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


Download the code

On Github : Link


Documentation

Shamrock documentation : Link

C++ API documentation : Link

Python module documentation : Link


Status

First paper accepted in MNRAS (see Publications)


Exemple of simulations

A protoplanetary disc with a planet :
Lense-thiring precesion :