Constraints on the Skyrme Equations of State from Properties of Doubly Magic Nuclei

Abstract

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.

5 page, 5 figures

References in corpus (4)

• The Giant Dipole Resonance as a quantitative constraint on the symmetry energy
• Electric Dipole Polarizability in ${}^{208}$Pb: insights from the Droplet Model
• Tensor interaction contributions to single-particle energies
• Dispelling the curse of the neutron skin in atomic parity violation

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