Abstract
We study the structural properties of some light mass nuclei using two different formalisms (i) a recently developed simple effective interaction in the frame work of microscopic non-relativistic Hartree-Fock method and (ii) the well-known relativistic mean field approach with NL3 parameter set. The bulk properties like binding energy, root mean square radii and quadrupole deformation parameter are estimated and compared with the available experimental data. The predicted results of both the formalisms are well comparable with the experimental observations. The analysis of density profiles of these light mass nuclei suggest that 22O, 23F, 34Si and 46Ar have bubble like structure.
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