Short-wave Approximation For Macroscopic Cosmology with Higgs Scalar Field

Abstract

Based on the macroscopic equations of cosmological evolution obtained earlier by the Author, a closed system of macroscopic Einstein equations in the short-wave approximation for perturbations of the scalar Higgs and gravitational fields has been obtained and examined. The obtained exact solutions of macroscopic equations are determined by three microscopic parameters, depending on the spectrum of perturbations.

arXiv comment10 pages., 3 figures, 10 references

References in corpus (5)

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• How well is our universe described by an FLRW model?
• Inflaton field potential producing the exactly flat spectrum of adiabatic perturbations
• Cosmological Evolution of Statistical System of Scalar Charged Particles
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Cited by in corpus (2)

• Cosmological evolution of a statistical system of degenerate scalar charged fermions with an asymmetric scalar doublet. II. One-component system of doubly charged fermions
• Gravitational-Scalar Instability of a Cosmological Model Based on a Two-Component System of Degenerate Scalarly Charged Fermions with Asymmetric Higgs Interaction. I. Equations for Perturbations