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Table A.1.
Main physical ingredients used in the Cesam2k20 models computed for this work.
| Initial chemical composition | Reference solar chemical composition of Asplund et al. (2009). |
|---|---|
| Convection | Mixing-Length Theory formalism (Böhm-Vitense 1958; Henyey et al. 1965). |
| Atmosphere | Reconstructed from a Hopf T(τ) relation (Hubeny & Mihalas 2014). |
| Opacity | Opacity tables from the OPAL team (Rogers & Iglesias 1992; Iglesias & Rogers 1996; Rogers & Nayfonov 2002), adapted to our choice of chemical composition and supplemented at low temperatures by the Wichita opacity tables (Ferguson et al. 2005). |
| Equation of state | Tabulated by the same collaboration (OPAL5, Rogers & Nayfonov 2002). |
| Nuclear reaction rate | Compilations from NACRE (Aikawa et al. 2006, except LUNA for the 14N(p, γ)15O reaction; Broggini et al. 2018). |
| Transport of chemical elements | Neglected. |
| Transport of angular momentum | Prescription of (Talon et al. 1997) with shear-induced turbulence modeled following Mathis et al. (2018). Convective zone are supposed to rotate as solid body. |
| Angular momentum loss | Scaling relation of Matt et al. (2015). |
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