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Equation of State for Warm Neutron Star Outer Crusts

  • Authors: David Barba-González, Conrado Albertus, M. Ángeles Pérez-García

David Barba-González et al 2026 The Astrophysical Journal 1012 .

  • Provider: AAS Journals

Caption: Figure 4.

Thermal index Γth as a function of baryonic density for several selected temperatures, as coming directly from MD. The simulated data points are tabulated in Table 2. We include (blue dashed line) the same Γth for an electron gas, to showcase ionic effects.

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