Revision of the energy calibration of the Yakutsk EAS array

Responses of surface and underground scintillation detectors of Yakutsk array are calculated for showers initiated by primary particles with energy E0>=1.0E17 eV within the frameworks of QGSJet01 QGSIIJet-II-04, SIBYLL-2.1 and EPOS-LHC hadron interaction models. A new estimation of E0 is obtained...

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Bibliographic Details
Main Authors: Glushkov, A. V., Pravdin, M. I., Sabourov, A.
Format: Text
Language:unknown
Published: arXiv 2014
Subjects:
High Energy Astrophysical Phenomena astro-ph.HE
FOS Physical sciences
Yakutsk
Online Access:https://dx.doi.org/10.48550/arxiv.1408.6302
https://arxiv.org/abs/1408.6302
Description
Summary:Responses of surface and underground scintillation detectors of Yakutsk array are calculated for showers initiated by primary particles with energy E0>=1.0E17 eV within the frameworks of QGSJet01 QGSIIJet-II-04, SIBYLL-2.1 and EPOS-LHC hadron interaction models. A new estimation of E0 is obtained with the use of various methods. The resulting energy is lower compared to the obtained with earlier method by factor ~1.33. : 15 pages, 5 figures

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