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# massive star | ||
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This setup models the convective burning shells in a massive star | ||
leading up to core collapse. Some details: | ||
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* The initial model is from MESA and is put onto a uniform grid using | ||
the routines in the AMReX Astrophysics initial model repo | ||
(https://github.com/amrex-astro/initial_models) in the | ||
``massive_star`` directory. | ||
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* We use simplified-SDC together with aprox19 and an NSE table | ||
(generated from pynucastro) | ||
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* The Castro ``drive_initial_convection`` functionality is used to | ||
establish the initial convective velocity field. |