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

  • Yoshida, F.
  • Tameda, Y.
  • Abbasi, R.U.
  • Abu-Zayyad, T.
  • Allen, M.
  • ... Cheon, B.G.
  • 외 156명
Citations

SCOPUS

0

초록

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.

키워드

AutocorrelationCosmologyMagnetic fieldsCosmic raysAnalysis methodArrival directionAutocorrelation analysisAutocorrelation functionsCosmic ray sourcesDirection distributionSource distributionSource typesTelescope arraysUltra high-energy cosmic rays
제목
A study of analysis method for the identification of UHECR source type
저자
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
발행일
2022-03
유형
Conference Paper
저널명
Proceedings of Science
395
페이지
1 ~ 11