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

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arxiv 1308.3664 v1 pith:HX73KBPL submitted 2013-08-16 nucl-th

classification nucl-th
keywords neutronstateequationsmatternucleipropertiesvalueconclude
verification ladder T0 review T1 audit T2 compute T3 formal
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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.

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Forward citations

Cited by 5 Pith papers

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  3. Extended Skyrme effective interactions with higher-order momentum-dependence for transport models and neutron stars

    nucl-th 2024-12 conditional novelty 6.0 of 10

    The authors generalize the Skyrme pseudopotential to N5LO with p^10 momentum dependence, fit it to the optical potential up to 2 GeV, and show the resulting interactions reproduce HADES proton flow data.

  4. Toward a Unified Understanding of the Dense Matter Equation of State

    nucl-th 2025-11 conditional novelty 2.0 of 10

    A review of three Bayesian/computational frameworks for combining heavy-ion and astrophysical constraints on the dense-matter equation of state, plus a proposed unified integration workflow.

  5. Neutron skin thickness for $^{nat}$Pb, $^{159}$Tb and effects of deformation on matter radii for Mg, Na, Ar isotopes

    nucl-ex 2025-06

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