Astrophysical reaction rate of30S(p, γ)31Cl studied by Coulomb dissociation
文献类型：会议论文
| 作者 | Togano, Y.1; Motobayashi, T.1; Aoi, N.1; Baba, H.1; Bishop, S.1; Cai, X.2; Doornenbal, P.1; Fang, D.2; Furukawa, T.1; Ieki, K.3 |
| 出版日期 | 2010 |
| 会议地点 | Heidelberg, Germany |
| 英文摘要 | The Coulomb dissociation of the proton-rich nucleus31Cl was studied experimentally using a31Cl beam at 58 MeV/nucleon with a lead target. The relative energy spectrum between30S ions and protons was obtained from the measured momentum vectors of the reaction products detected in coincidence by the invariant mass method. The first excited state in 31Cl was observed which is relevant to the resonant capture in the stellar30S(p, γ)31Cl reaction. Discussion for another observed state is also given. © Copyright owned by the author(s). |
| 会议录 | 11th Symposium on Nuclei in the Cosmos, NIC 2010
 |
| 会议录出版者 | Proceedings of Science (PoS) |
| 源URL | [http://119.78.100.186/handle/113462/63927]  |
| 专题 | 中国科学院近代物理研究所 |
| 作者单位 | 1.RIKEN Nishina Center, Saitama 351-0198, Japan 2.Shanghai Institute of Applied Physics, Chinese Academy of Sciences, Shanghai 201800, China 3.Department of Physics, Rikkyo University, Tokyo 171-8501, Japan 4.Department of Physics, Tohoku University, Miyagi 980-8578, Japan 5.Center for Nuclear Study, University of Tokyo, Saitama 351-0198, Japan 6.Department of Physics, Tokyo Institute of Technology, Tokyo 152-8551, Japan 7.Department of Physics, Saitama University, Saitama 338-8570, Japan 8.Institute of Modern Physics, Chinese Academy of Scienc Es, Lanzhou 730000, China |
| 推荐引用方式 GB/T 7714 | Togano, Y.,Motobayashi, T.,Aoi, N.,et al. Astrophysical reaction rate of30S(p, γ)31Cl studied by Coulomb dissociation[C]. 见:. Heidelberg, Germany. |
入库方式： OAI收割
来源：近代物理研究所
浏览0
下载0
收藏0
其他版本
除非特别说明，本系统中所有内容都受版权保护，并保留所有权利。