Solar s-process contributions with GCE model
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https://b2find.eudat.eu/dataset/ee6ed563-e4b5-5b98-9d0a-49e393a82123
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We study the s-process abundances (A>~90) at the epoch of the solar system formation. Asymptotic giant branch yields are computed with an updated neutron capture network and...
本研究针对太阳系形成时期的慢中子俘获过程(s-process)元素丰度(原子量A>约90)展开分析。研究采用更新后的中子俘获网络,对渐近巨星支(Asymptotic Giant Branch, AGB)恒星的元素产额进行计算,并……



