S-process nucleosynthesis in AGB stars with the full spectrum of turbulence scheme for convection.

Bibcode
2016JPhCS.728g2004Y
DOI
10.1088/1742-6596/728/7/072004
Yagüe, A.; García-Hernández, D. A.; Ventura, P.; Lugaro, M.
Bibliographical reference

Journal of Physics: Conference Series, Volume 728, Issue 7, article id. 072004 (2016).

Advertised on:
7
2016
Number of authors
4
IAC number of authors
2
Citations
0
Refereed citations
0
Description
The chemical evolution of asymptotic giant branch (AGB) stars models depends greatly on the input physics (e.g. convective model, mass loss recipe). Variations of hot bottom burning (HBB) strength, or third dredge-up (TDU) efficiency are among the main consequences of adopting different input physics in the AGB models. The ATON evolutionary code stands apart from others in that it uses the Full Spectrum of Turbulence convective model. Here we present the first results of a newly developed s-process nucleosynthesis module for ATON AGB models. Our results are compared also with observations and theoretical predictions of present AGB nucleosynthesis models using different input physics.
Type
Non-refereed

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