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PhysRevC.105.024318.pdf | 1.04 MB | Adobe PDF | 見る/開く |
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DCフィールド | 値 | 言語 |
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dc.contributor.author | Yoshida, Kenichi | en |
dc.contributor.alternative | 吉田, 賢市 | ja |
dc.date.accessioned | 2022-05-31T06:45:14Z | - |
dc.date.available | 2022-05-31T06:45:14Z | - |
dc.date.issued | 2022-02 | - |
dc.identifier.uri | http://hdl.handle.net/2433/274166 | - |
dc.description.abstract | Background: The observation of the superdeformed (SD) bands in ⁶⁰, ⁶²Zn indicates that the particle number 30 is a magic particle number, where two- and four-neutron single particles are considered to be promoted to the intruder 1g₉/₂ shell. However, the SD-yrast band in ⁶²Zn is assigned negative parity. Purpose: I investigate various SD configurations in the rapidly rotating ⁶⁰, ⁶²Zn and ⁶⁴Ge, and attempt elucidating the different roles of the energy gaps at particle numbers 30 and 32. Method: I employ a nuclear energy-density functional method: the configuration-constrained cranked Skyrme-Kohn-Sham approach is used to describe the rotational bands near the yrast line. Results: The negative-parity SD bands appear higher in energy than the positive-parity SD-yrast band in ⁶⁰Zn by about 4 MeV, which is indicative of the SD doubly magic nucleus. However, the energy gap in ⁶⁴Ge is smaller ≈2–3 MeV, though the quadrupole deformation of the SD states in ⁶⁴Ge is greater than that of ⁶⁰Zn. The present calculation predicts the occurrence of the hyperdeformed state in ⁶⁰Zn and ⁶⁴Ge at a high rotational frequency ≈2.0MeV/ℏ due to the occupation of the h₁₁/₂ shell. Conclusions: An SD-shell gap at particle number 30 and 32 appears at different deformations and the energy gap at particle number 32 is low, which make the SD structures of ⁶²Zn unique, where the negative-parity SD states appear lower in energy than the positive-parity one. | en |
dc.language.iso | eng | - |
dc.publisher | American Physical Society (APS) | en |
dc.rights | ©2022 American Physical Society | en |
dc.title | Super- and hyperdeformation in ⁶⁰Zn, ⁶²Zn, and ⁶⁴Ge at high spins | en |
dc.type | journal article | - |
dc.type.niitype | Journal Article | - |
dc.identifier.jtitle | Physical Review C | en |
dc.identifier.volume | 105 | - |
dc.identifier.issue | 2 | - |
dc.relation.doi | 10.1103/PhysRevC.105.024318 | - |
dc.textversion | publisher | - |
dc.identifier.artnum | 024318 | - |
dcterms.accessRights | open access | - |
datacite.awardNumber | 19K03824 | - |
datacite.awardNumber | 19K03872 | - |
datacite.awardNumber.uri | https://kaken.nii.ac.jp/ja/grant/KAKENHI-PROJECT-19K03824/ | - |
datacite.awardNumber.uri | https://kaken.nii.ac.jp/ja/grant/KAKENHI-PROJECT-19K03872/ | - |
dc.identifier.pissn | 2469-9985 | - |
dc.identifier.eissn | 2469-9993 | - |
jpcoar.funderName | 日本学術振興会 | ja |
jpcoar.funderName | 日本学術振興会 | ja |
jpcoar.awardTitle | 原子核密度汎関数法によるベータ崩壊率の微視的・系統的計算手法の確立 | ja |
jpcoar.awardTitle | 汎関数くりこみ群による量子多体系の密度汎関数理論の構築と第一原理計算 | ja |
出現コレクション: | 学術雑誌掲載論文等 |

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