Nuclear matter and finite nuclei properties using simple effective interaction

The last three decades have seen a regular interest to explain consistently the properties of nuclear matter, finite nuclei and nuclear reactions (nucleon-nucleus and nucleus-nucleus) with an effective interaction that has the efficiency to describe the two body system accurately. The relativistic and non-relativistic microscopic models, such as, Dirac-Brueckner-Hartree-Fock (DBHF), Brueckner-Hartree-Fock (BHF) and calculations using realistic interaction are considered to be standard techniques for reference in the regime of nuclear matter (NM), but ab initio extension to finite nucleus calculation in these models is still in rudimentary stage