Energy Density Functional Approach to Superfluid Nuclei

Abstract

We show that within the framework of a simple local nuclear energy density functional (EDF), one can describe accurately the one-- and two--nucleon separation energies of semi--magic nuclei. While for the normal part of the EDF we use previously suggested parameterizations, for the superfluid part of the EDF we use the simplest possible local form compatible with known nuclear symmetries.

4 pages + 3 embedded figures, published version

References in corpus (2)

• Pairing in nuclear systems: from neutron stars to finite nuclei
• Relativistic Hartree-Bogoliubov model with density-dependent meson-nucleon couplings

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