arXiv · gr-qc/9701019
Numerical Integration of Nonlinear Wave Equations for General Relativity
Abstract
A second-order numerical implementation is given for recently derived nonlinear wave equations for general relativity. The Gowdy T$^3$ cosmology is used as a test bed for studying the accuracy and convergence of simulations of one-dimensional nonlinear waves. The complete freedom in space-time slicing in the present formulation is exploited to compute in the Gowdy line-element. Second-order convergence is found by direct comparison of the results with either analytical solutions for polarized waves, or solutions obtained from Gowdy's reduced wave equations for the more general unpolarized waves. Some directions for extensions are discussed.
Explore related subjects
Keep this discovery
Explore connections, maps & timelines
Maurice H. P. M. van Putten. 1997-01-10. Numerical Integration of Nonlinear Wave Equations for General Relativity. https://doi.org/10.1103/physrevd.55.4705
Cite the original work for its findings. Save a collection to share your selection of sources.