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Analysis

This paper investigates the discrepancy in saturation densities predicted by relativistic and non-relativistic energy density functionals (EDFs) for nuclear matter. It highlights the interplay between saturation density, bulk binding energy, and surface tension, showing how different models can reproduce empirical nuclear radii despite differing saturation properties. This is important for understanding the fundamental properties of nuclear matter and refining EDF models.
Reference

Skyrme models, which saturate at higher densities, develop softer and more diffuse surfaces with lower surface energies, whereas relativistic EDFs, which saturate at lower densities, produce more defined and less diffuse surfaces with higher surface energies.