Three-dimensional hydrodynamic simulations of deep convection in massive stars
Thesis
Cristini, A. (2017). Three-dimensional hydrodynamic simulations of deep convection in massive stars
Convection plays a key role in the evolution of massive stars. Despite many decades of work on this topic, the treatment of convection (convective boundary mixing in particular) is still one of the major uncertainties in stellar evolution modelling.... Read More about Three-dimensional hydrodynamic simulations of deep convection in massive stars.