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astro-ph.HE2026
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…
nucl-th2026
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…