GPU-accelerated 3-D finite volume particle method

DOI10.1016/j.compfluid.2018.05.030zbMath1410.65337OpenAlexW2806115898MaRDI QIDQ720988

Siamak Alimirzazadeh, Sebastián Leguizamón, François Avellan, Ebrahim Jahanbakhsh, Audrey P. Maertens

Publication date: 18 July 2018

Published in: Computers and Fluids (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1016/j.compfluid.2018.05.030

zbMATH Keywords

performance optimizationspace-filling curveGPUFVPMoctree neighbor searchroofline model

Mathematics Subject Classification ID

Finite volume methods applied to problems in fluid mechanics (76M12) Particle methods and lattice-gas methods (76M28) Numerical algorithms for specific classes of architectures (65Y10) Finite volume methods for initial value and initial-boundary value problems involving PDEs (65M08) Probabilistic methods, particle methods, etc. for initial value and initial-boundary value problems involving PDEs (65M75)

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Uses Software

• CUDA
• DualSPHysics
• AQUAgpusph
• gpuSPHASE
• SPHEROS
• OpenSHMEM

Cites Work

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• DualSPHysics: Open-source parallel CFD solver based on smoothed particle hydrodynamics (SPH)
• Development of the meshless finite volume particle method with exact and efficient calculation of interparticle area
• GPU-acceleration for moving particle semi-implicit method
• A sparse octree gravitational \(N\)-body code that runs entirely on the GPU processor
• Simulating free surface flows with SPH
• Smoothed particle hydrodynamics method for fluid flows, towards industrial applications: motivations, current state, and challenges
• AQUAgpusph, a new free 3D SPH solver accelerated with OpenCL
• gpuSPHASE -- a shared memory caching implementation for 2D SPH using CUDA
• Exact finite volume particle method with spherical-support kernels
• Development of a finite volume particle method for 3-D fluid flow simulations
• A consistent and fast weakly compressible smoothed particle hydrodynamics with a new wall boundary condition
• Smoothed particle hydrodynamics: theory and application to non-spherical stars
• Finite Volume Methods for Hyperbolic Problems

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