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DC Field | Value | Language |
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dc.contributor.author | Kumar, P. | |
dc.contributor.author | Jha, K. | |
dc.contributor.author | Raina, P.K. | |
dc.contributor.author | Singh, P. P. | |
dc.date.accessioned | 2018-12-20T09:08:29Z | |
dc.date.available | 2018-12-20T09:08:29Z | |
dc.date.issued | 2018-12-20 | |
dc.identifier.uri | http://localhost:8080/xmlui/handle/123456789/1033 | |
dc.description.abstract | The experimental states of nuclei, close to semi-magic nuclei, having one extra proton on top of closed proton core, in general, connote the arrangement of proton orbitals within a shell. Herein, we have studied the arrangement of proton orbitals (π0d5/2, π1s1/2and π0d3/2) in sd-shell for Fluorine isotopes within the nuclear shell model framework. The contribution of different components of effective nucleon-nucleon interaction in the evolution of the energies of proton orbitals, and the orbital energy gaps π0d5/2−π1s1/2and π0d5/2−π0d3/2at 23,25F has been examined. Results show the evolution of quasi-shell gap at 23F due to key contribution of central force, in particular, of its even-channel, and destructive interference in the contribution of spin–orbit and tensor force. The excitation energies of 12+1and 32+1states of 23F, and 12+1state of 25F are in good agreement with their respective orbital energy gaps. The origin of 32+1state of 25F and its excitation energy has been delineated as an effect of the breakdown of semi-magic core 24O. ©2018 Elsevier B.V. All rights reserved. | en_US |
dc.language.iso | en_US | en_US |
dc.subject | Effective single particle energy | en_US |
dc.subject | Orbital energy gap | en_US |
dc.subject | Shell model | en_US |
dc.subject | Single particle nature | en_US |
dc.title | Quasi shell gap at 23F | en_US |
dc.type | Article | en_US |
Appears in Collections: | Year-2018 |
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