Complete model of cosmological evolution of a classical scalar field with the Higgs potential. I: Analysis of the model
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Publication:1984328
DOI10.1007/s11182-021-02359-6zbMath1472.83116arXiv2108.07626OpenAlexW3183713001MaRDI QIDQ1984328
Yu. G. Ignat'ev, A. R. Samigullina
Publication date: 13 September 2021
Published in: Russian Physics Journal (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/2108.07626
Unified quantum theories (81V22) Relativistic cosmology (83F05) Model quantum field theories (81T10) Geometrodynamics and the holographic principle (83E05) Foliations (differential geometric aspects) (53C12)
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Complete cosmological evolution model of a classical scalar field with a Higgs potential. II: Numerical simulation ⋮ Complete cosmological evolution model of a classical scalar field with a Higgs potential. III: Features of phase trajectory flows
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- Peculiarities of cosmological models based on a nonlinear asymmetric scalar doublet with minimal interaction. I. Qualitative analysis
- Peculiarities of cosmological models based on a nonlinear asymmetric scalar doublet with minimal interaction. II: Numerical analysis
- Qualitative and numerical analysis of a cosmological model based on an asymmetric scalar doublet with minimal couplings. II. Numerical modeling of phase trajectories
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