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Sensitivity of Neutron Star Observables to Transition Density in Hybrid Equation-of-State Models
general-relativity-and-quantum-cosmologyhigh-energy-astrophysical-phenomenahigh-energy-physics-phenomenologynuclear-theorysolar-and-stellar-astrophysics
We investigate how the transition density \(ρ_{tr}\) affects hybrid constructions of the neutron-star equation of state (EoS) in which a nucleonic description at low densities is matched to a model-agnostic high-density extension based on a speed-of-sound parametrization. Using four representative n
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