Abstract
We present a dynamical mechanism for completing inflationary phase transitions via bubble nucleation which can satisfy all known constraints for a wide spectrum of models and parameters. The approach is a generalization of the recent extended inflation model which corrects a serious flaw. We find an essentially model-independent bubble-size distribution which may be important for large-scale structure.
| Original language | English (US) |
|---|---|
| Pages (from-to) | 2740-2743 |
| Number of pages | 4 |
| Journal | Physical review letters |
| Volume | 64 |
| Issue number | 23 |
| DOIs | |
| State | Published - 1990 |
| Externally published | Yes |
All Science Journal Classification (ASJC) codes
- General Physics and Astronomy