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 Uncertaities due to convection and production of s-nuclei in massive stars


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We have investigated the role of the convective overshooting on the production of s-nuclei during core He-burning phase in stellar models with different initial mass and metallicity $15 \leq M {ZAMS}-M {\odot} \leq 25$; $10^{-4} \leq Z \leq 0.02$, considering a diffusive approach to model the convective overshooting. The results and their possible consequences on some open questions linked to the s-process weak component efficiency are discussed.



Autor: M. L. Pumo; G. Contino; A. Bonanno; R. A. Zappalà

Fuente: https://archive.org/







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