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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

Can we distinguish between adiabatic and isocurvature fluctuations with pulsar timing arrays?

Dark matter spike surrounding supermassive black holes binary and the nanohertz stochastic gravitational wave background

Cosmological constraints on small-scale primordial non-Gaussianity

Bayesian reconstruction of primordial perturbations from induced gravitational waves

Reconstructing primordial black hole power spectra from gravitational waves

Stochastic axionlike curvaton: Non-Gaussianity and primordial black holes without a large power spectrum

Induced gravitational waves for arbitrary higher orders: Vertex rules and loop diagrams in cosmological perturbation theory

Implications for the non-Gaussianity of primordial gravitational waves from pulsar timing arrays

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Quest for CMB spectral distortions to probe the scalar-induced gravitational wave background interpretation of pulsar timing array data

Constraining inflation with nonminimal derivative coupling with the Parkes Pulsar Timing Array third data release

Primordial black holes and their gravitational-wave signatures

Constraints on the inflaton potential from scalar-induced gravitational waves and primordial black holes

Implications of Pulsar Timing Arrays for Gauss-Bonnet inflation

Enhanced induced gravitational waves in Horndeski gravity

Estimating the gravitational wave background anisotropy: a Bayesian approach boosted by cross-correlation angular power spectrum

Loops in inflation with strongly non-geodesic motion

Can tensor-scalar induced GWs dominate PTA observations?

Isotropic background and anisotropies of gravitational waves induced by cosmological soliton isocurvature perturbations

Charting the nanohertz gravitational wave sky with pulsar timing arrays

Primordial black hole formation from the upward step model: Avoiding overproduction

Study of primordial non-Gaussianity $$f_{\textrm{NL}}$$ and $$g_{\textrm{NL}}$$ with the cross-correlations between the scalar-induced gravitational waves and the cosmic microwave background

Primordial black holes from effective field theory of stochastic single field inflation at NNNLO

Constraining string cosmology with the gravitational-wave background using the NANOGrav 15-year data set

The Pulsar Timing Array Signal from Infrared Regions of Scalar-Induced Gravitational Waves

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