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dc.contributor.authorKumar, P.-
dc.contributor.authorJha, K.-
dc.contributor.authorRaina, P. K.-
dc.contributor.authorSingh, P. P.-
dc.date.accessioned2021-08-24T21:36:11Z-
dc.date.available2021-08-24T21:36:11Z-
dc.date.issued2021-07-25-
dc.identifier.urihttp://localhost:8080/xmlui/handle/123456789/2486-
dc.description.abstractThe 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, π1s1/2 and 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 − π1s1/2 and π0d5/2 − π0d3/2 at 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 1 2 + 1 and 3 2 + 1 states of 23F, and 1 2 + 1 state of 25F are in good agreement with their respective orbital energy gaps. The origin of 3 2 + 1 state of 25F and its excitation energy has been delineated as an effect of the breakdown of semi-magic core 24Oen_US
dc.language.isoen_USen_US
dc.subjectEffective single particle energyen_US
dc.subjectOrbital energy gapen_US
dc.subjectShell modelen_US
dc.subjectSingle particle natureen_US
dc.titleQuasi shell gap at 23Fen_US
dc.typeArticleen_US
Appears in Collections:Year-2019

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