Stability of the cosmological system of degenerated scalar charged fermions and Higgs scalar fields. I. Mathematical model of linear plane perturbations

Abstract

A mathematical model of the evolution of plane perturbations in the cosmological statistical system of completely degenerated scalar-charged fermions with the Higgs scalar interaction is formulated. A complete closed system of differential equations describing the unperturbed state of a homogeneous and isotropic system and a system of self-consistent equations describing the evolution of small perturbations are constructed.

6 pages, 6 references

References in corpus (5)

• Statistical system with fantom scalar interaction. II. Macroscopic Equations and Cosmological Models
• Statistical system with a fantom scalar interaction in the Gravitation Theory. I. The Microscopic Dynamics
• A Complete Model of Cosmological Evolution of Scalar Field with Higgs Potential and Euclidian Cycles
• The Method of Self-Consistent Field and Macroscopical Einstein Equations for the Early Universe
• Cosmological evolution of a scalar-charged degenerate cosmological plasma with Higgs scalar fields

Cited by in corpus (4)

• Evolution of spherical perturbations in the cosmological environment of degenerate scalarly charged fermions with the Higgs scalar interaction
• Cosmological Models Based on a Statistical System of Scalar Charged Degenerate Fermions and an Asymmetric Higgs Scalar Doublet
• Cosmological evolution of a statistical system of degenerate scalar-charged fermions with an asymmetric scalar doublet. I. Two-component system of assorted charges
• Gravitational - Scalar Instability of a Two-Component Degenerate System of Scalar Charged Fermions with Asymmetric Higgs Interaction