Heavy ion fusion reactions in stars

doi:10.1063/1.5030828

	Heavy ion fusion reactions in stars
	Yoon, SC ; Tang, X. D.1,2; Cheoun, MK ; Hahn, KI ; Jeong, S ; Kim, SC ; Kwak, K ; Lee, YS
	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)
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
内容类型	会议论文
源URL	[http://119.78.100.186/handle/113462/58553]
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	Yoon, SC,Tang, X. D.,Cheoun, MK,et al. Heavy ion fusion reactions in stars[C]. 见:.