We study the simulation of stellar mergers, which requires complex simulations with high computational demands. We have developed Octo-Tiger, a finite volume grid-based hydrodynamics simulation code with Adaptive Mesh Refinement which is unique in conserving both linear and angular momentum to machine precision. To face the challenge of increasingly complex, diverse, and heterogeneous HPC systems, Octo-Tiger relies on high-level programming abstractions. We use HPX with its futurization capabilities to ensure scalability both between nodes and within, and present first results replacing MPI with libfabric achieving up to a 2.8x speedup. We extend Octo-Tiger to heterogeneous GPU-accelerated supercomputers, demonstrating node-level performanc...
Turbulent flows are known for the intermittent occurrence of intense strain rates and local rotatio...
This paper concentrates on four key tools for performing star cluster simulations developed during t...
With the increase in computational power in the last decade and the forthcoming Exascale supercomput...
OCTO-TIGER is an astrophysics code to simulate the evolution of self-gravitating and rotating system...
We present a highly scalable demonstration of a portable asynchronous many-task programming model an...
Stellar mergers between two suns are a significant field of study since they can lead to astrophysic...
We present Cholla (Computational Hydrodynamics On ParaLLel Architectures), a new three-dimensional h...
We report on a very large set of simulations of collisions between two main-sequence (MS) stars. The...
This thesis documents the hydrodynamics code Cholla and a numerical study of multiphase galactic win...
Outflows and jets are an integral part of the formation of young stars and are found to be commonpla...
The main target of this work is the discussion of the modern techniques (software and hardware) apt ...
We describe PTreeSPH, a gravity treecode combined with an SPH hydrodynamics code designed for massiv...
International audienceHPC appears more and more as a key player in the field of numerical simulation...
Supercomputers and grid networks are the basic instruments to elaborate and test physical models inv...
We discuss the high performance computing issues involved in the numerical simulation of binary neut...
Turbulent flows are known for the intermittent occurrence of intense strain rates and local rotatio...
This paper concentrates on four key tools for performing star cluster simulations developed during t...
With the increase in computational power in the last decade and the forthcoming Exascale supercomput...
OCTO-TIGER is an astrophysics code to simulate the evolution of self-gravitating and rotating system...
We present a highly scalable demonstration of a portable asynchronous many-task programming model an...
Stellar mergers between two suns are a significant field of study since they can lead to astrophysic...
We present Cholla (Computational Hydrodynamics On ParaLLel Architectures), a new three-dimensional h...
We report on a very large set of simulations of collisions between two main-sequence (MS) stars. The...
This thesis documents the hydrodynamics code Cholla and a numerical study of multiphase galactic win...
Outflows and jets are an integral part of the formation of young stars and are found to be commonpla...
The main target of this work is the discussion of the modern techniques (software and hardware) apt ...
We describe PTreeSPH, a gravity treecode combined with an SPH hydrodynamics code designed for massiv...
International audienceHPC appears more and more as a key player in the field of numerical simulation...
Supercomputers and grid networks are the basic instruments to elaborate and test physical models inv...
We discuss the high performance computing issues involved in the numerical simulation of binary neut...
Turbulent flows are known for the intermittent occurrence of intense strain rates and local rotatio...
This paper concentrates on four key tools for performing star cluster simulations developed during t...
With the increase in computational power in the last decade and the forthcoming Exascale supercomput...