Inhomogeneous Inflation: Numerical Evolution

Preprint

15 June 1993

preprint
Published by arXiv in arXiv

https://doi.org/10.48550/arXiv.astro-ph/9306009

Abstract

We describe our 3-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.

Keywords

INHOMOGENEOUS INFLATION
STRONGLY INHOMOGENEOUS
DIMENSIONAL NUMERICAL
NUMERICAL RELATIVITY
NUMERICAL EVOLUTION
PERTURBATION THEORY
CODE

All Related Versions

Version 1, 1993-06-15, ArXiv
Published version: Physical Review D, 48 (8), 3611.

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