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20232026
most citedNovel Scalings of Neutron Star Properties from Analyzing Dimensionless Tolman--Oppenheimer--Volkoff Equations

14 citations · 37 across the 10 of their papers we have counts for

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6 papers · 1 filter

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…

astro-ph.HE2025★ 1 cited

Is The Trace Anomaly at its Minimum Value at Neutron Star Centers?

Bao-Jun Cai, Bao-An Li, Yu-Gang Ma

While the equation of state (EOS) of neutron star (NS) matter has been extensively studied, the EOS-parameter or equivalently the dimensionless…

astro-ph.HE2025

Revisiting the Possibility of a Sharp Phase Transition in Cold Neutron Stars

Bao-Jun Cai, Bao-An Li, Yu-Gang Ma

First-order phase transitions (FOPTs) in cold neutron stars (NSs) have been extensively studied and have provided valuable insights into the behavior of the densest matter visible…

astro-ph.HE2025★ 14 cited

Novel Scalings of Neutron Star Properties from Analyzing Dimensionless Tolman--Oppenheimer--Volkoff Equations

Bao-Jun Cai, Bao-An Li

The TOV equations govern the radial evolution of pressure and energy density in static neutron stars (NSs) in hydrodynamical equilibrium. Using the reduced pressure and energy dens…

astro-ph.HE2024★ 4 cited

New Insights into Supradense Matter from Dissecting Scaled Stellar Structure Equations

Bao-Jun Cai, Bao-An Li

The strong-field gravity in General Relativity (GR) realized in neutron stars (NSs) renders the Equation of State (EOS) of supradense neutron star (NS) matter to b…

astro-ph.HE2024★ 6 cited

Unraveling Trace Anomaly of Supradense Matter via Neutron Star Compactness Scaling

Bao-Jun Cai, Bao-An Li

The trace anomaly quantifies the possibly broken conformal symmetry in supradense matter under pressure at energy density . Pertu…