PLANE-SYMMETRIC INHOMOGENEOUS VISCOUS FLUID COSMOLOGICAL MODELS WITH ELECTROMAGNETIC FIELD

DOI10.1142/S0218271802002153zbMath1062.83576MaRDI QIDQ4674719

Vinod Kumar Yadav, N. N. Saste, Anirudh Pradhan

Publication date: 18 May 2005

Published in: International Journal of Modern Physics D (Search for Journal in Brave)

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Electromagnetic fields in general relativity and gravitational theory (83C50) Exact solutions to problems in general relativity and gravitational theory (83C15)

Related Items (8)

A plane-symmetric magnetized inhomogeneous cosmological models of perfect fluid distribution with variable magnetic permeability in Lyra geometry ⋮ Some Bianchi type I viscous fluid cosmological models with a variable cosmological constant ⋮ Higher dimensional FRW cosmology with variable G and \(\Lambda \) ⋮ BIANCHI TYPE I ANISOTROPIC MAGNETIZED COSMOLOGICAL MODELS WITH VARYING Λ ⋮ Various dark energy models for variables G and Λ in f(R, T) modified theory ⋮ Plane symmetric viscous fluid cosmological models with varying \(\Lambda\)-term ⋮ Plane-symmetric inhomogeneous magnetized viscous fluid universe with a variable \(\Lambda\) ⋮ Cylindrically symmetric inhomogeneous cosmological models with viscous fluid and varying \(\Lambda\)

Cites Work

• Bulk viscous cosmological model
• A plane-symmetric inhomogeneous cosmological model of perfect fluid distribution with electromagnetic field
• A critical density cosmological model with varying gravitational and cosmological ``constants
• Static universe in a modified Brans-Dicke cosmology
• Variable-G cosmology and creation
• A class of inhomogeneous cosmological models
• Isentropic Hydrodynamics in Plane Symmetric Space-Times
• Isotropic homogeneous universe with viscous fluid
• New class of inhomogeneous cosmological perfect-fluid solutions without big-bang singularity
• Effect of Inhomogeneity on Cosmological Models
• Dissipative cosmology
• The cosmological constant problem
• Spherically Symmetrical Models in General Relativity
• Empty space-times admitting a three parameter group of motions

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