Anisotropic Bianchi type V perfect fluid cosmological models in Lyra's geometry

DOI10.1016/j.geomphys.2010.06.010zbMath1197.83128OpenAlexW1995635682MaRDI QIDQ1957172

Mohd. Zeyauddin, Shri Ram, C. P. Singh

Publication date: 24 September 2010

Published in: Journal of Geometry and Physics (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1016/j.geomphys.2010.06.010

zbMATH Keywords

cosmologyBianchi modelsgeneral relativityLyra geometryHubble's parameter

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Exact solutions to problems in general relativity and gravitational theory (83C15)

Related Items (9)

A new class of Bianchi cosmological models in Lyra's geometry ⋮ Phantom appearance of non-phantom matter in anisotropic cosmological model ⋮ Kantowski-Sachs cosmological model in Lyra's geometry ⋮ Particle creation and bulk viscosity in Bianchi-I universe in Saez-Ballester theory with different deceleration parameters ⋮ Anisotropic Bianchi type-III bulk viscous fluid universe in Lyra geometry ⋮ Bianchi type-V bulk viscous cosmological models with particle creation in Brans-Dicke theory ⋮ Non-existence of a massive scalar field for the Marder universe in Lyra and Riemannian geometries ⋮ Bianchi type III cosmological model with hybrid scale factor in the presence of Van der Waals fluid in Lyra manifold ⋮ Quark and strange quark matter in \(f(R)\) gravity for Bianchi type \(I\) and \(V\) space-times

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