Abstract
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.
- Received 27 September 1994
DOI:https://doi.org/10.1103/PhysRevD.51.1563
©1995 American Physical Society
