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A New Scaling of Neutron Star Tidal Deformability for Directly Probing the Central Equation of State Parameter
general-relativity-and-quantum-cosmologyhigh-energy-astrophysical-phenomenanuclear-experimentnuclear-theory
The dimensionless tidal deformability, $Λ$, of neutron stars (NSs), inferred from gravitational-wave (GW) observations, has thus far been used primarily to constrain the pressure of dense matter near twice nuclear saturation density, leaving the core equation of state (EOS) largely inaccessible to i
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