Conditions for inflation in an initially inhomogeneous universe

Details Conditions for inflation in an initially inhomogeneous universe Conditions for inflation in an initially inhomogeneous universe

1994-09-27

arxiv.org/abs/gr-qc/9409056v1

Phys.Rev. D51 (1995) 1563-1568

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

9 pages, plain Tex, gr-qc/yymmnnn

Scientific paper

10.1103/PhysRevD.51.1563

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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