QGSjet II and EPOS hadronic interaction models: comparison with the Yakutsk EAS array data-Reference-Cited by-同舟云学术

QGSjet II and EPOS hadronic interaction models: comparison with the Yakutsk EAS array data

Published:2009-12 Issue: Volume:196 Page:319-322
ISSN:0920-5632
Container-title:Nuclear Physics B - Proceedings Supplements
language:en
Short-container-title:Nuclear Physics B - Proceedings Supplements

Author:

Knurenko S.P.,Sabourov A.V.

Publisher

Elsevier BV

Subject

Nuclear and High Energy Physics,Atomic and Molecular Physics, and Optics

Reference11 articles.

1. Hadron interactions in cosmic rays at energies above the accelerator range

2. Problemy fiziki kosmicheskih luchei;Khristiansen,1987

3. M. N. Dyakonov, V. P. Egorova, S. P. Knurenko et al. Shirokie atmosfernye livni s energiei vyshe 1017 eV. Yakutsk: YaF SO AN SSSR. pp. 29–56. (in Russian)

4. On total inelastic cross sections and the average depth of the maximum of extensive air showers

5. Characteristics of EAS and primary particle mass composition in the energy region of 1017–3⋅1019 eV by Yakutsk data

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2. Search for ultra-high energy photons by complex data of the Yakutsk array;EPJ Web of Conferences;2019

3. Estimate of the Integral Photon Flux in the Region of Extremely High Energies in Complex Yakutsk EAS Array Data;JETP Letters;2018-06

4. Response time structure of electrons and muons recorded by scintillation detectors in showers with energies higher than 5 × 1018 eV at the Yakutsk EAS array: The search for neutrinos;Bulletin of the Russian Academy of Sciences: Physics;2017-04

5. Search for neutrino generated air shower candidates with energy ≥ 1019 eV and Zenith angle θ;EPJ Web of Conferences;2017