55 citations · 303 across the 12 of their papers we have counts for
12 papers
Properties of rapidly rotating hot neutron stars within Brueckner theory
Hong-Ming Liu, Bo-Xiu Zhou, Zeng-Hua Li +2
We study the properties of hot rapidly rotating neutron stars using various equations of state based on the Brueckner-Hartree-Fock approach at finite temperature. The temperature d…
Dark matter effects on the properties of quark stars and the implications for the peculiar objects
Hong-Ming Liu, Peng-Cheng Chu, He Liu +2
We systematically investigate the observable properties of dark matter-admixed quark stars (DQSs) using the confined-isospin-density-dependent-mass model in combination with the ge…
Dark matter effects on the properties of neutron stars: compactness and tidal deformability
Hong-Ming Liu, Jin-Biao Wei, Zeng-Hua Li +3
We systematically study the observable properties of dark-matter admixed neutron stars, employing a realistic nuclear EOS in combination with self-interacting fermionic dark matter…
Dark matter effects on the properties of neutron stars: optical radii
Hong-Ming Liu, Jin-Biao Wei, Zeng-Hua Li +2
We study the effects of dark matter on the properties of neutron stars by employing a DM-admixed model. The Brueckner-Hartree-Fock theory with realistic three-body forces and a gen…
Microscopic nuclear equation of state at finite temperature and stellar stability
Hong-Ming Liu, Jing Zhang, Zeng-Hua Li +3
A microscopic nuclear equation of state compatible with all current astrophysical constraints constructed within the Brueckner-Hartree-Fock formalism is presented and extended in a…
Binary neutron star merger simulations with hot microscopic equations of state
A. Figura, F. Li, J. -J. Lu +3
We perform binary neutron star merger simulations using a newly derived set of finite-temperature equations of state in the Brueckner-Hartree-Fock approach. We point out the import…
Accurate nuclear symmetry energy at finite temperature within a BHF approach
Jia-Jing Lu, Fan Li, Zeng-Hua Li +3
We compute the free energy of asymmetric nuclear matter in a Brueckner-Hartree-Fock approach at finite temperature, paying particular attention to the dependence on isospin asymmet…
Hybrid equation of state approach in binary neutron-star merger simulations
A. Figura, J. -J. Lu, G. F. Burgio +2
We investigate the use of hybrid equations of state in binary neutron-star simulations in full general relativity, where thermal effects are included in an approximate way through…
Hot neutron stars with microscopic equations of state
Jia-Jing Lu, Zeng-Hua Li, G. F. Burgio +1
We study the properties of hot beta-stable nuclear matter using equations of state derived within the Brueckner-Hartree-Fock approach at finite temperature including consistent thr…
Are nuclear matter properties correlated to neutron star observables ?
Jin-Biao Wei, Jia-Jing Lu, G. F. Burgio +2
We investigate properties of nuclear matter and examine possible correlations with neutron star observables for a set of microscopic nuclear equations of state derived within the B…
Nuclear symmetry potential in the relativistic impulse approximation
Zeng-Hua Li, Lie-Wen Chen, Che Ming Ko +2
Using the relativistic impulse approximation with the Love-Franey \textsl{NN} scattering amplitude developed by Murdock and Horowitz, we investigate the low-energy (100 MeV$\leq E_…
Probing the Isospin Dependent In-Medium Nucleon-Nucleon Cross Section by Nucleon Emissions
Jian-Ye Liu, Wen-Jun Guo, Yong-Zhong Xing +3
The effects of the symmetry potential and the isospin dependent in-medium nucleon-nucleon (NN) cross section on the number of proton(neutron) emissions N) are studied respe…