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Implications of pulsar timing array data for scalar-induced gravitational waves and primordial black holes: Primordial non-Gaussianity fNL considered

Sai Wang1, Zhi-Chao Zhao2,*, Jun-Peng Li1,3, and Qing-Hua Zhu4

  • 1Theoretical Physics Division, Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, People's Republic of China
  • 2Department of Applied Physics, College of Science, China Agricultural University, Qinghua East Road, Beijing 100083, People's Republic of China
  • 3School of Physical Sciences, University of Chinese Academy of Sciences, Beijing 100049, People's Republic of China
  • 4CAS Key Laboratory of Theoretical Physics, Institute of Theoretical Physics, Chinese Academy of Sciences, Beijing 100190, People's Republic of China

  • *Corresponding author: zhaozc@cau.edu.cn

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