most citedSpectral Difference method with a posteriori limiting: II- Application to low Mach number flows

2 citations · 2 across the 5 of their papers we have counts for

collaborators

5 papers

astro-ph.IM2026

RAMSES-GPU: Cell-by-Cell Adaptive Mesh Refinement with Magneto-Hydrodynamics and Self-Gravity on Graphics Processing Units

Romain Teyssier, Eric Moseley, Robert V. Caddy +9

We present the implementation and optimization of the cosmological simulation code RAMSES on Graphics Processing Units (GPUs) using CUDA Fortran. This accelerated version ports the…

astro-ph.IM2026

A Scalable Fast Multipole Method Poisson Solver for the RAMSES code: II. Adaptive Mesh Refinement and Adaptive Time Stepping

Jun-Young Lee, Romain Teyssier

We present an extended implementation of a scalable, O(N) Poisson solver based on the fast multipole method (FMM), fully compatible with adaptive mesh refinement (AMR) and adaptive…

astro-ph.IM2026

A Scalable Fast Multipole Method Poisson Solver for the RAMSES code: I. Unigrid Algorithm

Jun-Young Lee, Romain Teyssier

We present a scalable Poisson solver with complexity based on the fast multipole method (FMM) implemented in RAMSES. Our FMM constructs a hierarchy of FMM grids on top of th…

astro-ph.IM2026

Spectral Difference Method with a Posteriori Limiting: III- Navier-Stokes Equations with Arbitrary High-Order Accuracy

David A. Velasco-Romero, Romain Teyssier

We incorporate an arbitrarily high-order method for the Laplacian operator into the Spectral Difference method (SD). The resulting method is capable of capturing shocks thanks to i…

physics.flu-dyn20262 cited

Spectral Difference method with a posteriori limiting: II- Application to low Mach number flows

D. A. Velasco-Romero, R. Teyssier

Stellar convection poses two main gargantuan challenges for astrophysical fluid solvers: low-Mach number flows and minuscule perturbations over steeply stratified hydrostatic equil…