Nonlinear spinor field in cosmology
arXiv:gr-qc/0308088 · doi:10.1103/PhysRevD.69.124006
Abstract
Within the scope of Bianchi type VI (BVI) model the self-consistent system of nonlinear spinor and gravitational fields is considered. Exact self-consistent solutions to the spinor and gravitational field equations are obtained for some special choice of spatial inhomogeneity and nonlinear spinor term. The role of inhomogeneity in the evolution of spinor and gravitational field is studied. Oscillatory mode of expansion of the BVI universe is obtained for some special choice of spinor field nonlinearity.
RevTex4, 19 pages, 4 figures
References in corpus (1)
Cited by in corpus (33)
- Dark Matter and Dark Energy Interactions: Theoretical Challenges, Cosmological Implications and Observational Signatures
- CMB Anisotropies and Inflation from Non-Standard Spinors
- Fermions as sources of accelerated regimes in cosmology
- Noether symmetry for non-minimally coupled fermion fields
- Cosmological model with non-minimally coupled fermionic field
- Fermions in Brans-Dicke cosmology
- Nonlinear Spinor Fields and its role in Cosmology
- Fermionic cosmologies with Yukawa type interactions
- G-essence with Yukawa Interactions
- Bianchi-I classical and quantum spinor cosmology with signature change
- Fermions in a Walecka-type cosmology
- Classical and quantum spinor cosmology with signature change
- Nonlinear Spinor field in isotropic space-time and dark energy models
- Bianchi type-I model with cosmic string in the presence of a magnetic field: spinor description
- Time reparameterization in Bianchi type I spinor cosmology
- Nonlinear Spinor Fields in Bianchi type-I spacetime reexamined
- Bianchi type-V dark energy model with varying EoS parameter
- Bianchi type-VI anisotropic dark energy model with varying EoS parameter
- Conformally-coupled dark spinor and FRW universe
- Spinor model of a perfect fluid
- Reconstruction of f-essence and fermionic Chaplygin gas models of dark energy
- Nonlinear Spinor Fields in Bianchi type-VI spacetime
- Nonlinear Spinor Fields in Bianchi type- spacetime
- Shifted Riccati Procedure: Application to Conformal Barotropic FRW Cosmologies
- Bianchi type-II cosmological model: some remarks
- Some remarks on Bianchi type-II, VIII and IX models
- Accelerated expansion of the Universe driven by G-essence
- Nonlinear Spinor Fields in Bianchi type-III spacetime
- Space-time evolution induced by spinor fields with canonical and non-canonical kinetic terms
- Compactification and signature transition in Kaluza-Klein spinor cosmology
- Spinor field in Bianchi type- space-time
- Nonlinear Spinor Fields in LRS Bianchi type-I spacetime: Theory and observation
- Extension of the Einstein-Dirac-axion-aether theory based on an effective metric with a spinor kernel