The correlation between the charge radii differences in mirror nuclei pairs and the neutron
skin thickness has been studied with the so-called finite range simple effective interaction …

The properties of the core-crust transition in neutron stars are investigated using effective
nuclear forces of finite range. Special attention is paid to the so-called dynamical method for …

The detailed knowledge of the inner crust properties of neutron stars might be important to
explain different phenomena such as pulsar glitches or the possibility of an r-process site in …

The high-density behavior of stellar matter composed of nucleons and leptons under β β
equilibrium and charge neutrality conditions is studied with the Skyrme parametrizations …

An existing parametrization of the simple effective interaction (SEI) that is able to reproduce
the experimentally known crossing between the 2 p 3/2 and 1 f 5/2 single-particle (sp) proton …

The saturation properties of symmetric and asymmetric nuclear matter have been computed
using the finite range simple effective interaction with Yukawa form factor. The results of …

The importance of the fourth and higher order terms in the Taylor series expansion of energy
of isospin asymmetric nuclear matter in studies of the neutron star crust–core phase …

Deformed and spherical even–even nuclei are studied using a finite-range simple effective
interaction within the Hartree–Fock–Bogoliubov mean-field approach. Different parameter …

The properties of spin polarized pure neutron matter and symmetric nuclear matter (SNM)
are studied using the finite range simple effective interaction, upon its parametrization …

An extensive study is carried out for the island of stability in the superheavy nuclei Z= 120
and N= 164–220 within the effective field theory motivated relativistic mean-field (E-RMF) …