not accessible to accelerators. In this context we…

High Energy Physics - Phenomenology · Physics 2009-11-10 M. Rybczynski , Z. Wlodarczyk , O. V. Utyuzh , G. Wilk

The model dependence of the development of extensive air showers generated by high-energy cosmic-ray particles in the atmosphere is studied. The increase of proton-proton and proton-air inelastic cross-sections and values for the elasticity…

Astrophysics · Physics 2008-11-26 Joerg R. Hoerandel

We study the longitudinal development of hadronic showers in water and ice for energies up to 100 EeV. We present results of a hybrid Monte Carlo method developed for the purpose of simulating those showers. We show parameterizations of the…

Astrophysics · Physics 2007-05-23 J. Alvarez-Muñiz , E. Zas

The geometric distribution of high-energy hadrons >100 GeV in shower cores measured with the KASCADE calorimeter is analyzed. The data are checked for sensitivity to hadronic interaction features and indications of new physics as discussed…

High Energy Physics - Phenomenology · Physics 2011-09-01 KASCADE Collaboration , T. Antoni

We present an analysis of the correlation between the depth of the maximum of air-shower profiles and the signal in water-Cherenkov stations in events registered simultaneously by the fluorescence and surface detectors of the Pierre Auger…

High Energy Astrophysical Phenomena · Physics 2025-07-15 Alexey Yushkov

Inclined air showers - those arriving at ground with zenith angle with respect to the vertical theta > 60 deg - are characterised by the dominance of the muonic component at ground which is accompanied by an electromagnetic halo produced…

High Energy Astrophysical Phenomena · Physics 2014-11-20 I. Valino , J. Alvarez-Muniz , M. Roth , R. A. Vazquez , E. Zas

The behavior of a confined spherical symmetric anomalous fluid under high external pressure was studied with Molecular Dynamics simulations. The fluid is modeled by a ore-softened potential with two characteristic length scales, which in…

Soft Condensed Matter · Physics 2014-08-21 José Rafael Bordin , Leandro B. Krott , Marcia C. B. Barbosa

Presently large systematic uncertainties remain in the description of hadronic interactions at ultra-high energies and a fully consistent description of air-shower experimental data is yet to be reached. The amount of data collected by the…

High Energy Astrophysical Phenomena · Physics 2022-10-27 Jakub Vícha

The hadronic interaction model BBL implements the ideas of gluon saturation due to large densities. When approaching the black body limit at high energies, leading partons acquire large transverse momenta which breaks up their coherence.…

Astrophysics · Physics 2007-05-23 H. J. Drescher
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