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Experimental Study of Key Nuclear Reaction 18O(α,γ)22Ne in Evolution of Massive AGB Star

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文献出处
Annual Report of China Institute of Atomic Energy  2016年00期
机 构
Department,of,Nuclear,Physics
论文摘要

About a half of the abundances of elements heavier than iron comes from the so-called slowneutron capture process(s-process).Asymptotic giant branch(AGB)stars provide the most important place for s-process to take place with the

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