~(17)F+p共振散射的研究(英文)

• 作 者: 胡钧 He Jianjun Xu Shiwei H.Yamaguchi Ma Peng K.David Su Jun Wang Hongwei T.Nakao Y.Wakabayashi J.Y.Moon T.Teranishi H.S.Jung T.Hashimoto A.Chen D.Irvine S.Kubono
• 机 构: Center for Nuclear Study,the University of Tokyo,China Institute of Atomic Energy(CIAE),Shanghai Ins
• 出 处: IMP & HIRFL Annual Report
• 发表日期: 2012年00期
• 关键词: stellar 共振散射 F+p uncertain waiting proton explosive nuclei probably ignition

X-ray bursts[1]are probably an important source for the production of proton-rich nuclei via the high temperature rp-process[2],and the 14 O(α,p)17F reaction is thought to be one of the crucial stellar reactions during the ignition phase.By far,its reaction rate is still uncertain.Therefore,the studies of this waiting-point reaction are of great nuclear astrophysical importance to understand the energy generation and nucleosynthesis in the explosive stellar environments.

X-ray bursts [1] are probably an important source for the production of proton-rich nuclei via the high temperature rp-process [2], and the 14 O (α, p) 17F reaction is thought to be one of the crucial stellar reactions during the ignition phase. BY far, the study of this waiting-point reaction are of great nuclear astrophysical importance to understand the energy generation and nucleosynthesis in the explosive stellar environments.