Electroweak phase transition in the early universe?

Existence and properties of the electroweak phase transition in the early universe depend strongly on the mass of the Higgs scalar MH. There is presumably no true symmetry restoration at high temperature. Nevertheless, a first order phase transition occurs in the standard model for MH ≲ GeV. For a r...

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Bibliographic Details
Main Authors: Bergerhoff, Bastian (Author) , Wetterich, Christof (Author)
Format: Chapter/Article Conference Paper
Language:English
Published: 1998
In: Current topics in astrofundamental physics
Year: 1998, Pages: 211-240
DOI:10.1007/978-94-011-5046-0_6
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Online Access:Verlag, Volltext: http://dx.doi.org/10.1007/978-94-011-5046-0_6
Verlag, Volltext: https://link.springer.com/chapter/10.1007/978-94-011-5046-0_6
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Author Notes:Bastian Bergerhoff and Christof Wetterich
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Electroweak phase transition in the early universe? by Bergerhoff, Bastian (Author) , Wetterich, Christof (Author) ,


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