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• W4386431906 endingPage "3571" @default.
• W4386431906 startingPage "3537" @default.
• W4386431906 abstract "The slow neutron-capture process (s process) contributes to the production of roughly half of the elements heavier than iron. The main component of the s process takes place in the late phases (AGB phase) of low-mass stars and is the topic of most reviews on the s process. This review thus focuses on the weak s process taking place in massive stars with a special emphasis on the key role of rotation as well as key stellar and nuclear uncertainties. While the weak s process production at solar metallicity is limited to the first peak (Sr), rotation-induced mixing boosts this production at low metallicities to the second peak (Ba) and in extreme cases to the third peak (Pb). Rotation-boosted s process also opens the door to an enhanced production of p nuclei compared to classical non-rotating massive star model predictions." @default.
• W4386431906 created "2023-09-05" @default.
• W4386431906 creator A5008503083 @default.
• W4386431906 date "2023-01-01" @default.
• W4386431906 modified "2023-09-30" @default.
• W4386431906 title "Slow Neutron-Capture Process in Evolved Stars" @default.
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