Statistical cosmological fermion systems with phantom scalar interaction of particles
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Publication:1636022
DOI10.1134/S0202289318010085zbMath1390.83457OpenAlexW2805728136MaRDI QIDQ1636022
Yu. G. Ignat'ev, D. Yu. Ignatyev, A. A. Agathonov
Publication date: 4 June 2018
Published in: Gravitation \& Cosmology (Search for Journal in Brave)
Full work available at URL: https://doi.org/10.1134/s0202289318010085
Relativistic cosmology (83F05) Applications of statistics to physics (62P35) Statistical astronomy (85A35)
Related Items (7)
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 ⋮ 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 ⋮ Peculiarities of cosmological models based on a nonlinear asymmetric scalar doublet with minimal interaction. II: Numerical analysis ⋮ 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
- Unnamed Item
- Unnamed Item
- Nonminimal macroscopic models of a scalar field based on microscopic dynamics: extension of the theory to negative masses
- Relativistic kinetic theory of statistical systems with conformally invariant interparticle scalar interaction
- Cosmological evolutions of a completely degenerate Fermi system with scalar interactions between particles
- Numerical models of cosmological evolution of a degenerate Fermi-system of scalar charged particles
- 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
- Establishment of thermodynamic equilibrium in a cosmological model with arbitrary acceleration
- A new type of isotropic cosmological models without singularity
- Gauge approach to gravitation and regular Big Bang theory
- Collisionless self-gravitating statistical systems of scalarly interacting particles
- Gravitational Field as a Generalized Gauge Field
- Regular accelerating universe without dark energy in Poincaré gauge theory of gravity
- Cosmological evolution of a Boltzmann plasma with interparticle phantom scalar interaction. I: Symmetric cases
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