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
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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). |
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