R.L. Nayak, T. Sahoo and A. Acharya*
Department of physics, VSS University of Technology, Burla, Orissa, India
*Email: aacharya@iopb.res.in
This article is published with open access at www.chitkara.edu.in/publications
Department of physics, VSS University of Technology, Burla, Orissa, India
*Email: aacharya@iopb.res.in
This article is published with open access at www.chitkara.edu.in/publications
Abstract: Proton to neutron ratio around β-stability line presents an open challenge to the nuclear physicists. The prominent milestone in this regard is the discovery of the super heavy elements, nuclear halos in the lightest neutron-rich nuclei, experimental mapping of the nuclear shell structure near and far from stability. In this present paper, the behavior of the p- and n- halo nuclei near the β-stability line are discussed considering the variation of radius with respect to the mass number and N~Z for different nuclei. Our aim is to study the nuclear properties through neutron and proton skin. The isospin symmetry breaking is for heavy halo nuclei of strong interest.
Keywords: Neutron and proton drip line nuclei; β stability line; n- and p- skin
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