Review of MHD numerical methods for star formation, covering discretization techniques, divergence-free constraints, sink particles, and non-ideal effects like diffusion and the Hall effect.
A fast, robust, and simple implicit method for adaptive time-stepping on adaptive mesh-refinement grids.Astronomy and Astrophysics 563 (2014) A11
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Numerical Methods for Simulating Star Formation
Review of MHD numerical methods for star formation, covering discretization techniques, divergence-free constraints, sink particles, and non-ideal effects like diffusion and the Hall effect.