S-process nucleosynthesis in AGB stars with the full spectrum of turbulence scheme for convection.
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
Yagüe, A. et al.
Fecha de publicación:
7
2016