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A Complete Model of Cosmological Evolution of Scalar Field with Higgs Potential and Euclidian Cycles

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arxiv 2005.14010 v1 pith:HPOJW35C submitted 2020-05-28 gr-qc

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keywords beenhiggsmodelscalarsystemcasescompletecosmological
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The revision of the Author's results with respect to possibility of existence of the so-called Euclidian cycles in cosmological evolution of a system of Higgs scalar fields has been performed. The assumption of non-negativity of the Universe's extension velocity, which contradicts in certain cases to complete system of Einstein equations, has been removed. It has been shown that in cases when effective energy of the system tends to zero, a smooth transition of the model to the range of negative values of the extension velocity occurs, i.e. it occurs the transition to collapse stage rather than winding of the phase trajectories on the boundary of prohibited area. This process has been researched with a help of numerical simulation methods for the model based on classical scalar Higgs field.

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Cited by 1 Pith paper

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  1. Cosmological dynamics based on Lovelock's gravity. Qualitative analysis

    gr-qc 2026-08 conditional novelty 5.0 of 10

    For flat FRW universes in Lovelock gravity, the dynamics reduces to a single first-order ODE whose fixed and singular points classify all evolutions, including a new 'Big Shock' initial state for N>4 with negative couplings.

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