  We study the structural properties of some nuclei in the region of light mass
using simple effective interaction in the frame work of microscopic non
relativistic Hartree-Fock and relativistic mean field formalism. For the
reaction dynamics, well known Glauber model is used with the conjunctions of
the densities obtained from these formalism. We observe good agreement of
results by both the formalism in comparison to the experimental values. These
two different approaches seems to be equally capable to reproduce the ground
state properties of nuclei in this region. A careful study of reaction dynamics
suggest the superiority of relativistic mean field over the Hartree-Fock with
simple effective interaction densities. But good agreement of reaction cross
section is appeared with simple effective interaction density for halo nuclear
systems. The possibility of existence of bubble nuclei are also studied using
both the formalism.
