Principal Investigator:
Frederic Bournaud
, CEA Saclay (France)
HPC Platform used:
SuperMUC of LRZ
Local Project ID:
pr86di
Numerical simulations are a crucial tool to understand the physics of gas turbulence and star formation: there is no analytic theory. More than six decades of spatial scales need to be described, which is best done with "adaptive resolution" codes on supercomputers.
