Abstract
We describe our three-dimensional numerical relativity code for the evolution of inhomogeneous cosmologies. During the evolution, the constraint equations are monitored but not solved. The code has been tested against perturbation theory with good results. We present some runs of inhomogeneous inflation with strongly inhomogeneous initial data.
- Received 24 May 1993
DOI:https://doi.org/10.1103/PhysRevD.48.3611
©1993 American Physical Society