To learn numerical simulations for modeling gamma-ray bursts, foundational knowledge in stellar structure equations is essential, typically covered in undergraduate astrophysics courses. While MATLAB can be used for basic modeling of stars in hydrostatic equilibrium, more complex simulations, especially for stellar collapse, require advanced codes. MESA, a FORTRAN-based code, is recommended for beginners to explore stellar evolution, though it has limitations for simulating supernovae. For more complex events, including three-dimensional simulations, codes like FLASH may be necessary. Starting with MESA provides a solid foundation before tackling more advanced simulations.