  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.
