中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
The beta-decay rates of Fe-59 isotopes in shell burning environments and their influences on the production of Fe-60 in massive star

文献类型:会议论文

作者Li, K.1; Lam, Y. H.1; Qi, C.2; Tang, X.1; Zhang, N.1; Liu, WP; Li, ZH; Wang, YB; Guo, B; Shen, YP
出版日期2016
卷号109
DOI10.1051/epjconf/201610904006
英文摘要The experimental B(GT) strengths of the Fe-59 excited states were employed to determine the transition strengths which greatly contribute Fe-59 stellar beta-decay at typical carbon shell burning temperature. The result has been compared with the theoretical rates FFN (Fuller-Fowler-Newman) and LMP (Langanke&Martinez-Pinedo). Impact of the newly determined rate on the synthesis of cosmic gamma-emitter 60Fe has also been studied using one-zone model calculation. Our results show Fe-59 stellar beta-decay rate plays an important role in the Fe-60 nucleosynthesis. However the uncertainty of the decay rate is rather large due to the error of B(GT) strength that requires further studies.
会议录13TH INTERNATIONAL SYMPOSIUM ON ORIGIN OF MATTER AND EVOLUTION OF GALAXIES (OMEG2015)
会议录出版者E D P SCIENCES
会议录出版地17 AVE DU HOGGAR PARC D ACTIVITES COUTABOEUF BP 112, F-91944 CEDEX A, FRANCE
语种英语
WOS研究方向Astronomy & Astrophysics
WOS记录号WOS:000372789800010
源URL[http://119.78.100.186/handle/113462/57747]  
专题中国科学院近代物理研究所
通讯作者Li, K.
作者单位1.Chinese Acad Sci, Inst Modern Phys, Lanzhou 730000, Peoples R China
2.Royal Inst Technol, Dept Phys, S-10044 Stockholm, Sweden
推荐引用方式
GB/T 7714
Li, K.,Lam, Y. H.,Qi, C.,et al. The beta-decay rates of Fe-59 isotopes in shell burning environments and their influences on the production of Fe-60 in massive star[C]. 见:.

入库方式: OAI收割

来源:近代物理研究所

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