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- W3180348243 abstract "Current AGB stellar models provide an adequate description of the s-process nucleosynthesis that occurs. Nonetheless, they still suffer from many uncertainties related to the modeling of the 13C pocket formation and the adopted nuclear reaction rates. For many important s-process isotopes, a best set of neutron-capture cross sections was recently re-evaluated. Using stellar models prescribing that the 13C pocket is a by-product of magnetic-buoyancy-induced mixing phenomena, s-process calculations were carried out with this database. Significant effects are found for a few s-only and branching point isotopes, pointing out the need for improved neutron-capture cross section measurements at low energy." @default.
- W3180348243 created "2021-07-19" @default.
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- W3180348243 date "2021-07-11" @default.
- W3180348243 modified "2023-10-17" @default.
- W3180348243 title "s-Processing in Asymptotic Giant Branch Stars in the Light of Revised Neutron-Capture Cross Sections" @default.
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- W3180348243 doi "https://doi.org/10.3390/universe7070239" @default.
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