Nuclear mass table in density functional approach inspired by neutron-star observations
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- Hana Gil
- Center for Extreme Nuclear Matters, Korea University, Seoul 02841, South Korea
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- Nobuo Hinohara
- Center for Computational Sciences, University of Tsukuba, Tsukuba, Ibaraki 305-8577, Japan
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- Chang Ho Hyun
- Department of Physics Education, Daegu University, Gyeonsan 38453, South Korea
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- Kenichi Yoshida
- Research Center for Nuclear Physics, Osaka University, Ibaraki, Osaka 567-0047, Japan
書誌事項
- 公開日
- 2023-10-20
- 資源種別
- journal article
- 権利情報
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- https://link.aps.org/licenses/aps-default-license
- https://link.aps.org/licenses/aps-default-accepted-manuscript-license
- DOI
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- 10.1103/physrevc.108.044316
- 10.48550/arxiv.2304.01546
- 公開者
- American Physical Society (APS)
この論文をさがす
説明
Background: Nuclear energy-density functional (EDF) approach has been widely used to describe nuclear-matter equations of state (EoS) and properties of finite nuclei. Recent advancements in neutron-star (NS) observations have put constraints on the nuclear EoS. The Korea-IBS-Daegu-SKKU (KIDS) functional has been then developed to satisfy the NS observations and applied to homogeneous nuclear matter and spherical nuclei. Purpose: We examine the performance of the KIDS functional by calculating the masses and charge radii of even-even nuclei towards the drip lines. Method: The Kohn-Sham-Bogoliubov equation is solved by taking into account the axial deformation. Results: The root-mean-square deviation of the binding energy and the charge radius for the KIDS functional is 4.5--5.1 MeV and 0.03--0.04 fm, which is comparable to that for existing EDFs. The emergence and development of nuclear deformation in open-shell nuclei are well described. The location of the neutron drip line is according to the nuclear-matter parameter characterizing the low-mass NS. Conclusions: The NS-observation-inspired EDF offers a reasonable reproduction of the structures of finite nuclei. A future global optimization including more nuclear data will give better accuracy and high predictive power of neutron-rich nuclei.
9 pages, 6 figures, and 2 tables
収録刊行物
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- Physical Review C
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Physical Review C 108 (4), 2023-10-20
American Physical Society (APS)
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詳細情報 詳細情報について
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- CRID
- 1360021390560880256
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- ISSN
- 24699993
- 24699985
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- 資料種別
- journal article
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- データソース種別
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- Crossref
- KAKEN
- OpenAIRE

