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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 1.

Energy (from Equation (12)) as a function of baryonic density for ions. Solid lines correspond to the results of our microscopical simulations, while the ideal gas limit for each given temperature is shown as a dashed line, to showcase the system reaching it at sufficiently small densities.

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