Please use this identifier to cite or link to this item:
http://dspace.chitkarauniversity.edu.in/xmlui/handle/123456789/275
Full metadata record
DC Field | Value | Language |
---|---|---|
dc.contributor.author | Nayak, R. L. | - |
dc.contributor.author | Sahoo, T. | - |
dc.contributor.author | Acharya, A. | - |
dc.date.accessioned | 2022-03-25T06:09:53Z | - |
dc.date.available | 2022-03-25T06:09:53Z | - |
dc.date.issued | 2015-08-03 | - |
dc.identifier.issn | 2321-8649 | - |
dc.identifier.issn | 2321-9289 | - |
dc.identifier.uri | http://dspace.chitkarauniversity.edu.in/xmlui/handle/123456789/275 | - |
dc.description.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. | en_US |
dc.language.iso | en | en_US |
dc.relation.ispartofseries | ;CHAENG/2013/51628 | - |
dc.subject | Neutron and proton drip line nuclei | en_US |
dc.subject | β stability line | en_US |
dc.subject | n- and p- skin | en_US |
dc.subject | physics | en_US |
dc.title | Nuclei Near and Far From β-Stability Line | en_US |
dc.type | Article | en_US |
Appears in Collections: | Vol. 3 No. 1 (2015) |
Files in This Item:
File | Description | Size | Format | |
---|---|---|---|---|
139-Article Text-214-1-10-20190821.pdf | 217.36 kB | Adobe PDF | View/Open |
Items in DSpace are protected by copyright, with all rights reserved, unless otherwise indicated.