New determination of the astrophysical 13C(p, γ)14N S(E) factors and reaction rates via the 13C(7Li, 6He)14N reaction (vol 48, pg 13, 2012)

被引：0

作者：

Li, Y. J. ^{[1
]}

Li, Z. H. ^{[1
]}

Li, E. T. ^{[1
]}

Bai, X. X. ^{[1
]}

Su, J. ^{[1
]}

Guo, B. ^{[1
]}

Wang, B. X. ^{[1
]}

Yan, S. Q. ^{[1
]}

Zeng, S. ^{[1
]}

Li, Z. C. ^{[1
]}

Liu, J. C. ^{[1
]}

Liu, X. ^{[1
]}

Jin, S. J. ^{[1
]}

Wang, Y. B. ^{[1
]}

Zhang, L. Y. ^{[2
]}

Yu, X. Q. ^{[2
]}

Li, L. ^{[2
]}

Lian, G. ^{[1
]}

Fan, Q. W. ^{[1
]}

Liu, W. P. ^{[1
]}

机构：

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

[2] Chinese Acad Sci, Inst Modern Phys, Lanzhou 730000, Peoples R China

来源：

EUROPEAN PHYSICAL JOURNAL A | 2013年 / 49卷 / 08期

关键词：

D O I：

10.1140/epja/i2013-13106-8

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：

引用

页数：1

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