2H(6He,7Li)n, 12C(7Li,6He)13N reactions and 12C(p,γ)13N astrophysical S(E) factors

被引：5
|
作者：
Li, Z. H. [1 ]
Su, J. [1 ]
Guo, B. [1 ]
Li, E. T. [1 ]
Li, Z. C. [1 ]
Bai, X. X. [1 ]
Li, Y. J. [1 ]
Liu, J. C. [1 ]
Yan, S. Q. [1 ]
Wang, B. X. [1 ]
Wang, Y. B. [1 ]
Lian, G. [1 ]
Zeng, S. [1 ]
Fang, X. [1 ]
Liu, W. P. [1 ]
Chen, Y. S. [1 ]
Shu, N. C. [1 ]
Fan, Q. W. [1 ]
机构：
[1] China Inst Atom Energy, Beijing 102413, Peoples R China
来源：
NUCLEAR PHYSICS A | 2010年 / 834卷 / 1-4期
基金：
中国国家自然科学基金;
关键词：
CAPTURE;
D O I：
10.1016/j.nuclphysa.2010.01.117
中图分类号：
O57 [原子核物理学、高能物理学];
学科分类号：
070202 ;
摘要：
Angular distributions of H-2(He-6,Li-7)n and C-12(Li-7,He-6)N-13 reactions were measured at the HI-13 tandem accelerator, Beijing. Asymptotic normalization coefficient (ANC) of N-13 -> C-12 + p was derived to be 1.64 +/- 0.11 fm(-1/2) through distorted wave Born approximation (DWBA) analysis, which was then used to deduce the astrophysical S(E) factors for direct capture in C-12(p,gamma)N-13 at energies of astrophysical relevance.
引用
收藏
页码：661C / 663C
页数：3
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