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EXPERIMENTAL INVESTIGATION OF THE STELLAR REACTION (30)S(p, gamma)(31) Cl VIA COULOMB DISSOCIATION
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(蔡翔舟); Fang, D(方德清); Ma, YG(马余刚); Tian, W(田文栋); 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
2010
Conference NameInternational Symposium on Forefronts of Researches in Exotic Nuclear Structures
Source PublicationMODERN PHYSICS LETTERS A
Pages1763
Conference DateMAR 01-04, 2010
Conference PlaceTokamachi, JAPAN
AbstractThe Coulomb dissociation of the proton-rich nuclei (31)Cl was studied experimentally using (31)Cl beams at 58 MeV/nucleon with a lead target. The relative energy between the reaction products, (30)S and proton, was obtained. The first excited state in (31)Cl was observed which is relevant to the resonant capture of stellar (30)S(p, gamma)(31)Cl reaction
ISSN0217-7323
Indexed BySCI
Funding Project应物所课题组
Language英语
Document Type会议论文
Identifierhttp://ir.sinap.ac.cn/handle/331007/8839
Collection中科院上海应用物理研究所2004-2010年
Recommended Citation
GB/T 7714
Togano, Y,Motobayashi, T,Aoi, N,et al. EXPERIMENTAL INVESTIGATION OF THE STELLAR REACTION (30)S(p, gamma)(31) Cl VIA COULOMB DISSOCIATION[C],2010:1763.
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