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GUO Bing (郭冰), LI Zhihong (李志宏), LI Yunju (李云居), SU Jun (苏俊), BAI Xixiang (白希祥), CHEN Yongshou (陈永寿), FAN Qiwen (樊启文), JIN Sunjun (金孙均), LI Ertao (李二涛), LI Zhichang (李志常), LIAN Gang (连钢), et al. Indirect Measurement of Astrophysical 13C(α,n)16O S-Factors[J]. Plasma Science and Technology, 2012, 14(5): 357-359. DOI: 10.1088/1009-0630/14/5/01
Citation: GUO Bing (郭冰), LI Zhihong (李志宏), LI Yunju (李云居), SU Jun (苏俊), BAI Xixiang (白希祥), CHEN Yongshou (陈永寿), FAN Qiwen (樊启文), JIN Sunjun (金孙均), LI Ertao (李二涛), LI Zhichang (李志常), LIAN Gang (连钢), et al. Indirect Measurement of Astrophysical 13C(α,n)16O S-Factors[J]. Plasma Science and Technology, 2012, 14(5): 357-359. DOI: 10.1088/1009-0630/14/5/01
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    Abstract
  • The 13C(α,n)16O reaction is believed to be the main neutron source reaction for the s-process in AGB stars. The astrophysical S-factors of this reaction have been determined based on an evaluation of the α spectroscopic factor of the 1/2+ subthreshold state in 17O (Ex = 6.356 MeV) by using the 13C(11B,7Li)17O α transfer reaction. Our result confirms that the 1/2+ subthreshold resonance is dominant for the 13C(α,n)16O reaction at low energies of astrophysical interest.
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