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Simplified method to include the tensor contribution in α-cluster model
https://kitami-it.repo.nii.ac.jp/records/7258
https://kitami-it.repo.nii.ac.jp/records/72588296a0cf-a5f7-400f-ba49-2f6339c4c115
| 名前 / ファイル | ライセンス | アクション |
|---|---|---|
pr73_34310.pdf (225.5 kB)
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| Item type | 学術雑誌論文 / Journal Article(1) | |||||
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| 公開日 | 2008-02-17 | |||||
| タイトル | ||||||
| タイトル | Simplified method to include the tensor contribution in α-cluster model | |||||
| 言語 | en | |||||
| 言語 | ||||||
| 言語 | eng | |||||
| 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 |
Itagaki, N
× Itagaki, N× Masui, H× Ito, M× Aoyama, S× Ikeda, K |
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| 抄録 | ||||||
| 内容記述タイプ | Abstract | |||||
| 内容記述 | We propose a simplified model to directly take into account the contribution of the tensor interaction (SMT) for light nuclei by extending the α-cluster model. In Be, the energy curvewith respect to the relative distance between the two He clusters suggests that the cluster structure persists even though the tensor interaction contributes strongly. In addition to SMT, a simplified method to take into account the strong spin-orbit contribution is introduced and the coupling effects of these two models is shown to be important in C, in contrast to Be. | |||||
| 内容記述 | ||||||
| 内容記述タイプ | Other | |||||
| 内容記述 | (c)2006 The American Physical Society | |||||
| 書誌情報 |
Physical Review C 巻 73, p. 034310-1-034310-7, 発行日 2006 |
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| DOI | ||||||
| 識別子タイプ | DOI | |||||
| 関連識別子 | http://doi.org/10.1103/PhysRevC.73.034310 | |||||
| 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 | |||||
| 言語 | en | |||||
| 著者版フラグ | ||||||
| 言語 | en | |||||
| 値 | author | |||||
| 出版タイプ | ||||||
| 出版タイプ | AM | |||||
| 出版タイプResource | http://purl.org/coar/version/c_ab4af688f83e57aa | |||||
