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A Smoothed Particle Hydrodynamics Mini-App for Exascale

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arxiv 2005.02656 v1 pith:RNQPFUY5 submitted 2020-05-06 cs.CE

classification cs.CE
keywords mini-appsph-exaexascaleparticlesacceleratorastrophysicshybridhydrodynamics
verification ladder T0 review T1 audit T2 compute T3 formal
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The Smoothed Particles Hydrodynamics (SPH) is a particle-based, meshfree, Lagrangian method used to simulate multidimensional fluids with arbitrary geometries, most commonly employed in astrophysics, cosmology, and computational fluid-dynamics (CFD). It is expected that these computationally-demanding numerical simulations will significantly benefit from the up-and-coming Exascale computing infrastructures, that will perform 10 18 FLOP/s. In this work, we review the status of a novel SPH-EXA mini-app, which is the result of an interdisciplinary co-design project between the fields of astrophysics, fluid dynamics and computer science, whose goal is to enable SPH simulations to run on Exascale systems. The SPH-EXA mini-app merges the main characteristics of three state-of-the-art parent SPH codes (namely ChaNGa, SPH-flow, SPHYNX) with state-of-the-art (parallel) programming, optimization, and parallelization methods. The proposed SPH-EXA mini-app is a C++14 lightweight and flexible header-only code with no external software dependencies. Parallelism is expressed via multiple programming models, which can be chosen at compilation time with or without accelerator support, for a hybrid process+thread+accelerator configuration. Strong and weak-scaling experiments on a production supercomputer show that the SPH-EXA mini-app can be efficiently executed with up 267 million particles and up to 65 billion particles in total on 2,048 hybrid CPU-GPU nodes.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. An energy approach to pulsar-disc interaction: disc stability and implications for transitional millisecond pulsars

    astro-ph.HE 2025-05 conditional novelty 5.0 of 10

    Axisymmetric SPH-MHD simulations show accretion discs around oblique millisecond pulsars are disrupted when the inner disc radius lies well beyond the light cylinder, confirming the Ekşi and Alpar stability diagram.

  2. Cosmological Simulations of Galaxies

    astro-ph.GA 2025-07 unverdicted

    A comprehensive introductory review of cosmological galaxy simulation methods, covering initial conditions, numerical solvers, star formation and feedback, analysis, and validation.

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