Inhomogeneous Inflation: Numerical Evolution

Details Inhomogeneous Inflation: Numerical Evolution Inhomogeneous Inflation: Numerical Evolution

1993-06-15

arxiv.org/abs/astro-ph/9306009v1

Phys.Rev. D48 (1993) 3611-3624

Astronomy and Astrophysics

Astrophysics

18 pages, 20 figures available on request, plain TeX, HU-TFT-93-31

Scientific paper

10.1103/PhysRevD.48.3611

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.

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