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DC Field | Value | Language |
---|---|---|
dc.contributor.author | Sreeja, I. | - |
dc.contributor.author | Balasubramaniam, M. | - |
dc.date.accessioned | 2022-04-08T08:51:35Z | - |
dc.date.available | 2022-04-08T08:51:35Z | - |
dc.date.issued | 2018-02-05 | - |
dc.identifier.issn | 2321-8649 | - |
dc.identifier.issn | 2321-9289 | - |
dc.identifier.uri | http://dspace.chitkarauniversity.edu.in/xmlui/handle/123456789/360 | - |
dc.description.abstract | A 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.iso | en | en_US |
dc.relation.ispartofseries | ;CHAENG/2013/51628 | - |
dc.subject | Halo nuclei | en_US |
dc.subject | Cluster Core model | en_US |
dc.subject | Preformation Probability | en_US |
dc.subject | nuclear physics | en_US |
dc.title | The Three-Body Structure of 2n and 2p Halo Nuclei | en_US |
dc.type | Article | en_US |
Appears in Collections: | Vol. 5 No. 2 (2018) |
Files in This Item:
File | Description | Size | Format | |
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59-Article Text-69-1-10-20190819.pdf | 1.35 MB | Adobe PDF | View/Open |
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