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Constraints on the Skyrme Equations of State from Properties of Doubly Magic Nuclei
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Constraints on the Skyrme Equations of State from Properties of Doubly Magic Nuclei
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I use properties of doubly-magic nuclei to constrain nuclear matter and neutron matter equations of state. I conclude that the data determined the value of the neutron equation of state and the symmetry energy near a density of $\rho_{on}$ = 0.10 nucleons/fm$^{3}$. The slope at that point is constrained by the value of the neutron skin.
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