Bianchi type-III cosmological models with time dependent displacement vector for barotropic fluid distribution in Lyra geometry

DOI10.1007/s10773-009-0106-yzbMath1184.83044OpenAlexW2012158785MaRDI QIDQ849098

Naresh K. Chandnani, Raj Bali

Publication date: 24 February 2010

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

Full work available at URL: https://doi.org/10.1007/s10773-009-0106-y

zbMATH Keywords

Lyra geometrydisplacement vectorBianchi III

Mathematics Subject Classification ID

Relativistic cosmology (83F05) 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 (3)

Thick domain walls coupled with viscous fluid and electromagnetic field in Lyra geometry ⋮ A new class of inhomogeneous cosmological models with electromagnetic field in normal gauge for Lyra's manifold ⋮ Bianchi type-III bulk viscous and barotropic perfect fluid cosmological models in Lyra's geometry

Cites Work

• Bianchi type V and \(VI_ 0\) cosmological models in Lyra geometry
• Exact spatially homogeneous cosmologies
• Bianchi type III and Kantowski-Sachs cosmological models in Lyra geometry
• Topology and cosmology
• Über eine Modifikation der Riemannschen Geometrie
• HIGHER DIMENSIONAL COSMOLOGICAL MODEL IN LYRA GEOMETRY
• Bianchi type-I cosmological model for perfect fluid distribution in Lyra geometry
• Bianchi type-I cosmological models in Lyra’s geometry
• INHOMOGENEOUS COSMOLOGICAL MODEL IN LYRA GEOMETRY
• BIANCHI TYPE I MAGNETOFLUID COSMOLOGICAL MODELS WITH VARIABLE COSMOLOGICAL CONSTANT REVISITED
• A Scalar-Tensor Theory of Gravitation in a Modified Riemannian Manifold
• Mach’s principle and the creation of matter

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