Nucleosynthesis Constraints on Defect-Mediated Electroweak Baryogenesis

Details Nucleosynthesis Constraints on Defect-Mediated Electroweak Baryogenesis Nucleosynthesis Constraints on Defect-Mediated Electroweak Baryogenesis

1995-01-12

arxiv.org/abs/astro-ph/9501040v1

Phys.Lett.B349:329-334,1995

Astronomy and Astrophysics

Astrophysics

11 pages, uses TEX

Scientific paper

10.1016/0370-2693(95)00272-M

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.

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