Please use this identifier to cite or link to this item: http://dspace.chitkarauniversity.edu.in/xmlui/handle/123456789/360
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dc.contributor.authorSreeja, I.-
dc.contributor.authorBalasubramaniam, M.-
dc.date.accessioned2022-04-08T08:51:35Z-
dc.date.available2022-04-08T08:51:35Z-
dc.date.issued2018-02-05-
dc.identifier.issn2321-8649-
dc.identifier.issn2321-9289-
dc.identifier.urihttp://dspace.chitkarauniversity.edu.in/xmlui/handle/123456789/360-
dc.description.abstractA three-cluster model developed for ternary fission studies has been applied for the first time to study the three-body structure of 2n and 2p halo nuclei. For the experimentally known 2n, 2p halo nuclei, all possible ternary fragmentation potential energy surface (PES) is calculated. The two-body breakup reported earlier, clearly indicated a strong minimum in the PES corresponding to 1n/1p and/or 2n/2p cluster plus core configuration. However, the present calculations of PES reveal that, the three- body breakup does not result always with 2n and/or 2p as a cluster. A 1n and/or 1p cluster along with the core is initially formed, and then the core loses one nucleon to make either a 2n plus core or 2p plus core structure. The results are substantiated with the calculations of preformation probability calculated within quantum mechanical fragmentation theory.en_US
dc.language.isoenen_US
dc.relation.ispartofseries;CHAENG/2013/51628-
dc.subjectHalo nucleien_US
dc.subjectCluster Core modelen_US
dc.subjectPreformation Probabilityen_US
dc.subjectnuclear physicsen_US
dc.titleThe Three-Body Structure of 2n and 2p Halo Nucleien_US
dc.typeArticleen_US
Appears in Collections:Vol. 5 No. 2 (2018)

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