Please use this identifier to cite or link to this item: http://dspace.chitkarauniversity.edu.in/xmlui/handle/123456789/241
Full metadata record
DC FieldValueLanguage
dc.contributor.authorBalasubramaniam, M.-
dc.contributor.authorManimaran, K.-
dc.date.accessioned2022-03-09T05:23:42Z-
dc.date.available2022-03-09T05:23:42Z-
dc.date.issued2013-09-08-
dc.identifier.issn2321-8649-
dc.identifier.issn2321-9289-
dc.identifier.urihttp://dspace.chitkarauniversity.edu.in/xmlui/handle/123456789/241-
dc.description.abstractUsing the preformation cluster model of Gupta and collaborators we have studied all the possible cluster decay modes of 127 I. The calculated half-lives are compared with recently measured lower limits of cluster decay half-lives (for the clusters like 24Ne, 28Mg, 30Mg, 32Si, 34Si, 48Ca and 49Sc) of 127I. Our calculated half-life values lies well above the experimentally measured lower limits and the trend of the values also matches with experimental ones.en_US
dc.language.isoEngen_US
dc.relation.ispartofseriesCHAENG/2013/51628-
dc.subjectNuclearen_US
dc.subjectPhysicsen_US
dc.subjectCluster radioactivityen_US
dc.subjectFissionen_US
dc.titleCluster Radioactivity in 127Ien_US
dc.typeArticleen_US
Appears in Collections:Vol. 1 No. 1 (2013)

Files in This Item:
File Description SizeFormat 
7-Article Text-6-1-10-20190816.pdf578.63 kBAdobe PDFView/Open


Items in DSpace are protected by copyright, with all rights reserved, unless otherwise indicated.