Whereas muon in extensive air shower is an observable sensitive to the primary composition and to the hadron interaction properties, the discrepancy between measured and estimated values has not been solved.
Using the new data of forward hadron from an accelerator experiment, a hadron interaction model (QGSJET II-04) is modified.
Air shower simulated with the modified interaction model develops quickly and produces more muons.
But these changes are not enough to solve the discrepancy.
Volume 301 -
35th International Cosmic Ray Conference (ICRC2017) -
Session Cosmic-Ray Indirect. CRI- hadronic interactions/EAS development
Influence of forward hadron production on the development of extensive air shower
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Pre-published on:
August 16, 2017
Published on:
August 03, 2018
Abstract
DOI: https://doi.org/10.22323/1.301.0306
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Copyright owned by the author(s) under the term of the Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License.