Prolate-to-oblate shape phase transitions in neutron-rich odd-mass nuclei

dc.contributor.authorK. Nomura
dc.contributor.authorR. Rodríguez-Guzmán
dc.contributor.authorL. M. Robledo
dc.date.accessioned2025-08-06T10:34:15Z
dc.date.available2025-08-06T10:34:15Z
dc.date.issued2018
dc.description.abstractWe investigate the prolate‑to‑oblate shape phase transitions in the neutron‑rich Pt, Os, and Ir nuclei in the mass region A ≈ 190. The IBM-fermion Hamiltonian, used for odd‑mass ^185–199Pt, ^185–193Os, and ^185–195Ir, is partly derived from microscopic HFB calculations with the Gogny‑D1M interaction; remaining parameters are fitted to experimental odd‑mass spectral data. Calculated observables—especially low‑energy excitation spectra and effective deformation parameters—indicate a systematic shape transition with neutron number across all three isotopic chains, mirroring trends in neighboring even–even nuclei.
dc.identifier.citationNomura, K.; Rodríguez-Guzmán, R.; & Robledo, L. M. (2018). Prolate-to-oblate shape phase transitions in neutron-rich odd-mass nuclei. Physical Review C, 97(6): 064314. DOI: 10.1103/PhysRevC.97.064314 — arXiv:1803.07802v2 (nucl-th) — Nazarbayev University
dc.identifier.urihttps://nur.nu.edu.kz/handle/123456789/9095
dc.language.isoen
dc.subjectprolate-to-oblate shape transition
dc.subjectneutron-rich odd-mass Pt
dc.subjectOs
dc.subjectIr isotopes
dc.subjectinteracting boson-fermion model
dc.subjectGogny D1M energy density functional
dc.subjectmicroscopic–macroscopic modeling
dc.titleProlate-to-oblate shape phase transitions in neutron-rich odd-mass nuclei
dc.typeArticle

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