The phase evolution of the Universe during its cooling down in 2HDM

Ginzburg, I. F. and Ivanov, I. P. and Kanishev, K. A. (2010) The phase evolution of the Universe during its cooling down in 2HDM. Il nuovo cimento C, 33 (2). pp. 119-127. ISSN 1826-9885

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Abstract

Two Higgs Doublet Model at different values of parameters realizes ground state (vacuum) with different properties. The parameters of the Gibbs potential are varied during cooling down of the Universe after Big Bang. At this variation properties of vacuum state can vary, Universe suffers phase transitions. The evolution of phase states and chains of phase transitions can be much more diverse than in Standard Model with single Higgs doublet. We analyzed phase history of earlier Universe for each set of parameters and find sets of modern parameters, responsible for different chains of thermal phase transitions.

Item Type: Article
Uncontrolled Keywords: Finite-temperature field theory ; Spontaneous and radiative symmetry breaking ; Electroweak interactions ; Particle-theory and field-theory models of the early Universe (including cosmic pancakes, cosmic strings, chaotic phenomena, inflationary universe, etc.)
Subjects: 500 Scienze naturali e Matematica > 510 Matematica
Depositing User: Marina Spanti
Date Deposited: 31 Mar 2020 15:59
Last Modified: 31 Mar 2020 15:59
URI: http://eprints.bice.rm.cnr.it/id/eprint/16838

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