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LI Zhihong (李志宏), GUO Bing (郭冰), LI Yunju (李云居), SU Jun (苏俊), LI Ertao (李二涛), BAI Xixiang (白希祥), WANG Youbao (王友宝), ZENG Sheng (曾晟), WANG Baoxiang (王宝祥), YAN Shengquan (颜胜权), LI Zhichang (李志常), et al. Determination of the Astrophysical S(E) Factors or Rates for Radiative Capture Reaction with One Nucleon Transfer Reaction[J]. Plasma Science and Technology, 2012, 14(6): 488-491. DOI: 10.1088/1009-0630/14/6/11
Citation: LI Zhihong (李志宏), GUO Bing (郭冰), LI Yunju (李云居), SU Jun (苏俊), LI Ertao (李二涛), BAI Xixiang (白希祥), WANG Youbao (王友宝), ZENG Sheng (曾晟), WANG Baoxiang (王宝祥), YAN Shengquan (颜胜权), LI Zhichang (李志常), et al. Determination of the Astrophysical S(E) Factors or Rates for Radiative Capture Reaction with One Nucleon Transfer Reaction[J]. Plasma Science and Technology, 2012, 14(6): 488-491. DOI: 10.1088/1009-0630/14/6/11
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Determination of the Astrophysical S(E) Factors or Rates for Radiative Capture Reaction with One Nucleon Transfer Reaction

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  • 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.
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