The nuclear energy density functionals with modified radial dependence of the isoscalar effective mass

Abstract

Calculations for infinite nuclear matter with realistic nucleon-nucleon interactions suggest that the isoscalar effective mass (IEM) of a nucleon at the saturation density equals $m^{\ast }/m\sim 0.8\pm 0.1$, at variance with empirical data on the nuclear level density in finite nuclei which are consistent with $m^{\ast }/m\approx 1$. This contradicting results might be reconciled by enriching the radial dependence of IEM. In this work four new terms are introduced into the Skyrme-force inspired local energy-density functional: $\tau (\nabla \rho {)}^2$, $\tau \frac{d\rho }{dr}$, ${\tau }^2$ and $\tau \Delta \rho$. The aim is to investigate how they influence the radial dependence of IEM and, in turn, the single-particle spectra.

6 pages, 2 figures, contribution from 16th Nuclear Physics Workshop in Kazimierz Dolny, Poland

References in corpus (2)

• Spin-orbit and tensor mean-field effects on spin-orbit splitting including self-consistent core polarizations
• Error analysis of nuclear mass fits

Cited by in corpus (2)

• Nuclear energy functional with a surface-peaked effective mass: Global properties
• Sensitivity of $\beta$-decay rates to the radial dependence of the nucleon effective mass