Conditions for inflation in an initially inhomogeneous universe

Dalia S. Goldwirth; Nathalie Deruelle

Conditions for inflation in an initially inhomogeneous universe

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arxiv gr-qc/9409056 v1 pith:4TFESJPD submitted 1994-09-27 gr-qc astro-ph

Nathalie Deruelle , Dalia S. Goldwirth This is my paper · ORCID

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keywords inflationuniversebeforebig-bangconditionsdriveneinsteinequations

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Using a long wavelength iteration scheme to solve Einstein's equations near the Big-Bang singularity of a universe driven by a massive scalar field, we find how big initial quasi-isotropic inhomogeneities can be before they can prevent inflation to set in.

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