17F+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 

作者机构：Center for Nuclear Studythe University of Tokyo China Institute of Atomic Energy(CIAE) Shanghai Institute of Applied Physics(SINAP)CAS Nishina CenterRIKEN Department of PhysicsChung-Ang University Department of PhysicsKyushu University RCNPOsaka University Department of Physics and AstronomyMcMaster University 

出 版 物：《IMP & HIRFL Annual Report》 (中国科学院近代物理研究所和兰州重离子研究装置年报(英文版))

年 卷 期：2012年第0期

页      面：55-56页

学科分类：08[工学] 0827[工学-核科学与技术] 082701[工学-核能科学与工程] 

摘      要：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 *** far,its reaction rate is still ***,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.