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Comparison between the Gamow shell model and the cluster-orbital shell model for weakly bound systems
https://kitami-it.repo.nii.ac.jp/records/7354
https://kitami-it.repo.nii.ac.jp/records/7354cf079a3a-594b-4ff9-82d5-d8b9cff37a34
| 名前 / ファイル | ライセンス | アクション |
|---|---|---|
346masui_.pdf (162.1 kB)
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| Item type | 学術雑誌論文 / Journal Article(1) | |||||
|---|---|---|---|---|---|---|
| 公開日 | 2009-04-07 | |||||
| タイトル | ||||||
| タイトル | Comparison between the Gamow shell model and the cluster-orbital shell model for weakly bound systems | |||||
| 言語 | en | |||||
| 言語 | ||||||
| 言語 | eng | |||||
| キーワード | ||||||
| 主題Scheme | Other | |||||
| 主題 | nuclear shell model | |||||
| キーワード | ||||||
| 主題Scheme | Other | |||||
| 主題 | nuclear cluster model | |||||
| キーワード | ||||||
| 主題Scheme | Other | |||||
| 主題 | wave functions | |||||
| キーワード | ||||||
| 主題Scheme | Other | |||||
| 主題 | nuclei with mass number 1 to 5 | |||||
| キーワード | ||||||
| 主題Scheme | Other | |||||
| 主題 | nuclei with mass number 6 to 19 | |||||
| キーワード | ||||||
| 主題Scheme | Other | |||||
| 主題 | nuclear resonances | |||||
| 資源タイプ | ||||||
| 資源タイプ識別子 | http://purl.org/coar/resource_type/c_6501 | |||||
| 資源タイプ | journal article | |||||
| アクセス権 | ||||||
| アクセス権 | open access | |||||
| アクセス権URI | http://purl.org/coar/access_right/c_abf2 | |||||
| 著者 |
Masui, H
× Masui, H× Kato, K× Ikdea, K |
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| 抄録 | ||||||
| 内容記述タイプ | Abstract | |||||
| 内容記述 | We study contributions of poles and continua of the single-particle states to the wave function obtained by the cluster-orbital shell model (COSM). The COSM wave function is described in terms of a linear combination of nonorthogonal Gaussian basis sets. We study oxygen and helium isotopes as examples of normal and weakly bound nuclei. In the investigation of the contribution of the single-particle states, we expand the COSM wave function by using an extended completeness relation, which is constructed by the solution of the single-particle Hamiltonian. We use the complex scaling method to obtain the bound, resonant, and continuum states of the Hamiltonian and construct the extended completeness relation. The results are compared with those obtained by the Gamow shell model calculation. | |||||
| 内容記述 | ||||||
| 内容記述タイプ | Other | |||||
| 内容記述 | c2007 The American Physical Society | |||||
| 書誌情報 |
Physical Review C 巻 75, 号 3, p. 034316, 発行日 2007-03 |
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| ISSN | ||||||
| 収録物識別子タイプ | EISSN | |||||
| 収録物識別子 | 2469-9993 | |||||
| DOI | ||||||
| 識別子タイプ | DOI | |||||
| 関連識別子 | http://doi.org/10.1103/PhysRevC.75.034316 | |||||
| フォーマット | ||||||
| 内容記述タイプ | Other | |||||
| 内容記述 | application/pdf | |||||
| 出版者 | ||||||
| 出版者 | American Physical Society | |||||
| 著者版フラグ | ||||||
| 値 | publisher | |||||
| 出版タイプ | ||||||
| 出版タイプ | VoR | |||||
| 出版タイプResource | http://purl.org/coar/version/c_970fb48d4fbd8a85 | |||||
