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 :