Stability of the cosmological system of degenerated scalarly charged fermions and Higgs scalar fields. I: Mathematical model of linear plane perturbations
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Publication:2054878
DOI10.1134/S0202289321010102zbMath1480.83042arXiv2103.13866MaRDI QIDQ2054878
Publication date: 3 December 2021
Published in: Gravitation \& Cosmology (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/2103.13866
Unified quantum theories (81V22) Gravitational energy and conservation laws; groups of motions (83C40) Perturbations in context of PDEs (35B20) Fermionic systems in quantum theory (81V74)
Related Items (4)
Cosmological solutions and qualitative analysis in the generalized scalar-tensor theory of gravity with the Higgs potential ⋮ Evolution of spherical perturbations in the cosmological environment of degenerate scalar-charged fermions with a scalar Higgs coupling ⋮ 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 scalarly charged fermions with an asymmetric scalar doublet. I: two-component system of assorted charges
Cites Work
- Statistical systems with phantom scalar interaction in gravitation theory. I. Microscopic dynamics
- Statistical systems with phantom scalar interaction in gravitation theory. II. Macroscopic equations and cosmological models
- The self-consistent field method and macroscopic Einstein equations for the early universe
- A complete model of cosmological evolution of a scalar field with Higgs potential and Euclidean cycles
- Cosmological evolution of a scalar-charged degenerate cosmological plasma with Higgs scalar fields
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