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From the 1 of 7 linked papers with an AI index.

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7 papers

astro-ph.CO2026

Probing Graviton Mass with MeerKAT PTA and SKA--PTA Forecasts

Zhi-Chao Zhao, Sai Wang

The paper uses data from the MeerKAT pulsar timing array to set upper limits on the graviton mass and forecasts that the upcoming SKA pulsar timing array could improve these limits…

astro-ph.CO2026

Constraints on the Sum of Neutrino Masses from ACT DR6 and DESI DR2 Considering Isocurvature Initial Conditions

Hongsheng Hou, Sai Wang, Zhi-Chao Zhao +1

We present a robust assessment of cosmological constraints on the sum of neutrino masses () when relaxing the standard assumption of purely adiabatic primordial initial…

astro-ph.CO2026

Reassessing the SIGW Interpretation of PTA Signal: The Role of Third-Order Gravitational Waves and Implications for the PBH Overproduction

Zhi-Chao Zhao, Sai Wang, Qing-Hua Zhu +1

In light of recent interpretations attributing pulsar timing array (PTA) signal to second-order gravitational waves induced by linear cosmological curvature perturbations in the ea…

gr-qc2026

Fundamental Physics and Cosmology with TianQin

Jun Luo, Haipeng An, Ligong Bian +33

The exploration of the surrounding world and the universe is an important theme in the legacy of humankind. The detection of gravitational waves is adding a new dimension to this g…

astro-ph.CO2026

Isotropy, anisotropies and non-Gaussianity in the scalar-induced gravitational-wave background: diagrammatic approach for primordial non-Gaussianity up to arbitrary order

Jun-Peng Li, Sai Wang, Zhi-Chao Zhao +1

Produced nonlinearly by the enhanced linear cosmological curvature perturbations, the scalar-induced gravitational waves (SIGWs) can serve as a potentially powerful probe of primor…

astro-ph.CO2025

Constraints on the lepton asymmetry from DESI DR2 BAO data

Zhi-Chao Zhao, Dong-Mei Xia, Sai Wang

It is important to explore the potential existence of lepton asymmetry in the neutrino sector. Conducting a joint analysis of DESI DR2 BAO data and \emph{Planck} 2018 CMB data, we…