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Detecting intermediate-mass black holes using miniature pulsar timing arrays in globular clusters

Xian Chen1,2,*, Verónica Vázquez-Aceves2, Siyuan Chen3,4, Kejia Lee1,5,6,7, Yanjun Guo4,5, and Kuo Liu3,4

  • 1Department of Astronomy, School of Physics, Peking University, Beijing 100871, China
  • 2Kavli Institute for Astronomy and Astrophysics at Peking University, Beijing 100871, China
  • 3Shanghai Astronomical Observatory, Chinese Academy of Sciences, 80 Nandan Road, Shanghai 200030, China
  • 4State Key Laboratory of Radio Astronomy and Technology, A20 Datun Road, Chaoyang District, Beijing 100101, China
  • 5National Astronomical Observatories, Chinese Academy of Sciences, A20 Datun Road, Chaoyang District, Beijing 100101, China
  • 6Yunnan Astronomical Observatories, Chinese Academy of Sciences, Kunming 650216, Yunnan, China
  • 7Beijing Laser Acceleration Innovation Center, Huairou, Beijing 101400, China

  • *Contact author: xian.chen@pku.edu.cn

To Understand the Radiative Processes of Pulsars and Fast Radio Bursts with the FAST

Wei-Yang 维扬 Wang 王 et al.

Chinese Phys. Lett. 43 051103 (2026)

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