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Nucleosynthesis Constraints on Defect-Mediated Electroweak Baryogenesis

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arxiv astro-ph/9501040 v1 pith:7TVX3NK5 submitted 1995-01-12 astro-ph hep-ph

Robert Brandenberger (Brown Univ.) , Anne-Christine Davis (DAMTP , Univ. of Cambridge) , Martin J. Rees (Inst. of Astronomy This is my paper · ORCID
classification astro-phhep-ph
keywords electroweakbaryogenesisdefect-mediatednucleosynthesisconstraintsbaryonbaryonsconsiderations
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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.

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  1. The Bearable Inhomogeneity of the Baryon Asymmetry

    hep-ph 2025-05 conditional novelty 6.0 of 10

    BBN deuterium abundances exclude baryon-to-photon inhomogeneities above roughly 26-28% RMS, probing physics at temperatures up to a few TeV.

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