Explore multidimensional hydrodynamical simulations and radiative transfer in white dwarf research through this 21-minute conference talk by Samuel Boos from the University of Alabama. Delivered at the "White Dwarfs from Physics to Astrophysics" conference hosted by the Kavli Institute for Theoretical Physics, delve into cutting-edge modeling techniques used to study these abundant stellar remnants. Gain insights into how advanced simulations contribute to our understanding of white dwarf formation, evolution, and their role as astrophysical probes. Discover how these computational methods enhance our ability to interpret data from all-sky surveys, providing a comprehensive view of the Galactic white dwarf population and their implications for various astrophysical phenomena.