Abstract
We discuss the formation of nontopological solitons in a second-order phase transition in the early Universe. Ratios of dimensionless coupling constants in the Lagrangean determine their abundance and mass. For a large range of parameters, nontopological solitons can be cosmologically significant, contributing a significant fraction of the present mass density of the Universe.
- Received 20 January 1988
DOI:https://doi.org/10.1103/PhysRevLett.60.2101
©1988 American Physical Society