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.
- Received 16 February 1990
DOI:https://doi.org/10.1103/PhysRevLett.64.2740
©1990 American Physical Society