Solving Einstein's Equation Numerically on Manifolds With Arbitrary Spatial Topologies
arXiv:1312.0701 · doi:10.1103/PhysRevD.89.044044
Abstract
This paper develops a method for solving Einstein's equation numerically on multi-cube representations of manifolds with arbitrary spatial topologies. This method is designed to provide a set of flexible, easy to use computational procedures that make it possible to explore the never before studied properties of solutions to Einstein's equation on manifolds with arbitrary toplogical structures. A new covariant, first-order symmetric-hyperbolic representation of Einstein's equation is developed for this purpose, along with the needed boundary conditions at the interfaces between adjoining cubic regions. Numerical tests are presented that demonstrate the long-term numerical stability of this method for evolutions of a complicated, time-dependent solution of Einstein's equation coupled to a complex scalar field on a manifold with spatial topology S^3. The accuracy of these numerical test solutions is evaluated by performing convergence studies and by comparing the full non-linear numerical results to the analytical perturbation solutions, which are also derived here.
20 pages, 12 figures, 1 table; v2 minor revisions to agree with published version
References in corpus (6)
- High-accuracy waveforms for binary black hole inspiral, merger, and ringdown
- Solving Einstein's Equations With Dual Coordinate Frames
- An Improved Gauge Driver for the Generalized Harmonic Einstein System
- Evolution of a family of expanding cubic black-hole lattices in numerical relativity
- Outer boundary conditions for Einstein's field equations in harmonic coordinates
- Solving Partial Differential Equations Numerically on Manifolds with Arbitrary Spatial Topologies