Phlegethon: a fully compressible magnetohydrodynamic code for simulations in stellar astrophysics
PHLEGETHON is a fully compressible magnetohydrodynamic (MHD) code designed for simulating complex astrophysical phenomena within stars. It integrates advanced numerical methods, including low-dissipation Riemann solvers and well-balanced discretizations, to accurately model stellar dynamics from the main sequence through supernova progenitors. The code enables researchers to study processes like reactive convection and magnetic field amplification in diverse stellar environments using high-performance computing resources.