EXPERIMENTAL INVESTIGATION OF THE STELLAR REACTION (30)S(p, gamma)(31) Cl VIA COULOMB DISSOCIATION

Y. Togano,T. Motobayashi, N. Aoi,H. Baba,Shawn Bishop,X. Z. Cai, P. Doornenbal, D. Q. Fang,Takeshi Furukawa,Kazuo Ieki,Naohito Iwasa, Takeo Kawabata, S. Kanno,Nagao Kobayashi, Y. Kondo,T. Kuboki,N. Kume,K. Kurita,Meiko Kurokawa,Y. G. Ma, Y. Matsuo,H. Murakami,Masafumi Matsushita,Takashi Nakamura, K. Okada,Shuichi Ota,Y. Satou,Susumu Shimoura, R. Shioda, K. Tanaka,Satoshi Takeuchi,Wendong Tian,H. W. Wang,J. S. Wang,Kazunari Yamada,Y. Yamada, K. Yoneda

International Nuclear Physics Conference 2010, INPC2010（2011）

引用 3|浏览3

暂无评分

摘要

Coulomb dissociation of the proton-rich nucleus 31Cl was studied experimentally using a 31Cl beam at 58 MeV/nucleon with a lead target. The relative energy spectrum of 30S+p system 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 stellar 30S(p,γ)31Cl reaction. Discussion for another observed state is also given.

查看译文

AI 理解论文

溯源树

样例

生成溯源树，研究论文发展脉络

Chat Paper

正在生成论文摘要