Introducing two improved methods for approximating radiative cooling in hydrodynamical simulations of accretion discs

Introducing two improved methods for approximating radiative cooling in hydrodynamical simulations of accretion discspubhttps://doi.org/10.1093/mnras/stae1249https://clok.uclan.ac.uk/51463/Phantom Smoothed Particle Hydrodynamics and Magnetohydrodynamics codeds_exthttps://github.com/alisonkyoung1/phantom