String cosmological model in the presence of a magnetic flux

Abstract

A Bianchi type I string cosmological model in the presence of a magnetic flux is investigated. A few plausible assumptions regarding the parametrization of the cosmic string and magneto-fluid are introduced and some exact analytical solutions are presented.

9 pages, 4 Figures

References in corpus (3)

• Cosmology and Astrophysical Constraints of Gauss-Bonnet Dark Energy
• Gauss-Bonnet Quintessence: Background Evolution, Large Scale Structure and Cosmological Constraints
• A New Class of Inhomogeneous String Cosmological Models in General Relativity

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• Bianchi Type-II String Cosmological Models in Normal Gauge for Lyra's Manifold with Constant Deceleration Parameter
• Bianchi type-I string cosmological model in the presence of a magnetic flux: exact and qualitative solutions
• Bianchi type-I model with cosmic string in the presence of a magnetic field: spinor description
• Bianchi type-I string cosmological model in the presence of a magnetic field: classical versus loop quantum cosmology approaches
• Bianchi VI_0&III models. Self-similar approach
• The Bulk Viscous String Cosmology in An Anisotropic Universe With Late Time Acceleration
• Magnetic Bianchi type II string cosmological model in loop quantum cosmology