210 citations · 1.3k across the 39 of their papers we have counts for
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Extracting the Central Sound Speed of Neutron Stars through Intrinsic Stellar Structure Scaling with Reduced Equation-of-State Model Dependence
Jian-Hao Shi, Bao-Jun Cai, Yu-Gang Ma
Inferring neutron star (NS) core properties remains sensitive to the assumed equation of state (EOS). Using a nonlinear Walecka model with generalized -meson self-interactions,…
Neutron Skin Effects on Particle Emission in Heavy-Ion Collisions: A Topic Review with Astrophysical and Nuclear Structure Connections
Bao-Jun Cai, De-Qing Fang, Yu-Gang Ma
The neutron skin, defined by the difference between neutron and proton root-mean-square radii, is a characteristic manifestation of isospin asymmetry and an important probe of the…
A New Scaling of Neutron Star Tidal Deformability for Directly Probing the Central Equation of State Parameter
Jian-Hao Shi, Bao-Jun Cai, Bao-An Li +1
The dimensionless tidal deformability, , of neutron stars (NSs), inferred from gravitational-wave (GW) observations, has thus far been used primarily to constrain the pressure o…
An Effective Upper Bound on the Pressure-to-Energy Density Ratio in Neutron Stars
Bao-Jun Cai, Bao-An Li, Yu-Gang Ma
The equation-of-state (EOS) parameter , defined as the ratio of pressure to energy density, encapsulates the fundamental response of matter under extreme com…