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A study of analysis method for the identification of UHECR source type

Authors
Yoshida, F.Tameda, Y.Abbasi, R.U.Abu-Zayyad, T.Allen, M.Arai, Y.Arimura, R.Barcikowski, E.Belz, J.W.Bergman, D.R.Blake, S.A.Buckland, I.Cady, R.Cheon, B.G.Chiba, J.Chikawa, M.Fujii, T.Fujisue, K.Fujita, K.Fujiwara, R.Fukushima, M.Fukushima, R.Furlich, G.Gonzalez, R.Hanlon, W.Hayashi, M.Hayashida, N.Hibino, K.Higuchi, R.Honda, K.Ikeda, D.Inadomi, T.Inoue, N.Ishii, T.Ito, H.Ivanov, D.Iwakura, H.Iwasaki, A.Jeong, H.M.Jeong, S.Jui, C.C.H.Kadota, K.Kakimoto, F.Kalashev, O.Kasahara, K.Kasami, S.Kawai, H.Kawakami, S.Kawana, S.Kawata, K.Kharuk, I.Kido, E.Kim, H.B.Kim, J.H.Kim, J.H.Kim, M.H.Kim, S.W.Kimura, Y.Kishigami, S.Kubota, Y.Kurisu, S.Kuzmin, V.Kuznetsov, M.Kwon, Y.J.Lee, K.H.Lubsandorzhiev, B.Lundquist, J.P.Machida, K.Matsumiya, H.Matsuyama, T.Matthews, J.N.Mayta, R.Minamino, M.Mukai, K.Myers, I.Nagataki, S.Nakai, K.Nakamura, R.Nakamura, T.Nakamura, T.Nakamura, Y.Nakazawa, A.Nishio, E.Nonaka, T.Oda, H.Ogio, S.Ohnishi, M.Ohoka, H.Oku, Y.Okuda, T.Omura, Y.Ono, M.Onogi, R.Oshima, A.Ozawa, S.Park, I.H.Potts, M.Pshirkov, M.S.Remington, J.Rodriguez, D.C.Rubtsov, G.I.Ryu, D.Sagawa, H.Sahara, R.Saito, Y.Sakaki, N.Sako, T.Sakurai, N.Sano, K.Sato, K.Seki, T.Sekino, K.Shah, P.D.Shibasaki, Y.Shibata, F.Shibata, N.Shibata, T.Shimodaira, H.Shin, B.K.Shin, H.S.Shinto, D.Smith, J.D.Sokolsky, P.Sone, N.Stokes, B.T.Stroman, T.A.Takagi, Y.Takahashi, Y.Takamura, M.Takeda, M.Takeishi, R.Taketa, A.Takita, M.Tameda, Y.Tanaka, H.Tanaka, K.Tanaka, M.Tanoue, Y.Thomas, S.B.Thomson, G.B.Tinyakov, P.Tkachev, I.Tokuno, H.Tomida, T.Troitsky, S.Tsuda, R.Tsunesada, Y.Uchihori, Y.Udo, S.Uehama, T.Urban, F.Wong, T.Yada, K.Yamamoto, M.Yamazaki, K.Yang, J.Yashiro, K.Yoshida, F.Yoshioka, Y.Zhezher, Y.Zundel, Z.the Telescope Array Collaboration
Issue Date
Mar-2022
Publisher
Sissa Medialab Srl
Citation
Proceedings of Science, v.395, pp.1 - 11
Indexed
SCOPUS
Journal Title
Proceedings of Science
Volume
395
Start Page
1
End Page
11
URI
https://scholarworks.bwise.kr/hanyang/handle/2021.sw.hanyang/182202
ISSN
1824-8039
Abstract
The autocorrelation analysis using the arrival direction of Ultra High Energy Cosmic Rays (UHECRs) has been previously reported by the Telescope Array (TA) experiment. It is expected that the autocorrelation function reflects the source distribution. We simulate the expected arrival direction distribution of the cosmic rays using the catalogs of candidate sources. We take into account random deflection in the magnetic fields, with the magnitude of deflection determined by the charge and energy of the cosmic rays, coherence length and magnitude of the extragalactic magnetic field (EGMF), and by distance to source. In addition, in order to compare with the results of TA, we consider the TA exposure. We compare the autocorrelation of the arrival directions corresponding to different source catalogs with the isotropic distribution. We calculate the autocorrelation function for each type of source candidates using this procedure. We will discuss the ability of this method to identify the source type of UHECRs.
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