SPH-EXA: Enhancing the Scalability of SPH codes Via an Exascale-Ready SPH Mini-App
@article{Guerrera2019SPHEXAET, title={SPH-EXA: Enhancing the Scalability of SPH codes Via an Exascale-Ready SPH Mini-App}, author={Danilo Guerrera and Aur{\'e}lien Cavelan and Rub{\'e}n M. Cabez{\'o}n and David Imbert and Jean-Guillaume Piccinali and Ali Mohammed and Lucio Mayer and Darren S. Reed and Florina M. Ciorba}, journal={ArXiv}, year={2019}, volume={abs/1905.03344} }
Numerical simulations of fluids in astrophysics and computational fluid dynamics (CFD) are among the most computationally-demanding calculations, in terms of sustained floating-point operations per second, or FLOP/s. It is expected that these numerical simulations will significantly benefit from the future Exascale computing infrastructures, that will perform 10^18 FLOP/s. The performance of the SPH codes is, in general, adversely impacted by several factors, such as multiple time-stepping…
References
SHOWING 1-10 OF 44 REFERENCES
Towards a Mini-App for Smoothed Particle Hydrodynamics at Exascale
- Computer Science2018 IEEE International Conference on Cluster Computing (CLUSTER)
- 2018
This work extrapolates the common basic SPH features in the three codes for the purpose of consolidating them into a pure-SPH, Exascale-ready, optimized, mini-app, serving as direct feedback to the parent codes, to improve their performance and overall scalability.
SPHYNX: an accurate density-based SPH method for astrophysical applications
- Physics
- 2016
Hydrodynamical instabilities and shocks are ubiquitous in astrophysical scenarios. Therefore, an accurate numerical simulation of these phenomena is mandatory to correctly model and understand many…
Equalizing resolution in smoothed-particle hydrodynamics calculations using self-adaptive sinc kernels
- Physics
- 2014
Context. The smoothed-particle hydrodynamics (SPH) technique is a numerical method for solving gas-dynamical problems. It has been applied to simulate the evolution of a wide variety of astrophysical…
Fundamental differences between SPH and grid methods
- Physics
- 2006
We have carried out a comparison study of hydrodynamical codes by investigating their performance in modelling interacting multiphase fluids. The two commonly used techniques of grid and smoothed…
A test suite for quantitative comparison of hydrodynamic codes in astrophysics
- Physics
- 2008
We test four commonly used astrophysical simulation codes, enzo, flash, gadget and hydra, using a suite of numerical problems with analytic initial and final states. Situations similar to the…
Adaptive techniques for clustered N-body cosmological simulations
- Computer Science
- 2014
This paper presents the parallel design of ChaNGa and address many challenges arising due to the high dynamic ranges of clustered datasets, and proposes optimizations based on adaptive techniques.
Core-collapse supernovae in the hall of mirrors
- PhysicsAstronomy & Astrophysics
- 2018
Context. Modeling core-collapse supernovae (SNe) with neutrino transport in three dimensions (3D) requires tremendous computing resources and some level of approximation. We present a first…
SPH accuracy improvement through the combination of a quasi-Lagrangian shifting transport velocity and consistent ALE formalisms
- PhysicsJ. Comput. Phys.
- 2016
MiniGhost: A Miniapp for Exploring Boundary Exchange Strategies Using Stencil Computations in Scientific Parallel Computing
- Computer Science
- 2012
This report describes miniGhost, a miniapp designed for exploration of the capabilities of current as well as emerging and future architectures within the context of current and future architecture applications, and joins the suite of miniapps developed as part of the Mantevo project.