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Isovector splitting of nucleon effective masses, ab-initio benchmarks and extended stability criteria for Skyrme energy functionals

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arxiv nucl-th/0607065 v2 pith:JMIEVG7X submitted 2006-07-28 nucl-th

classification nucl-th
keywords skyrmeab-initioeffectiveenergyfinitemassessplittingability
verification ladder T0 review T1 audit T2 compute T3 formal
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We study the effect of the splitting of neutron and proton effective masses with isospin asymmetry on the properties of the Skyrme energy density functional. We discuss the ability of the latter to predict observable of infinite matter and finite nuclei, paying particular attention to controlling the agreement with ab-initio predictions of the spin-isospin content of the nuclear equation of state, as well as diagnosing the onset of finite size instabilities, which we find to be of critical importance. We show that these various constraints cannot be simultaneously fulfilled by the standard Skyrme force, calling at least for an extension of its P-wave part.

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  1. White dwarf-neutron star matter transition and the effect of light elements

    nucl-th 2026-08 conditional novelty 5.0 of 10

    A unified relativistic mean-field model connects white dwarfs to neutron stars and finds light-element seeds shift neutron star radii by roughly 0.2 km at 1.4 solar masses.

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