中文

利用望远镜阵列实验对 EeV 中性粒子点源进行北天巡天搜索

高能天体物理现象 2015-05-14 v2

摘要

我们报告了利用望远镜阵列实验的闪烁体表面探测器,在 2008 年 5 月至 2013 年 5 月期间,对北天区约 1018^{18} eV 中性粒子稳态点源进行搜索的结果。我们在北天区 0.5 EeV 以上未发现显著的点源超出。随后,我们还搜索了与 Fermi 明亮银河源的重合情况。在统计不确定性范围内未发现显著重合。因此,我们设定了中子通量的上限,对应于北天区 E>1E>1 EeV 时 95% 置信水平下的平均通量 0.07 km2^{-2} yr1^{-1}。这是在假设点源情况下北天巡天中最严格的通量上限。天鹅座 X-3 (Cygnus X-3) 的中子通量在 95% 置信水平下的上限也被设定为 E>0.5E>0.5 EeV 时 0.2 km2^{-2} yr1^{-1}。这一数值比之前的通量测量值低一个数量级。

关键词

引用

@article{arxiv.1407.6145,
  title  = {A Northern Sky Survey for Point-Like Sources of EeV Neutral Particles with the Telescope Array Experiment},
  author = {R. U. Abbasi and M. Abe and T. Abu-Zayyad and M. Allen and R. Anderson and R. Azuma and E. Barcikowski and J. W. Belz and D. R. Bergman and S. A. Blake and R. Cady and M. J. Chae and B. G. Cheon and J. Chiba and M. Chikawa and W. R. Cho and T. Fujii and M. Fukushima and T. Goto and W. Hanlon and Y. Hayashi and N. Hayashida and K. Hibino and K. Honda and D. Ikeda and N. Inoue and T. Ishii and R. Ishimori and H. Ito and D. Ivanov and C. C. H. Jui and K. Kadota and F. Kakimoto and O. Kalashev and K. Kasahara and H. Kawai and S. Kawakami and S. Kawana and K. Kawata and E. Kido and H. B. Kim and J. H. Kim and J. H. Kim and S. Kitamura and Y. Kitamura and V. Kuzmin and Y. J. Kwon and J. Lan and S. I. Lim and J. P. Lundquist and K. Machida and K. Martens and T. Matsuda and T. Matsuyama and J. N. Matthews and M. Minamino and K. Mukai and I. Myers and K. Nagasawa and S. Nagataki and T. Nakamura and T. Nonaka and A. Nozato and S. Ogio and J. Ogura and M. Ohnishi and H. Ohoka and K. Oki and T. Okuda and M. Ono and A. Oshima and S. Ozawa and I. H. Park and M. S. Pshirkov and D. C. Rodriguez and G. Rubtsov and D. Ryu and H. Sagawa and N. Sakurai and A. L. Sampson and L. M. Scott and P. D. Shah and F. Shibata and T. Shibata and H. Shimodaira and B. K. Shin and J. D. Smith and P. Sokolsky and R. W. Springer and B. T. Stokes and S. R. Stratton and T. A. Stroman and T. Suzawa and M. Takamura and M. Takeda and R. Takeishi and A. Taketa and M. Takita and Y. Tameda and H. Tanaka and K. Tanaka and M. Tanaka and S. B. Thomas and G. B. Thomson and P. Tinyakov and I. Tkachev and H. Tokuno and T. Tomida and S. Troitsky and Y. Tsunesada and K. Tsutsumi and Y. Uchihori and S. Udo and F. Urban and G. Vasiloff and T. Wong and R. Yamane and H. Yamaoka and K. Yamazaki and J. Yang and K. Yashiro and Y. Yoneda and S. Yoshida and H. Yoshii and R. Zollinger and Z. Zundel},
  journal= {arXiv preprint arXiv:1407.6145},
  year   = {2015}
}

备注

27 pages, 10 figures, 3 tables, accepted for publication in the Astrophysical Journal