Interacting Spinor and Scalar Fields in Bianchi type-I Universe filled with Perfect Fluid: Exact Self-consistent Solutions
arXiv:gr-qc/9609056 · doi:10.1023/A:1018887024268
Abstract
Self-consistent solutions to interacting spinor and scalar field equations in General Relativity are studied for the case of Bianchi type-I space-time filled with perfect fluid. The initial and the asymptotic behavior of the field functions and the metric one has been thoroughly studied.
LaTex, 15 pages, Submitted to General Relativity and Gravitation
Cited by in corpus (42)
- Spinors, Inflation, and Non-Singular Cyclic Cosmologies
- Fermions as sources of accelerated regimes in cosmology
- Spinor Field in Bianchi type-I Universe: regular solutions
- Anisotropic cosmological models with a perfect fluid and a term
- Bianchi type I cosmology with scalar and spinor fields
- Noether symmetry for non-minimally coupled fermion fields
- Nonlinear spinor field in cosmology
- Cosmological model with non-minimally coupled fermionic field
- Dirac Spinor in Bianchi-I Universe with Time Dependent Gravitational and Cosmological Constants
- Fermions in Brans-Dicke cosmology
- Nonlinear Spinor Fields and its role in Cosmology
- Fermionic cosmologies with Yukawa type interactions
- Phantom cosmologies and fermions
- Spinor fields in spherical symmetry. Einstein-Dirac and other space-times
- Cosmological model with fermion and tachyon fields interacting via Yukawa-type potential
- Nonlinear Spinor Fields in Bianchi type-I spacetime: Problems and Possibilities
- Fermions in a Walecka-type cosmology
- Fermion field as inflaton, dark energy and dark matter
- Nonlinear Spinor field in isotropic space-time and dark energy models
- Spinor model of a perfect fluid and their applications in Bianchi type-I and FRW models
- Nonlinear spinor field in Bianchi type-I Universe filled with viscous fluid: numerical solutions
- An unified cosmological evolution driven by a mass dimension one fermionic field
- Cosmological Models Based on a Statistical System of Scalar Charged Degenerate Fermions and an Asymmetric Higgs Scalar Doublet
- Interacting scalar and spinor fields in Bianchi type I universe filled with magneto-fluid
- Nonlinear Spinor Fields in Bianchi type-I spacetime reexamined
- Spinor fields in spherically symmetric space-time
- A Cosmological Model with Dark Spinor Source
- Isotropization in Bianchi type-I cosmological model with fermions and bosons interacting via Yukawa potential
- Similarity of cosmological models and its application to the analysis of cosmological evolution
- Anisotropic cosmological models with spinor and scalar fields and viscous fluid in presence of a term: qualitative solutions
- Anisotropic cosmological models with spinor field and viscous fluid in presence of a term: qualitative solutions
- Nonlinear Spinor Fields in Bianchi type-VI spacetime
- Nonlinear Spinor Fields in Bianchi type- spacetime
- Inhomogeneous scalar field solutions and inflation
- Nonlinear Spinor Fields in Bianchi type-III spacetime
- Interacting spinor and scalar fields in Bianchi type-I Universe filled with viscous fluid: exact and numerical solutions
- Interaction of the axionic dark matter, dynamic aether, spinor and gravity fields as an origin of oscillations of the fermion effective mass
- Spinors in cylindrically symmetric space-time
- Fermionic Tachyons as a Source of Dark Energy
- Exit from accelerated regimes by symmetry breaking in a universe filled with fermionic and bosonic sources
- Spinor field in Bianchi type- space-time
- Nonlinear Spinor Fields in LRS Bianchi type-I spacetime: Theory and observation