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The Future of Solar Modelling: Requirements for a New Generation of Solar Models
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A Core-sensitive Mixed f/g-mode of the Sun Predicted by Wave Topology and Hydrodynamical Simulation
Arthur Le Saux, Armand Leclerc, Guillaume Laibe, Pierre Delplace and Antoine Venaille The Astrophysical Journal Letters 987(1) L12 (2025) https://doi.org/10.3847/2041-8213/ade396
Inferring the efficiency of convective-envelope overshooting in red giant branch stars
L. Briganti, M. Tailo, E. Ceccarelli, A. Miglio, M. Matteuzzi, A. Mucciarelli, A. Mazzi, A. Bragaglia and S. Khan Astronomy & Astrophysics 700 A163 (2025) https://doi.org/10.1051/0004-6361/202553980
Mixing by internal gravity waves in stars: assessing numerical simulations against theory
J Morton, T Guillet, I Baraffe, A Morison, A Le Saux, D G Vlaykov, T Goffrey and J Pratt Monthly Notices of the Royal Astronomical Society 537(1) 154 (2025) https://doi.org/10.1093/mnras/staf010
Convective shells in the interior of Cepheid variable stars: Overshooting models based on hydrodynamic simulations
M. Stuck, J. Pratt, I. Baraffe, J. A. Guzik, M.-G. Dethero, D. G. Vlaykov, T. Goffrey and A. Le Saux Astronomy & Astrophysics 698 A304 (2025) https://doi.org/10.1051/0004-6361/202555172
Testing a non-local 1-equation turbulent convection model: A solar model
3D Hydrodynamic Simulations of Massive Main-sequence Stars. III. The Effect of Radiation Pressure and Diffusion Leading to a 1D Equilibrium Model
Huaqing Mao, Paul Woodward, Falk Herwig, Pavel A. Denissenkov, Simon Blouin, William Thompson and Benjamin McDermott The Astrophysical Journal 975(2) 271 (2024) https://doi.org/10.3847/1538-4357/ad6c4f
Equilibrium tides and magnetic activity in stars with close-by massive planets
Effects of stratification on overshooting and waves atop the convective core of M⊙ main-sequence stars
A Morison, A Le Saux, I Baraffe, J Morton, T Guillet, D G Vlaykov, T Goffrey and J Pratt Monthly Notices of the Royal Astronomical Society 532(2) 2778 (2024) https://doi.org/10.1093/mnras/stae1678
Internally heated and fully compressible convection: Flow morphology and scaling laws
The shape of convection in 2D and 3D global simulations of stellar interiors
M.-G. Dethero, J. Pratt, D. G. Vlaykov, I. Baraffe, T. Guillet, T. Goffrey, A. Le Saux and A. Morison Astronomy & Astrophysics 692 A46 (2024) https://doi.org/10.1051/0004-6361/202451814
3D hydrodynamics simulations of a 3 M⊙ core helium burning star
Simon Blouin, Falk Herwig, Huaqing Mao, Pavel Denissenkov and Paul R Woodward Monthly Notices of the Royal Astronomical Society 527(3) 4847 (2023) https://doi.org/10.1093/mnras/stad3518
3D hydrodynamics simulations of internal gravity waves in red giant branch stars
Simon Blouin, Huaqing Mao, Falk Herwig, Pavel Denissenkov, Paul R Woodward and William R Thompson Monthly Notices of the Royal Astronomical Society 522(2) 1706 (2023) https://doi.org/10.1093/mnras/stad1115
Impact of radial truncation on global 2D hydrodynamic simulations for a Sun-like model
D G Vlaykov, I Baraffe, T Constantino, et al. Monthly Notices of the Royal Astronomical Society 514(1) 715 (2022) https://doi.org/10.1093/mnras/stac1278