Determination of the Astrophysical S(E) Factors or Rates for Radiative Capture Reaction with One Nucleon Transfer Reaction  

作　　者：李志宏 郭冰 李云居 苏俊 李二涛 白希祥 王友宝 曾晟 王宝祥 颜胜权 李志常 刘建成 连钢 金孙均 刘鑫 柳卫平 

机构地区：[1]China Institute of Atomic Energy

出　　处：《Plasma Science and Technology》2012年第6期488-491,共4页等离子体科学和技术（英文版）

基　　金：supported by the National Basic Research Programme of China (No. 2007CB815003);National Natural Science Foundation of China(Nos. 10675173, 10705053, 10735100 and 11021504)

摘　　要：The radiative capture reaction plays an important role in nuclear astrophysics. We have indirectly measured the astrophysical S（E） factors for some proton capture reactions and reaction rates for several neutron capture reactions with one nucleon transfer reactions at HI-13 tandem accelerator in recent years. Some of them are compiled into IAEA EXFOR database and JINA REACLIB project, and used in the network calculations of Big Bang nucleosynthesis and type-I X-ray bursts.The radiative capture reaction plays an important role in nuclear astrophysics. We have indirectly measured the astrophysical S（E） factors for some proton capture reactions and reaction rates for several neutron capture reactions with one nucleon transfer reactions at HI-13 tandem accelerator in recent years. Some of them are compiled into IAEA EXFOR database and JINA REACLIB project, and used in the network calculations of Big Bang nucleosynthesis and type-I X-ray bursts.

关 键 词：NUCLEOSYNTHESIS transfer reaction spectroscopic factor radiative capture 

分 类 号：P14[天文地球—天体物理]