https://doi.org/10.1051/epjconf/201921002003
Hadronic interaction studied by TA
Institute for Cosmic Ray Research, University of Tokyo, Chiba, Japan
* e-mail: sako@icrr.u-tokyo.ac.jp
Published online: 17 May 2019
Two studies by the Telescope Array group related to the hadronic interaction observed with Extensive Air Showers are reviewed. (1) Inelastic p-air cross section ![$ \sigma _{p - air}^{inel} = 567.0 \pm 70.5\,[{\rm{stat]}}_{ - 25}^{ + 29} [{\rm{sys}}]\,{\rm{mb}} $](/articles/epjconf/abs/2019/15/epjconf_uhecr18_02003/epjconf_uhecr18_02003-eq1.gif)
and total p-p cross section ![$ \sigma _{p - p}^{tot} = 170_{ - 44}^{ + 48} [{\rm{stat}}]_{ - 17}^{ + 19} [{\rm{sys}}]\,{\rm{mb}} $](/articles/epjconf/abs/2019/15/epjconf_uhecr18_02003/epjconf_uhecr18_02003-eq2.gif)
were determined using the 5 years of TA hybrid data with one of the 3 FD stations. These results at the highest energy 
showed good agreements with the extrapolation from the previous measurements and model predictions. (2) The signal sizes of SD were compared between data and MC using 7 years of TA SD data in the energy range from 1018.8 eV to 1019.2 eV. It was found that the data/MC ratios exceed unity and the deviation becomes larger when the expected fraction of muon signal, defined as muon purity P, is higher. The results support the muon excess (with respect to MC) problem reported by the previous observations.
© The Authors, published by EDP Sciences, 2019
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