Decoupling of the general scalar field mode and the solution space for Bianchi type I and V cosmologies coupled to perfect fluid sources
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Publication:3441704
DOI10.1063/1.2188210zbMath1111.83011arXivgr-qc/0506132OpenAlexW3105618798MaRDI QIDQ3441704
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Publication date: 16 May 2007
Published in: Journal of Mathematical Physics (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/gr-qc/0506132
Related Items (10)
Phantom expansion with non-linear Schrödinger-type formulation of scalar field cosmology ⋮ Bianchi type V cosmological models with varying cosmological term ⋮ Bulk viscous L.R.S. Bianchi type V tilted stiff fluid cosmological model in general relativity ⋮ Comprehensive analysis of the symmetries and conservation laws of the geodesic equations for a particular string inspired FRLW solution ⋮ The geometric nature of Lie and Noether symmetries ⋮ From Feshbach-resonance managed Bose-Einstein condensates to anisotropic universes: applications of the Ermakov-Pinney equation with time-dependent nonlinearity ⋮ Exact solutions in chiral cosmology ⋮ The dynamical behavior of homogeneous scalar-field spacetimes with general self-interaction potentials ⋮ Scalar field exact solutions for non-flat FLRW cosmology: a technique from non-linear Schrödinger-type formulation ⋮ Bianchi type II, III and V diagonal Einstein metrics re-visited
Cites Work
- Exact solution of scalar field cosmology with exponential potentials and transient acceleration
- Time-dependent automorphism inducing diffeomorphisms in vacuum Bianchi cosmologies and the complete closed form solutions for types II and V
- Exact scalar field cosmologies
- Bianchi cosmologies: the role of spatial topology
- Spinor sources in cosmology
- Cosmic dynamics of Bose–Einstein condensates
- Cosmology with exponential potentials
- Scalar field cosmologies with barotropic matter: models of Bianchi class B
- Exact scalar field cosmologies with a fluid
- Dynamical Systems in Cosmology
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