Physical Characteristics of Free Oscillations of Scalar Fields with Zero Effective Energy and Euclidean Cycles in Cosmological Models

A study and numerical modeling of the cosmological evolution of a classical scalar field with the Higgs potential was carried out. Based on the formulated similarity properties of cosmological models, their main characteristics are studied for models with different interaction scales: the Planck scale, the Grand Unified scale and the Standard Model scale. Based on numerical integration, the similarity properties of these models are proven with high accuracy.

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Physical Characteristics of Free Oscillations of Scalar Fields with Zero Effective Energy and Euclidean Cycles in Cosmological Models

Cited by 2 publications

References 10 publications

Exact Plane-Wave Solution of the Equations of a Theory of Gravitation with a Massive Graviton

Exact Plane-Wave Solution of the Equations of a Theory of Gravitation with a Massive Graviton

Complete Model of Cosmological Evolution of a Classical Scalar Field with the Higgs Potential. I. Analysis of the Model

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