Bianchi type I magnetized tilted imperfect barotropic fluid cosmological models in general relativity

DOI10.1134/S0202289308040105zbMath1176.83143OpenAlexW1979098182MaRDI QIDQ733840

D. Kharzeev

Publication date: 19 October 2009

Published in: Gravitation \& Cosmology (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1134/s0202289308040105

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Exact solutions to problems in general relativity and gravitational theory (83C15)

Related Items (2)

Viscous Bianchi type I universe with stiff matter and decaying vacuum energy density ⋮ LRS Bianchi type II tilted barotropic fluid cosmological model with heat conduction in general relativity

Cites Work

• Unnamed Item
• Magnetized cosmological model
• Homogeneous anisotropic cosmological models with viscous fluid and magnetic field
• Bianchi type V perfect fluid models with source-free electromagnetic fields
• Stiff magnetofluid cosmological model
• Tilted electromagnetic Bianchi type \(VI_ 0 \)cosmological model
• Tilted Bianchi type I stiff fluid magnetized cosmological model in general relativity
• Generalized expanding and shearing anisotropic Bianchi type I magnetofluid cosmological model in general relativity
• Bianchi type-III non-static magnetized cosmological model for perfect fluid distribution in general relativity
• Magneto-dilatonic Bianchi-I cosmology: isotropization and singularity problems
• A Bianchi type II cosmological model of Petrov type D representing an imperfect fluid with a source-free magnetic field
• Bianchi VI0 viscous fluid cosmology with magnetic field

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