EXPERIMENTAL INVESTIGATION OF THE STELLAR REACTION S-30(p, gamma)(31) Cl VIA COULOMB DISSOCIATION
| Data(s) |
2010
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|---|---|
| Resumo |
The Coulomb dissociation of the proton-rich nuclei Cl-31 was studied experimentally using Cl-31 beams at 58 MeV/nucleon with a lead target. The relative energy between the reaction products, S-30 and proton, was obtained. The first excited state in Cl-31 was observed which is relevant to the resonant capture of stellar S-30(p, gamma)Cl-31 reaction |
| Identificador | |
| Idioma(s) |
英语 |
| Fonte |
Togano, Y; Motobayashi, T; Aoi, N; Baba, H; Bishop, S; Doornenbal, P; Furukawa, T; Kanno, S; Kondo, Y; Kurokawa, M; Matsuo, Y; Murakami, H; Takeuchi, S; Yamada, K; Yoneda, K; Cai, X; Fang, D; Ma, YG; Tian, W; Wang, H; Ieki, K; Kurita, K; Matsushita, M; Okada, K; Shioda, R; Yamada, Y; Iwasa, N; Kume, N; Kawabata, T; Ota, S; Shimoura, S; Kobayashi, N; Nakamura, T; Satou, Y; Tanaka, K; Kuboki, T; Wang, J.EXPERIMENTAL INVESTIGATION OF THE STELLAR REACTION S-30(p, gamma)(31) Cl VIA COULOMB DISSOCIATION,MODERN PHYSICS LETTERS A,2010,25(21-23):1763-1766 |
| Palavras-Chave | #RIKEN |
| Tipo |
期刊论文 |
