The flows of phase trajectories of cosmological models based on the vacuum classical Higgs field and their behavior on the Einstein–Higgs surface near singular points of a dynamical system are investigated by numerical simulation. The influence of the singular points on the process of phase flow splitting is shown and the efficiency of the Einstein–Higgs hypersurface application is demonstrated.
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Translated from Izvestiya Vysshikh Uchebnykh Zavedenii, Fizika, No. 10, pp. 26–31, October, 2021.
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Ignat’ev, Y.G., Samigullina, A.R. Complete Cosmological Evolution Model of a Classical Scalar Field with a Higgs Potential. III. Features of Phase Trajectory Flows. Russ Phys J 64, 1808–1814 (2022). https://doi.org/10.1007/s11182-022-02529-0
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DOI: https://doi.org/10.1007/s11182-022-02529-0