Electroweak Baryogenesis with Electroweak Strings
arXiv:astro-ph/9206001 · doi:10.1016/0370-2693(93)90604-G
Abstract
If stable electroweak strings are copiously produced during the electroweak phase transition, they may contribute significantly to the presently observed baryon to entropy ratio of the Universe. This analysis establishes the feasibility of implementing an electroweak baryogenesis scenario without a first order phase transition.
BROWN-HET-862, 12 pages; use phyzzx
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Cited by in corpus (55)
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- N=1 Supersymmetric Cosmic Strings
- Fermions Destabilize Electroweak Strings
- Doppelganger defects
- Cosmic Strings and Electroweak Baryogenesis
- Formation of Topological Defects at First Order Phase Transitions
- Local and Nonlocal Defect-Mediated Electroweak Baryogenesis
- The formation rate of semilocal strings
- Non-Abelian strings and domain walls in two Higgs doublet models
- Stabilization of Embedded Defects by Plasma Effects
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- Stabilization of the Electroweak Z String in the Early Universe
- The Dirac Sea Contribution To The Energy Of An Electroweak String
- Stability of an electroweak string with a fermion condensate
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- Topologically Stable Z - Strings in the Supersymmetric Standard Model
- Baryogenesis from Domain Walls in the Next-to-Minimal Supersymmetric Standard Model
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- Stable -strings with topological polarization in two Higgs doublet model
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