The Barcelona-Catania-Paris-Madrid functional with a realistic effective mass

Abstract

The Barcelona-Catania-Paris-Madrid (BCPM) functional recently proposed to describe nuclear structure properties of finite nuclei is generalized as to include a realistic effective mass. The resulting functional is as good as the previous one in describing binding energies, radii, deformation properties, etc and, in addition, the description of Giant Quadrupole Resonance energies is greatly improved.

8 pages, 5 figures

References in corpus (9)

• Relativistic Nuclear Energy Density Functionals: adjusting parameters to binding energies
• Khon-Sham Density Functional Inspired Approach to Nuclear Binding
• Dynamic versus static fission paths with realistic interactions
• Nucleon effective masses within the Brueckner-Hartree-Fock theory: Impact on stellar neutrino emission
• Application of the gradient method to Hartree-Fock-Bogoliubov theory
• Neutron-proton effective mass splitting in neutron-rich matter at normal density from analyzing nucleon-nucleus scattering data within an isospin dependent optical model
• Octupole deformation properties of the Barcelona-Catania-Paris energy density functionals
• Deformation properties of the BCP energy density functional
• Systematic study of infrared energy corrections in truncated oscillator spaces

Cited by in corpus (16)

• Nuclear Equation of State from ground and collective excited state properties of nuclei
• Nucleon Effective Masses in Neutron-Rich Matter
• Towards an ab initio covariant density functional for nuclear structure
• Theory of Nuclear Fission
• Constraints on the symmetry energy and its associated parameters from nuclei to neutron stars
• Microscopically-based energy density functionals for nuclei using the density matrix expansion: Full optimization and validation
• Tides in merging neutron stars: Consistency of the GW170817 event with experimental data on finite nuclei
• Nucleon effective mass in hot dense matter
• Time-dependent extension of the self-consistent band theory for neutron star matter: Anti-entrainment effects in the slab phase
• Nucleus giant resonances from an improved isospin-dependent Boltzmann-Uehling-Uhlenbeck transport approach
• Isochronic evolution and the radioactive decay of r-process nuclei
• Optimized nuclear energy density functionals including long-range pion contributions
• Impact of Hot Inner Crust on Compact Stars at Finite Temperature
• New Skyrme parametrizations to describe finite nuclei and neutron star matter with realistic effective masses
• Microscopic-Macroscopic Approach for Ground-State Energies Based on the Gogny Force with the Wigner-Kirkwood Averaging Scheme
• Including particle-vibration coupling in the Fayans functional. Odd-even mass differences of semi-magic nuclei