EPJ Web Conf.
Volume 210, 2019Ultra High Energy Cosmic Rays 2018 (UHECR 2018)
|Number of page(s)||7|
|Published online||17 May 2019|
Hadronic interaction studied by TA
Institute for Cosmic Ray Research, University of Tokyo, Chiba, Japan
* e-mail: firstname.lastname@example.org
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 and total p-p cross section 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
This is an open access article distributed under the terms of the Creative Commons Attribution License 4.0 (http://creativecommons.org/licenses/by/4.0), which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.