Determination of the 12C(p, γ)13N reaction rates from the 12C(7Li,6He)13N reaction

被引：14

作者：

Li ZhiHong ^{[1
]}

Su Jun ^{[1
]}

Guo Bing ^{[1
]}

Li ZhiChang ^{[1
]}

Bai XiXiang ^{[1
]}

Liu JianCheng ^{[1
]}

Li YunJu ^{[1
]}

Yan ShengQuan ^{[1
]}

Wang BaoXiang ^{[1
]}

Wang YouBao ^{[1
]}

Lian Gang ^{[1
]}

Zeng Sheng ^{[1
]}

Li Ertao ^{[1
]}

Chen YongShou ^{[1
]}

Shu NengChuan ^{[1
]}

Fan QiWen ^{[1
]}

Liu WeiPing ^{[1
]}

机构：

[1] China Inst Atom Energy, Beijing 102413, Peoples R China

来源：

SCIENCE CHINA-PHYSICS MECHANICS & ASTRONOMY | 2010年 / 53卷 / 04期

基金：

中国国家自然科学基金;

关键词：

the C-12(Li-7; He-6)N-13; reaction; DWBA analysis; asymptotic normalization coefficient; astrophysical S(E)-factor; 1P SHELL NUCLEI; LIGHT-NUCLEI; ANGULAR-DISTRIBUTIONS; SPECTROSCOPIC FACTORS; ELASTIC-SCATTERING; RADIATIVE-CAPTURE; UNBOUND STATES; CARBON; STARS; C-13;

D O I：

10.1007/s11433-010-0128-8

中图分类号：

O4 [物理学];

学科分类号：

0702 ;

摘要：

The angular distribution of the C-12(Li-7,He-6)N-13 reaction at E(Li-7) = 44.0 MeV was measured at the HI-13 tandem accelerator of Beijing, China. The asymptotic normalization coefficient (ANC) of N-13 -> C-12 + p was derived to be (1.64 +/- 0.11) fm(-1/2) through the distorted wave Born approximation (DWBA) analysis. The ANC was then used to deduce the astrophysical S(E) factors and reaction rates for the C-12(p, gamma)N-13 direct capture reaction at energies of astrophysical relevance.

引用

页码：658 / 663

页数：6

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