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Sai Wang ¹, Zhi-Chao Zhao ^2,*, Jun-Peng Li^1,3, 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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Articles Citing

Implications of pulsar timing array data for scalar-induced gravitational waves and primordial black holes: Primordial non-Gaussianity $f_{N L}$ considered

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Nanohertz Gravitational Waves

Constraints on holographic QCD phase transitions from PTA observations

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