Abstract
In the early Universe, the relative abundance of a massive weakly interacting particle species "freezes out" when the annihilation rate becomes less than the expansion rate. Although ineffective in reducing the total number of the species, occasional annihilations still occur after freeze-out. The residual annihilations of massive particles () after primordial nucleosynthesis can strongly alter the light-element abundances through photodissociation. For particles with typical weak-interaction cross sections and lifetimes sec, we find that the mass range GeV is ruled out, independent of how they subsequently decay.
- Received 11 September 1989
DOI:https://doi.org/10.1103/PhysRevD.41.3080
©1990 American Physical Society