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

collaborators

19 papers

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…

nucl-th2026

Trace anomaly and isospin splitting in inverse-mapped relativistic mean-field theory

Wen-Jie Xie, Jun-Hua Guo

Trace anomaly and sound speed provide EOS-level probes of dense-matter nonconformality, but do not by themselves identify the microscopic channels responsible for the response. We…

nucl-th2026

Finite-nucleus-protected high-density extension of covariant density functionals constrained by multimessenger data

Wen-Jie Xie, Jun-Hua Guo

We construct a finite-nucleus-protected high-density extension of covariant density functionals by modifying only the isoscalar-vector channel outside the finite-nucleus calibratio…

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…

nucl-th2025★ 5 cited

Evolutions of in-medium baryon-baryon scattering cross sections and stiffness of dense nuclear matter from Bayesian analyses of FOPI proton flow excitation functions

Bao-An Li, Wen-Jie Xie

Within a Bayesian statistical framework using a Gaussian Process (GP) emulator for an isospin-dependent Boltzmann-Uehling-Uhlenbeck (IBUU) transport model simulator of heavy-ion re…

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…