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
A mathematical model is formulated for the evolution of plane perturbations in a cosmological two-component statistical system of completely degenerate scalarly charged fermions with an asymmetric scalar Higgs interaction. A complete closed system of differential equations describing the unperturbed state of a homogeneous and isotropic system and a system of self-consistent evolution equations of small perturbations are constructed.
Keywords
cosmological models,
Higgs fields,
degenerate fermions,
scalar charges,
perturbations,
instabilityAuthors
Ignat’ev Yu.G. | Institute of Physics Kazan Federal University | yurii.ignatev.1947@yandex.ru |
Всего: 1
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