A Direct Multigrid Poisson Solver for Oct-Tree Adaptive Meshes
arXiv:0710.4397 · doi:10.1086/526425
Abstract
We describe a finite-volume method for solving the Poisson equation on oct-tree adaptive meshes using direct solvers for individual mesh blocks. The method is a modified version of the method presented by Huang and Greengard (2000), which works with finite-difference meshes and does not allow for shared boundaries between refined patches. Our algorithm is implemented within the FLASH code framework and makes use of the PARAMESH library, permitting efficient use of parallel computers. We describe the algorithm and present test results that demonstrate its accuracy.
10 pages, 6 figures, accepted by the Astrophysical Journal; minor revisions in response to referee's comments; added charm
References in corpus (11)
- Cosmological Hydrodynamics with Adaptive Mesh Refinement: a new high resolution code called RAMSES
- Adaptive Refinement Tree - a new high-resolution N-body code for cosmological simulations
- Divergence-Free Adaptive Mesh Refinement for Magnetohydrodynamics
- MLAPM - a C code for cosmological simulations
- Robustness of Cosmological Simulations I: Large Scale Structure
- A High-resolution Adaptive Moving Mesh Hydrodynamic Algorithm
- Block Structured Adaptive Mesh and Time Refinement for Hybrid, Hyperbolic + N-body Systems
- A Fast Algorithm for Solving the Poisson Equation on a Nested Grid
- AMRA: An Adaptive Mesh Refinement Hydrodynamic Code for Astrophysics
- COSMOS: A Hybrid N-Body/Hydrodynamics Code for Cosmological Problems
- Out-of-Core Hydrodynamic Simulations for Cosmological Applications
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