Speaker
Bruno Peres
Description
The M1 scheme aimed at neutrino treatment in core collapse supernovae codes has numerous advantages. It is a good tradeoff between computational cost and accuracy. The M1 equations are hyperbolic, making it perfectly suitable for GR, and a part of the equations can be treated explicitely. I will show an implementation of the M1 in the CoCoNuT code, along with possibilities of future works in CoCoNuT.
