Published February 18, 2025 | Version v1
Model Open

Calibrating chemical mixing induced by internal gravity waves based on hydrodynamical simulations

  • 1. Université Toulouse III - Paul Sabatier
  • 2. ROR icon CEA Paris-Saclay - Etablissement de Saclay
  • 3. ROR icon CEA Paris-Saclay
  • 4. ROR icon Newcastle University

Description

Computational setup of Mombarg, Varghese & Ratnasingam (2025, A&A). Following items are included:

  • inlist_template_IGWmix: MESA r24.03.1 inlist used for non-rotating models with internal gravity wave (IGW) mixing included.

  • inlist_template_IGWrot: MESA r24.03.1 inlist used for rotating models without IGW mixing included.

  • run_star_extras: MESA implementation to compute the chemical diffusion coefficient predicted from IGW mixing (parameter A should set in inlist)

  • MESA_models_MVR2024.zip: computed MESA models as presented in the paper. 
    Example of file naming, M3_O0.0_Z0.02_fov0.02_nodiff_IGWmix_massloss_m-correction_4-14uHz_mmax1_A1d-3: 3Msun, 0% initial critical rotation, metallicity 0.02 (mass fraction), exponential overshoot f_ov = 0.02, IGW frequencies 4 to 14 uHz with m_max =1, constant A = 10^-3.

Files

MESA_models_MVR2024.zip

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Additional details

Funding

European Research Council
4D-STAR 101071505
Agence Nationale de la Recherche
MASSIF ANR-21-CE31-0018- 02
Science and Technology Facilities Council
ST/W001020/1