Fast Electroweak Symmetry Breaking and Cold Electroweak Baryogenesis
arXiv:1005.0752 · doi:10.1088/1475-7516/2010/09/019
Abstract
We construct a model for delayed electroweak symmetry breaking that takes place in a cold Universe with T<<100 GeV and which proceeds by a fast quench rather than by a conventional, slow, phase transition. This is achieved by coupling the Standard Model Higgs to an additional scalar field. We show that the quench transition can be made fast enough for successful Cold Electroweak Baryogenesis, while leaving known electroweak physics unchanged.
13 pages, 5 figures. Section and extra checks added, conclusions unchanged. Published version
References in corpus (5)
Cited by in corpus (13)
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- Simulations of Cold Electroweak Baryogenesis: Finding the optimal quench time
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- Simulations of Cold Electroweak Baryogenesis: Dependence on the source of CP-violation
- The Electroweak Vacuum Angle at Finite Temperature and Implications for Baryogenesis