210 citations
- East Texas A&M UniversityUS14 papers
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- Xinjiang Astronomical ObservatoryCN8 papers
- Guangxi Normal UniversityCN6 papers
- Guangzhou UniversityCN6 papers
- Beijing Normal UniversityCN4 papers
- Institute of Modern PhysicsCN4 papers
- Shanghai Institute of Applied PhysicsCN4 papers
- Southeast UniversityCN4 papers
- Sun Yat-sen UniversityCN4 papers
- Texas A&M UniversityUS4 papers
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33 papers
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…
Bayesian constraints on quark stars from multi-messenger observations
Wen-Jie Xie, Cheng-Jun Xia, Chen Zhang +1
We perform a systematic Bayesian analysis of quark star equations of state under current multimessenger constraints, investigating the impact of prior assumptions and extreme-mass…
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…
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…
Bayesian inference of nuclear incompressibility from collective flow in mid-central Au+Au collisions at 400--1500 MeV/nucleon
J. M. Wang, X. G. Deng, W. J. Xie +2
The incompressibility of symmetric nuclear matter (SNM) is determined through a Bayesian analysis of collective flow data from Au + Au collisions at beam energies $E = 400 -150…
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 $^{…