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3D simulations of a neon burning convective shell in a massive star
C Georgy, F Rizzuti, R Hirschi, V Varma, W D Arnett, C Meakin, M Mocak, A StJ Murphy and T Rauscher Monthly Notices of the Royal Astronomical Society 531(4) 4293 (2024) https://doi.org/10.1093/mnras/stae1381
Towards a self-consistent model of the convective core boundary in upper main sequence stars
3D stellar evolution: hydrodynamic simulations of a complete burning phase in a massive star
F Rizzuti, R Hirschi, W D Arnett, C Georgy, C Meakin, A StJ Murphy, T Rauscher and V Varma Monthly Notices of the Royal Astronomical Society 523(2) 2317 (2023) https://doi.org/10.1093/mnras/stad1572
The impact of convective criteria on the properties of massive stars
Realistic 3D hydrodynamics simulations find significant turbulent entrainment in massive stars
F Rizzuti, R Hirschi, C Georgy, W D Arnett, C Meakin and A StJ Murphy Monthly Notices of the Royal Astronomical Society 515(3) 4013 (2022) https://doi.org/10.1093/mnras/stac1981
Numerical experiments to help understand cause and effect in massive star evolution
Eoin Farrell, Jose H Groh, Georges Meynet and J J Eldridge Monthly Notices of the Royal Astronomical Society 512(3) 4116 (2022) https://doi.org/10.1093/mnras/stac538
Dynamics in a stellar convective layer and at its boundary: Comparison of five 3D hydrodynamics codes