66 citations · 221 across the 11 of their papers we have counts for
12 papers
Symmetry energy effect on the secondary component of GW190814 as a neutron star
Xuhao Wu, Shishao Bao, Hong Shen +1
The secondary component of GW190814 with a mass of 2.50-2.67 may be the lightest black hole or the heaviest neutron star ever observed in a binary compact object system…
Impact of strong magnetic fields on the inner crust of neutron stars
S. S. Bao, J. N. Hu, H. Shen
We study the impact of strong magnetic fields on the pasta phases that are expected to exist in the inner crust of neutron stars. We employ the relativistic mean field model to des…
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…
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 nuclear symmetry energy and equation of state on neutron star properties
Fan Ji, Jinniu Hu, Shishao Bao +1
We study the effects of nuclear symmetry energy on the mass-radius relation and tidal deformability of neutron stars, considering the self-consistency of the equation of state (EOS…
The phase transition in hot hypernuclei within relativistic Thomas-Fermi approximation
Jinniu Hu, Zhaowen Zhang, Shishao Bao +1
A self-consistent description for hot hypernuclei in hypothetical big boxes is developed within the relativistic Thomas-Fermi approximation in order to investigate directly the…