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dc.contributor.authorNayak, R. L.-
dc.contributor.authorSahoo, T.-
dc.contributor.authorAcharya, A.-
dc.date.accessioned2022-03-25T06:09:53Z-
dc.date.available2022-03-25T06:09:53Z-
dc.date.issued2015-08-03-
dc.identifier.issn2321-8649-
dc.identifier.issn2321-9289-
dc.identifier.urihttp://dspace.chitkarauniversity.edu.in/xmlui/handle/123456789/275-
dc.description.abstractProton 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.en_US
dc.language.isoenen_US
dc.relation.ispartofseries;CHAENG/2013/51628-
dc.subjectNeutron and proton drip line nucleien_US
dc.subjectβ stability lineen_US
dc.subjectn- and p- skinen_US
dc.subjectphysicsen_US
dc.titleNuclei Near and Far From β-Stability Lineen_US
dc.typeArticleen_US
Appears in Collections:Vol. 3 No. 1 (2015)

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