Peculiarities of cosmological models based on a nonlinear asymmetric scalar doublet with minimal interaction. I. Qualitative analysis

DOI10.1134/S0202289319010055zbMath1426.83050OpenAlexW2930782697MaRDI QIDQ2320503

Yu. G. Ignat'ev, I. A. Kokh

Publication date: 23 August 2019

Published in: Gravitation \& Cosmology (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1134/s0202289319010055

zbMATH Keywords

cosmological modelsphantom scalar fields

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Dynamical systems in other branches of physics (quantum mechanics, general relativity, laser physics) (37N20) Exact solutions to problems in general relativity and gravitational theory (83C15)

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The self-consistent field method and macroscopic Einstein equations for the early universe ⋮ A complete model of cosmological evolution of a scalar field with Higgs potential and Euclidean cycles ⋮ Physical characteristics of free oscillations of scalar fields with zero effective energy and Euclidean cycles in cosmological models ⋮ Short-wave approximation for macroscopic cosmology with Higgs scalar field ⋮ Complete model of cosmological evolution of a classical scalar field with the Higgs potential. I: Analysis of the model ⋮ Cosmological evolution of a scalar-charged degenerate cosmological plasma with Higgs scalar fields ⋮ Complete cosmological model based on an asymmetric scalar Higgs doublet ⋮ Energy-based approach to Euclidean cycles in cosmological models based on scalar fields ⋮ Cosmological models based on a statistical system of scalar charged degenerate fermions and an asymmetric Higgs scalar doublet ⋮ Cosmological evolution of a statistical system of degenerate scalarly charged fermions with an asymmetric scalar doublet. I: two-component system of assorted charges ⋮ Phase flows in the complete model of cosmological evolution of the asymmetric scalar Higgs doublet\(^\sharp\)

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