English

Evolutions in 3D numerical relativity using fixed mesh refinement

General Relativity and Quantum Cosmology 2010-04-06 v3

Abstract

We present results of 3D numerical simulations using a finite difference code featuring fixed mesh refinement (FMR), in which a subset of the computational domain is refined in space and time. We apply this code to a series of test cases including a robust stability test, a nonlinear gauge wave and an excised Schwarzschild black hole in an evolving gauge. We find that the mesh refinement results are comparable in accuracy, stability and convergence to unigrid simulations with the same effective resolution. At the same time, the use of FMR reduces the computational resources needed to obtain a given accuracy. Particular care must be taken at the interfaces between coarse and fine grids to avoid a loss of convergence at higher resolutions, and we introduce the use of "buffer zones" as one resolution of this issue. We also introduce a new method for initial data generation, which enables higher-order interpolation in time even from the initial time slice. This FMR system, "Carpet", is a driver module in the freely available Cactus computational infrastructure, and is able to endow generic existing Cactus simulation modules ("thorns") with FMR with little or no extra effort.

Keywords

Cite

@article{arxiv.gr-qc/0310042,
  title  = {Evolutions in 3D numerical relativity using fixed mesh refinement},
  author = {Erik Schnetter and Scott H. Hawley and Ian Hawke},
  journal= {arXiv preprint arXiv:gr-qc/0310042},
  year   = {2010}
}

Comments

20 pages, 15 figures; published version, but with colour figures