Exascale super-computers now becoming available rely on hybrid energy-efficient architectures that involve an accelerator such as Graphics Processing Units (GPU). Leveraging the computational power of these machines often means a significant rewrite of the numerical tools each time a new architecture becomes available. To address these issues, we present Idefix, a new code for astrophysical flows that relies on the Kokkos meta-programming library to guarantee performance portability on a wide variety of architectures while keeping the code as simple as possible for the user. Idefix is based on a Godunov finite-volume method that solves the non-relativistic HD and MHD equations on various grid geometries. Idefix includes a wide choice of sol...
We present the newly developed code, GPU-accelerated Adaptive-MEsh-Refinement code (GAMER), which ad...
This thesis documents the hydrodynamics code Cholla and a numerical study of multiphase galactic win...
Supercomputers and grid networks are the basic instruments to elaborate and test physical models inv...
International audienceExascale super-computers now becoming available rely on hybrid energy-efficien...
The paper presents a new hydrodynamical code, OMPEGAS, for the 3D simulation of astrophysical flows ...
We present Cholla (Computational Hydrodynamics On ParaLLel Architectures), a new three-dimensional h...
We present the FARGO3D code, recently publicly released. It is a magnetohydrodynamics code developed...
GPU computing is expected to play an integral part in all modern Exascale supercomputers. It is also...
With advance of supercomputers we can now afford simulations with very large range of scales. In ast...
23 pagesWe describe Graphics Processing Unit-Imogen (GPU-Imogen), an astrophysical hydrodynamics co...
We present the PLUTO code for the solution of high-Mach number flows in 1, 2 and 3 spatial dimension...
We present a new hydrodynamical code GPUPEGAS 2.0 for 3D simulation of astrophysical flows using the...
Simulations conducted on high-performance, massively parallel mainframes have become a central tool ...
We present a new 1-D multi-physics simulation code with use cases intended for, but not limited to, ...
We present a new numerical code, PLUTO, for the solution of hypersonic flows in 1, 2 and 3 spatial d...
We present the newly developed code, GPU-accelerated Adaptive-MEsh-Refinement code (GAMER), which ad...
This thesis documents the hydrodynamics code Cholla and a numerical study of multiphase galactic win...
Supercomputers and grid networks are the basic instruments to elaborate and test physical models inv...
International audienceExascale super-computers now becoming available rely on hybrid energy-efficien...
The paper presents a new hydrodynamical code, OMPEGAS, for the 3D simulation of astrophysical flows ...
We present Cholla (Computational Hydrodynamics On ParaLLel Architectures), a new three-dimensional h...
We present the FARGO3D code, recently publicly released. It is a magnetohydrodynamics code developed...
GPU computing is expected to play an integral part in all modern Exascale supercomputers. It is also...
With advance of supercomputers we can now afford simulations with very large range of scales. In ast...
23 pagesWe describe Graphics Processing Unit-Imogen (GPU-Imogen), an astrophysical hydrodynamics co...
We present the PLUTO code for the solution of high-Mach number flows in 1, 2 and 3 spatial dimension...
We present a new hydrodynamical code GPUPEGAS 2.0 for 3D simulation of astrophysical flows using the...
Simulations conducted on high-performance, massively parallel mainframes have become a central tool ...
We present a new 1-D multi-physics simulation code with use cases intended for, but not limited to, ...
We present a new numerical code, PLUTO, for the solution of hypersonic flows in 1, 2 and 3 spatial d...
We present the newly developed code, GPU-accelerated Adaptive-MEsh-Refinement code (GAMER), which ad...
This thesis documents the hydrodynamics code Cholla and a numerical study of multiphase galactic win...
Supercomputers and grid networks are the basic instruments to elaborate and test physical models inv...