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

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

Measuring the anisotropies in astrophysical and cosmological gravitational-wave backgrounds with Taiji and LISA networks

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Split Majoron model confronts the NANOGrav signal and cosmological tensions

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Complete analysis of the background and anisotropies of scalar-induced gravitational waves: primordial non-Gaussianity f NL and g NL considered

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Induced gravitational wave interpretation of PTA data: a complete study for general equation of state

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Constraints on non-Gaussian primordial curvature perturbation from the LIGO-Virgo-KAGRA third observing run

Angular bispectrum and trispectrum of scalar-induced gravitational waves: all contributions from primordial non-Gaussianity fNLand gNL

Detecting a gravitational wave background from inflation with null energy condition violation: prospects for Taiji

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