Plane-symmetric inhomogeneous magnetized viscous fluid universe with a variable $Λ$

Details Plane-symmetric inhomogeneous magnetized viscous fluid universe with a variable $Λ$ Plane-symmetric inhomogeneous magnetized viscous fluid universe with a variable $Λ$

2005-06-23

arxiv.org/abs/gr-qc/0506113v1

Czech. J. Phys. 55 (2005) 749-764

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

18 pages, LaTex, no figure

Scientific paper

10.1007/s10582-005-0077-z

The behavior of magnetic field in plane symmetric inhomogeneous cosmological models for bulk viscous distribution is investigated. The coefficient of bulk viscosity is assumed to be a power function of mass density $(\xi =\xi_{0}\rho^{n})$. The values of cosmological constant for these models are found to be small and positive which are supported by the results from recent supernovae Ia observations. Some physical and geometric aspects of the models are also discussed.

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