Heavy ion fusion reactions in stars
文献类型：会议论文
| 作者 | Tang, X. D.1,2; Cheoun, MK; Hahn, KI; Jeong, S; Kim, SC; Kwak, K; Lee, YS; Yoon, SC |
| 出版日期 | 2018 |
| 卷号 | 1947 |
| DOI | 10.1063/1.5030828 |
| 英文摘要 | Heavy ion fusion reactions play important roles in a wide variety of stellar burning scenarios. C-12+ C-12. C-12+ O-16 and O-16+O-16 are the principle reactions during the advance burning stages of massive star. C-12+C-12 also triggers the happening of superburst and Type Ia supernovae. The heavy ion fusion reactions of the neutron-rich isotopes such as O-24 are the major heating source in the crust of neutron star. In this talk, I will review the challenges and the recent progress in the study of these heavy ion fusion reactions at stellar energies. The outlook for the studies of the astrophysical heavy-ion fusion reactions will also be presented. |
| 会议录 | 14TH INTERNATIONAL SYMPOSIUM ON ORIGIN OF MATTER AND EVOLUTION OF GALAXIES (OMEG 2017)
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| 会议录出版者 | AMER INST PHYSICS |
| 会议录出版地 | 2 HUNTINGTON QUADRANGLE, STE 1NO1, MELVILLE, NY 11747-4501 USA |
| 语种 | 英语 |
| 资助项目 | National Natural Science Foundation of China[11021504] ; National Natural Science Foundation of China[11321064] ; National Natural Science Foundation of China[11475228] ; National Natural Science Foundation of China[11490564] |
| WOS研究方向 | Astronomy & Astrophysics |
| WOS记录号 | WOS:000434142300024 |
| 源URL | [http://119.78.100.186/handle/113462/58554]  |
| 专题 | 中国科学院近代物理研究所 |
| 通讯作者 | Tang, X. D. |
| 作者单位 | 1.Chinese Acad Sci, Inst Modern Phys, Lanzhou, Gansu, Peoples R China 2.Lanzhou Univ, Joint Dept Nucl Phys, Lanzhou, Gansu, Peoples R China |
| 推荐引用方式 GB/T 7714 | Tang, X. D.,Cheoun, MK,Hahn, KI,et al. Heavy ion fusion reactions in stars[C]. 见:. |
入库方式： OAI收割
来源：近代物理研究所
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