A Plane-Symmetric Inhomogeneous Cosmological Model of Perfect Fluid Distribution with Electromagnetic Field I
arXiv:0705.4411 · doi:10.1088/0253-6102/54/1/35
Abstract
A plane-symmetric inhomogeneous cosmological model of perfect fluid distribution with electro-magnetic field is obtained. The source of the magnetic field is due to an electric current produced along the z-axis. is the non-vanishing component of electromagnetic field tensor. To get a deterministic solution, we assume the free gravitational field is Petrov type-II non-degenerate. The behaviour of the electro-magnetic field tensor together with some physical aspects of the model are also discussed.
11 pages, no figure
References in corpus (6)
- Bianchi Type I Magnetofluid Cosmological Models with Variable Cosmological Constant Revisited
- Bianchi Type I Anisotropic Magnetized Cosmological Models with Varying
- Plane-Symmetric Inhomogeneous Bulk Viscous Cosmological Models with Variable
- Plane-symmetric inhomogeneous magnetized viscous fluid universe with a variable
- Some Inhomogeneous Magnetized Viscous Fluid Cosmological Models with Varying
- Plane Symmetric Inhomogeneous Cosmological Models with a Perfect Fluid in General Relativity