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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 2.

Points depict MD results for pressure as a function of baryonic density within ions for different temperatures. Smooth, solid lines are predictions from our neural network prescription, with goodness of fit R2 > 0.989718 when compared to the simulation’s results.

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