Explosive Nucleosynthesis: Coupling Reaction Networks to AMR   Hydrodynamics
  In recent years the technique of Adaptive Mesh Refinement (AMR) has been successfully applied to several astrophysical problems. This method should also allow a consistent multi-dimensional modelling of supernova explosions. In this contribution we address some of the computational difficulties encountered when trying to apply the AMR method to explosive nucleosynthesis and supernova envelope ejection. 
K. Kifonidis (MPA), T. Plewa (Copernicus Astronomical Center and MPA)   and E. Mueller (MPA)