89 citations · 1.1k across the 63 of their papers we have counts for
9 papers · 1 filter
The origin of the spin-orbit and pseudospin-orbit splittings' evolution in neutron drop
Yinghui Ge, Ying Zhang, Jinniu Hu
We found the same staggering pattern in the evolution of the spin-orbit (SO) and pseudospin-orbit (PSO) splittings in neutron drops obtained by the energy-density functional (EDF)…
The possibility of the secondary object in GW190814 as a neutron star
Kaixuan Huang, Jinniu Hu, Ying Zhang +1
A compact object was observed with a mass by LIGO Scientific and Virgo collaborations (LVC) in GW190814, which provides a great challenge to the investigations…
Nuclear pasta in hot and dense matter and its influence on the equation of state for astrophysical simulations
Fan Ji, Jinniu Hu, Shishao Bao +1
We explore the properties of nuclear pasta appearing in supernova matter, i.e., matter at finite temperature with a fixed proton fraction. The pasta phases with a series of geometr…
Properties of nuclear matter in relativistic Brueckner-Hartree-Fock model with high-precision charge-dependent potentials
Chencan Wang, Jinniu Hu, Ying Zhang +1
Properties of nuclear matter are investigated in the framework of relativistic Brueckner-Hartree-Fock model with the latest high-precision charge-dependent Bonn (pvCD-Bonn) potenti…
Properties of neutron star described by a relativistic model
Chencan Wang, Jinniu Hu, Ying Zhang +1
Properties of neutron star are investigated by an available relativistic method, i.e., the relativistic Brueckner-Hartree-Fock (RBHF) model, with the latest high-preci…
The one-pion-exchange potential with contact terms from lattice QCD simulations
Jinniu Hu, Ying Zhang, Hong Shen +1
The pion-mass-dependent nucleon-nucleon () potentials in term of one-pion exchange and contact terms are obtained from the latest lattice QCD simulations of two-nucleon system,…
Effects of symmetry energy on the radius and tidal deformability of neutron stars in relativistic mean-field model
Jinniu Hu, Shishao Bao, Ying Zhang +3
The radii and tidal deformabilities of neutron stars are investigated in the framework of relativistic mean-field (RMF) model with different density-dependent behaviors of symmetry…
Effects of symmetry energy on equation of state for simulations of core-collapse supernovae and neutron-star mergers
Hong Shen, Fan Ji, Jinniu Hu +1
We construct a new equation of state (EOS) for numerical simulations of core-collapse supernovae and neutron-star mergers based on an extended relativistic mean-field model with a…
Single hypernuclei within quark mean-field model
Linzhuo Wu, Jinniu Hu, Hong Shen
The quark mean-field (QMF) model is applied to study the single hypernuclei. The charm baryon, , is constructed by three constituent quarks, , and , confin…