Calculating some nuclear properties of chromium isotopes in the shell model

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dc.authoridKorna, Ahmed/0000-0001-5605-4065
dc.authoridAlshammari, Hamed/0000-0001-8443-4102
dc.authoridAbbasi, Akbar/0000-0002-4664-3744
dc.authoridAli, Ahmed H./0000-0002-1525-1406
dc.contributor.authorAli, Ahmed H.
dc.contributor.authorAbbasi, Akbar
dc.contributor.authorAkkoyun, Serkan
dc.contributor.authorKorna, A. H.
dc.contributor.authorHossain, I.
dc.contributor.authorAlshammari, H.
dc.contributor.authorZakaly, Hesham M. H.
dc.date.accessioned2025-05-04T16:47:22Z
dc.date.available2025-05-04T16:47:22Z
dc.date.issued2024
dc.departmentSivas Cumhuriyet Üniversitesi
dc.description.abstractThe present study provides an in-depth theoretical examination of the shell model for a range of even-even Chromium (Z = 24) isotopes, encompassing neutron numbers both 22 and 36. The shell model calculations relied on assumptions about the disregarded core-polarization effects and the utilization of effective charges. We performed extensive theoretical calculations to determine the probability of reduced electric quadrupole transition, B(E2;0g.s+ -> 2+), the intrinsic quadrupole moments (Q0), the deformation parameters (beta 2,delta), and the inclusion of effective interactions such as fpd6, fpv, fpbm, and kb3. Using the NuShellX@MSU algorithm, the one-body density matrix elements (OBDM) were computed for these isotopes. Various effective charges were utilized in these computations, including NU-E effective charges obtained from the Nushellx@MSU software, ST-E standard effective charges, and BM-E effective charges calculated using Bohr and Mottelson's method. Comparative analysis was conducted between the theoretical values of transition rate B(E2), intrinsic quadrupole moments, deformation parameters and the available experimental data. The gained theoretical conclusions were subsequently contrasted with prior experimental data, which had similarly demonstrated the collapse of the magical property of the Cr isotope. The intrinsic quadrupole moment was optimal when employing the kb3 interaction, but the deformation parameter appeared optimal when using two interactions, fpbm and kb3. Furthermore, it has been demonstrated that the magical characteristic of the 52Cr (N = 28) isotope undergoes collapse.
dc.identifier.doi10.1007/s12648-024-03478-9
dc.identifier.issn0973-1458
dc.identifier.issn0974-9845
dc.identifier.scopus2-s2.0-85211504079
dc.identifier.scopusqualityQ2
dc.identifier.urihttps://doi.org/10.1007/s12648-024-03478-9
dc.identifier.urihttps://hdl.handle.net/20.500.12418/35582
dc.identifier.wosWOS:001367938800001
dc.identifier.wosqualityQ2
dc.indekslendigikaynakWeb of Science
dc.indekslendigikaynakScopus
dc.language.isoen
dc.publisherIndian Assoc Cultivation Science
dc.relation.ispartofIndian Journal of Physics
dc.relation.publicationcategoryMakale - Uluslararası Hakemli Dergi - Kurum Öğretim Elemanı
dc.rightsinfo:eu-repo/semantics/closedAccess
dc.snmzKA_WOS_20250504
dc.subjectCore
dc.subjectDeformation
dc.subjectExcitation
dc.subjectTransition rate
dc.subjectIntrinsic
dc.subjectQuadrupole
dc.titleCalculating some nuclear properties of chromium isotopes in the shell model
dc.typeArticle

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