Numerical models of cosmological evolution of a degenerate Fermi-system of scalar charged particles
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Publication:891492
DOI10.1134/S0202289315020048zbMath1325.83026arXiv1408.4738MaRDI QIDQ891492
A. A. Agathonov, Yu. G. Ignat'ev
Publication date: 17 November 2015
Published in: Gravitation \& Cosmology (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1408.4738
Relativistic cosmology (83F05) Exact solutions to problems in general relativity and gravitational theory (83C15) Computational methods for problems pertaining to relativity and gravitational theory (83-08) Einstein-Maxwell equations (83C22)
Related Items (9)
Statistical cosmological fermion systems with phantom scalar interaction of particles ⋮ Cosmological evolution of the Boltzmann plasma with phantom scalar interparticle interaction. II: Multicomponent system without charge symmetry ⋮ Qualitative and numerical analysis of a cosmological model based on a phantom scalar field with self-interaction ⋮ Qualitative and numerical analysis of a cosmological model based on a classical massive scalar field ⋮ Relativistic kinetic theory of statistical systems with conformally invariant interparticle scalar interaction ⋮ Complete cosmological model based on an asymmetric scalar Higgs doublet ⋮ Cosmological models based on a statistical system of scalar charged degenerate fermions and an asymmetric Higgs scalar doublet ⋮ Peculiarities of cosmological models based on a nonlinear asymmetric scalar doublet with minimal interaction. I. Qualitative analysis ⋮ Cosmological evolution of a statistical system of degenerate scalarly charged fermions with an asymmetric scalar doublet. I: two-component system of assorted charges
Uses Software
Cites Work
- Exact solution of the relativistic magnetohydrodynamic equations in the background of a plane gravitational wave with combined polarization
- 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
- Cosmological evolution of the degenerated plasma with interparticle scalar interaction. II: formulation of mathematical model
- Cosmological evolution of plasma with scalar interparticle interaction. I. canonical formulation of classical scalar interaction
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