1. Study of muons from ultrahigh energy cosmic ray air showers measured with the Telescope Array experiment
- Author
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S. Kitamura, Hidemi Ito, Kenta Yashiro, Eiji Kido, M. V. Kuznetsov, Kazuhiro Machida, Jyunsei Chiba, Dongsu Ryu, Y. Takagi, Douglas Bergman, Toshiyuki Nonaka, K. Nagasawa, Hideki Tanaka, Elliott Barcikowski, J. H. Kim, T. Goto, G. Furlich, Takaaki Ishii, Y. Omura, Keitaro Fujita, Dmitri Ivanov, Pierre Sokolsky, J. Ogura, Yasunori Saito, B. K. Shin, Igor Tkachev, D. C. Rodriguez, R. Sahara, M. Takeda, Shigehiro Nagataki, Keijiro Mukai, Yuichiro Tameda, John N. Matthews, Akimichi Taketa, Rasha Abbasi, H. Oda, K. Yamazaki, M. Yamamoto, L. M. Scott, Nobuyuki Sakurai, T. Suzawa, Y. Yoneda, N. Inoue, M. Ohnishi, Sergey Troitsky, J. Remington, Y. Hayashi, Inkyu Park, Federico R. Urban, S. Udo, C. C. H. Jui, Isaac Myers, Y. J. Kwon, Hideyuki Ohoka, K. Kawata, Ryota Onogi, Koichi Sekino, A. Di Matteo, K. H. Lee, S. B. Thomas, T.-A. Shibata, Naoaki Hayashida, Takayuki Tomida, Gordon Thomson, T. Matsuyama, S. Ozawa, R. Mayta, Hongsu Kim, Priti Shah, Tom Stroman, Robert Cady, Y. Zhezher, Grigory Rubtsov, Hideaki Shimodaira, Hyoming Jeong, Y. Takahashi, Mai Takamura, K. Kasahara, Y. Uchihori, Shoichi Kishigami, S. Yoshida, Naoto Sakaki, R. Azuma, Masaomi Ono, Tareq Abu-Zayyad, R. Yamane, Kiyoshi Tanaka, Motoki Hayashi, J. P. Lundquist, Shingo Kawana, William Hanlon, M. Allen, H. Kawai, T. Okuda, J. Yang, H. Tokuno, J. D. Smith, Daisuke Ikeda, S. R. Stratton, Tiffany Wong, R. Takeishi, T. Seki, Masaki Fukushima, Masato Takita, K. Martens, K. Tsutsumi, Peter Tinyakov, Samuel Blake, Shoichi Ogio, Zach Zundel, Fumiya Shibata, R. Ishimori, Toshitsugu Fujii, Oleg Kalashev, H. Yamaoka, Michiyuki Chikawa, Ryo Nakamura, Kazuo Saito, H. Yoshii, Heungsu Shin, Toru Nakamura, K. Hibino, Kenichi Kadota, BayarJon Paul Lubsandorzhiev, Mayuko Minamino, K. Honda, Yasunori Kitamura, Masaaki Tanaka, John Belz, Hiroyuki Sagawa, Ben Stokes, B. G. Cheon, S. Kawakami, Maxim Pshirkov, Akitoshi Oshima, Y. Tsunesada, M. Abe, Fumio Kakimoto, Vladim Kuzmin, and S. Jeong
- Subjects
High Energy Astrophysical Phenomena (astro-ph.HE) ,Physics ,Muon ,COSMIC cancer database ,Particle number ,Physics::Instrumentation and Detectors ,010308 nuclear & particles physics ,Astrophysics::High Energy Astrophysical Phenomena ,Monte Carlo method ,Hadron ,FOS: Physical sciences ,Cosmic ray ,01 natural sciences ,law.invention ,Telescope ,Nuclear physics ,Air shower ,13. Climate action ,law ,0103 physical sciences ,High Energy Physics::Experiment ,Astrophysics - High Energy Astrophysical Phenomena ,010306 general physics - Abstract
One of the uncertainties in interpretation of ultra-high energy cosmic ray (UHECR) data comes from the hadronic interaction models used for air shower Monte Carlo (MC) simulations. The number of muons observed at the ground from UHECR-induced air showers is expected to depend upon the hadronic interaction model. One may therefore test the hadronic interaction models by comparing the measured number of muons with the MC prediction. In this paper, we present the results of studies of muon densities in UHE extensive air showers obtained by analyzing the signal of surface detector stations which should have high $\it{muon \, purity}$. The muon purity of a station will depend on both the inclination of the shower and the relative position of the station. In 7 years' data from the Telescope Array experiment, we find that the number of particles observed for signals with an expected muon purity of $\sim$65% at a lateral distance of 2000 m from the shower core is $1.72 \pm 0.10{\rm (stat.)} \pm 0.37 {\rm (syst.)}$ times larger than the MC prediction value using the QGSJET II-03 model for proton-induced showers. A similar effect is also seen in comparisons with other hadronic models such as QGSJET II-04, which shows a $1.67 \pm 0.10 \pm 0.36$ excess. We also studied the dependence of these excesses on lateral distances and found a slower decrease of the lateral distribution of muons in the data as compared to the MC, causing larger discrepancy at larger lateral distances.
- Published
- 2018
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