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321D (WP2)

SHYNE will use 3D hydrodynamics simulations to improve the treatment of rotation and convection used in 1D stellar evolution models.
Convection and convective boundary mixing
Multi-D models of the dynamical shear instability in a 20 solar mass star (Edelmann et al 2016, in prep.) using the SLH hydrodynamics code (Miczek, F.; Röpke, F. K.; Edelmann, P. V. F., 2015, A&A, 576A, 50M)
Relevant literature
Relevant papers