An astrophysical code for AMR & SPH on GPU clusters
Description
An general purpose code tu perform hydrodynamical simulations with various numerical methods. This code is platform agnostic, meaning that it can run on a laptop up to a multi-GPU cluster
The code works using MPI with SYCL
Status
First paper submitted to MNRAS (see Publications)
A protoplanetary disc with a planet :
Lense-thiring precesion :