Spectroscopic factors for low-lying N-16 levels and the astrophysical N-15(n,gamma)N-16 reaction rate

doi:10.1103/PhysRevC.89.012801

	Spectroscopic factors for low-lying N-16 levels and the astrophysical N-15(n,gamma)N-16 reaction rate
	Guo, B.1; Li, Z. H.1; Li, Y. J.1; Su, J.1; Pang, D. Y.2,3; Yan, S. Q.1; Wu, Z. D.1; Li, E. T.4; Bai, X. X.1; Du, X. C.1
刊名	PHYSICAL REVIEW C
	2014-01-27
卷号	89
ISSN号	0556-2813
DOI	10.1103/PhysRevC.89.012801
文献子类	Article
英文摘要	Background: Fluorine is a key element for nucleosynthetic studies since it is extremely sensitive to the physical conditions within stars. The astrophysical site to produce fluorine is suggested to be asymptotic giant branch stars. In these stars the N-15(n,gamma)N-16 reaction could affect the abundance of fluorine by competing with N-15(alpha,gamma)F-19.
资助项目	973 program of China[2013CB834406]
WOS关键词	ASYMPTOTIC GIANT BRANCH ; 1P SHELL ; DWBA ANALYSIS ; LIGHT NUCLEI ; AGB STARS ; S-PROCESS ; FLUORINE ; NUCLEOSYNTHESIS ; F-19 ; UNCERTAINTIES
WOS研究方向	Physics
语种	英语
出版者	AMER PHYSICAL SOC
WOS记录号	WOS:000332157900002
内容类型	期刊论文
源URL	[http://119.78.100.186/handle/113462/49569]
专题	中国科学院近代物理研究所
通讯作者	Guo, B.
作者单位	1.China Inst Atom Energy, Beijing 102413, Peoples R China 2.Beihang Univ, Sch Phys & Nucl Energy Engn, Beijing 100191, Peoples R China 3.Beihang Univ, Int Res Ctr Nucl & Particles Cosmos, Beijing 100191, Peoples R China 4.Shenzhen Univ, Coll Phys Sci & Technol, Shenzhen 518060, Peoples R China 5.Chinese Acad Sci, Inst Modern Phys, Lanzhou 730000, Peoples R China
推荐引用方式 GB/T 7714	Guo, B.,Li, Z. H.,Li, Y. J.,et al. Spectroscopic factors for low-lying N-16 levels and the astrophysical N-15(n,gamma)N-16 reaction rate[J]. PHYSICAL REVIEW C,2014,89.
APA	Guo, B..,Li, Z. H..,Li, Y. J..,Su, J..,Pang, D. Y..,...&Liu, W. P..(2014).Spectroscopic factors for low-lying N-16 levels and the astrophysical N-15(n,gamma)N-16 reaction rate.PHYSICAL REVIEW C,89.
MLA	Guo, B.,et al."Spectroscopic factors for low-lying N-16 levels and the astrophysical N-15(n,gamma)N-16 reaction rate".PHYSICAL REVIEW C 89(2014).