activity
20162026
most citedProgress in Constraining Nuclear Symmetry Energy Using Neutron Star Observables Since GW170817

210 citations · 384 across the 11 of their papers we have counts for

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Showing astro-ph.HEShow all

6 papers · 1 filter

astro-ph.HE2026

Bayesian Inference of fine-features of dense matter EOS from future high-precision data of neutron star radii

Bao-An Li, Xavier Grundler, Wen-Jie Xie +1

Future high-precision X-ray and gravitational wave observatories are expected to measure the radii of neutron stars (NSs) with an accuracy better than about 0.1 km. However, it rem…

astro-ph.HE2025★ 4 cited

Bayesian Inference of Hybrid Star Properties from Future High-Precision Measurements of Their Radii

Bao-An Li, Xavier Grundler, Wen-Jie Xie +1

Future high-precision X-ray and gravitational-wave observations of neutron stars (NSs) are expected to constrain NS radii with uncertainties as small as ~km. Such unpr…

astro-ph.HE2024★ 20 cited

Bayesian Inference of Fine-Features of Nuclear Equation of State from Future Neutron Star Radius Measurements to 0.1km Accuracy

Bao-An Li, Xavier Grundler, Wen-Jie Xie +1

To more precisely constrain the Equation of State (EOS) of supradense neutron-rich nuclear matter, future high-precision X-ray and gravitational wave observatories are proposed to…

astro-ph.HE2024★ 18 cited

Impact of The Newly Revised Gravitational Redshift of X-ray Burster GS 1826-24 on The Equation of State of Supradense Neutron-Rich Matter

Wen-Jie Xie, Bao-An Li, Nai-Bo Zhang

Thanks to the recent advancement in producing rare isotopes and measuring their masses with unprecedented precision, the updated nuclear masses around the waiting-point nucleus $^{…

astro-ph.HE2020★ 89 cited

Bayesian Inference of the Symmetry Energy of Super-Dense Neutron-Rich Matter from Future Radius Measurements of Massive Neutron Stars

Wen-Jie Xie, Bao-An Li

Using an explicitly isospin-dependent parametric Equation of State (EOS) for the core of neutron stars (NSs) within the Bayesian statistical approach, we infer the EOS parameters o…

astro-ph.HE2019

Bayesian Inference of High-density Nuclear Symmetry Energy from Radii of Canonical Neutron Stars

Wen-Jie Xie, Bao-An Li

The radius of neutron stars (NSs) with a mass of 1.4 M has been extracted consistently in many recent studies in the literature. Using representative …