Tri-axial deformation in nuclei with realistic NN interactions
arXiv:1405.6005 · doi:10.1103/PhysRevC.90.034312
Abstract
The structure of finite nuclei is investigated by employing an interaction model which is based on the low-momentum interaction . It is supplemented by a density-dependent contact interaction fitted to reproduce the saturation properties of infinite nuclear matter within the Hartree-Fock approach. The calculations of finite nuclei are performed in a basis of plane waves discretized in a cartesian box of appropriate size. As a first example the structure of Ne isotopes is considered ranging from Ne to the neutron drip line. Rather good agreement is obtained for the bulk properties of these nuclei without any free parameter. The basis is also appropriate to describe other deformed nuclei and the transition from discrete nuclei to homogeneous matter which is supposed to occur in the crust of neutron stars.
References in corpus (7)
- Chiral effective field theory and nuclear forces
- The influence of pairing on the nuclear matrix elements of the neutrinoless double beta decays
- Low-momentum interactions with smooth cutoffs
- Low-energy dipole excitations in neon isotopes and N=16 isotones within the quasiparticle random phase approximation and the Gogny force
- Relativistic Hartree-Fock-Bogoliubov model for deformed nuclei
- Weakly bound nuclei and realistic NN interactions
- Study of the ground-state energy of 40Ca with the CD-Bonn nucleon-nucleon potential