Abstract
We discuss the evolution of toy universes coupled to a massive scalar field. Under most initial conditions such a universe enters an inflationary phase from which it emerges naturally. When the universe is anisotropic or inhomogeneous, the anisotropy or inhomogeneity freezes during the inflationary phase.
| Original language | English |
|---|---|
| Pages (from-to) | 331-335 |
| Number of pages | 5 |
| Journal | Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics |
| Volume | 163 |
| Issue number | 5-6 |
| DOIs | |
| State | Published - 28 Nov 1985 |
| Externally published | Yes |
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