Nucleosynthesis Constraints on Defect-Mediated Electroweak Baryogenesis
arXiv:astro-ph/9501040 · doi:10.1016/0370-2693(95)00272-M
Abstract
In the defect-mediated electroweak baryogenesis scenario, baryons are produced in well separated regions of space. It is shown that between the electroweak phase transition at a temperature of $T \sim 100 {\rm GeV}$ and the end of nucleosynthesis at $T \sim 1 {\rm KeV}$ the baryon inhomogeneities dissipate, and that no constraints on defect-mediated electroweak baryogenesis can be derived from considerations of inhomogeneous nucleosynthesis.
11 pages, uses TEX