Statistical system with fantom scalar interaction. II. Macroscopic Equations and Cosmological Models

Abstract

Based on the proposed earlier by the Author approach to macroscopic description of scalar interaction, this paper develops the macroscopic model of relativistic plasma with a fantom scalar interaction of elementary particles. In the article the macroscopic equations for a statistical system with scalar interaction of particles are obtained and the complete set of macroscopic equations describing cosmological models is built.

10 pages, 11 references

References in corpus (4)

• The cosmological evolution of the cosmological plasma with interpartial scalar interaction. I. The canonic formulation of classical scalar interaction
• Cosmological evolution of the cosmological plasma with interpartial scalar interaction. III. Model with the attraction of the like scalar charged particles
• Cosmological evolution of the cosmological plasma with interpartial scalar interaction. II. Formulation of mathematical model
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• Complete cosmological model based on a asymmetric scalar Higgs doublet
• Nonminimal Macroscopic Models of a Scalar Field Based on Microscopic Dynamics. I. Extension of the Theory for Negative Masses
• Cosmological Models Based on a Statistical System of Scalar Charged Degenerate Fermions and an Asymmetric Higgs Scalar Doublet
• Numerical Models of Cosmological Evolution of the Degenerated Fermi-system of Scalar Charged Particles
• Gravitational - Scalar Instability of a Two-Component Degenerate System of Scalar Charged Fermions with Asymmetric Higgs Interaction
• Cosmological evolution of a statistical system of degenerate scalar-charged fermions with an asymmetric scalar doublet. I. Two-component system of assorted charges
• The Qualitative and Numerical Analysis of the Cosmological Model Based on Phantom Scalar Field with Self
• Cosmological evolution of a scalar-charged degenerate cosmological plasma with Higgs scalar fields
• Cosmological evolution of a statistical system of degenerate scalar charged fermions with an asymmetric scalar doublet. II. One-component system of doubly charged fermions
• Evolution of plane perturbations in the cosmological environment of the Higgs scalar field and an ideal scalar charged fluid
• Stability of the cosmological system of degenerated scalar charged fermions and Higgs scalar fields. I. Mathematical model of linear plane perturbations
• The Stability of the Cosmological System of Degenerate Scalar Charged Fermions and Higgs Scalar Fields. II. The Evolution of Short-Wave Perturbations
• The self-consistent field method and the macroscopic universe consisting of a fluid and a black holes
• Dynamics of cosmological models with nonlinear classical phantom scalar fields. I. Formulation of the mathematical model
• The Statistical Model with Interpartial Scalar Conformally Invariant Interaction
• The Possibility Of The Strict Global Thermodynamic Equilibrium In The Expanding Universe At Presence Of The Fundamental Scalar Field