BIANCHI TYPE I MAGNETIZED DUST FILLED UNIVERSE IN LYRA GEOMETRY

DOI10.1142/S0217751X10050603zbMath1202.83125MaRDI QIDQ3065594

Raj Bali, Naresh K. Chandnani, Jagdish Prasad Dhanka

Publication date: 6 January 2011

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

zbMATH Keywords

dustBianchi ImagnetizedLyra geometry

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Classes of solutions; algebraically special solutions, metrics with symmetries for problems in general relativity and gravitational theory (83C20) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55)

Related Items (5)

Late time isotropy viewed through Bianchi type I cosmological models with vacuum energy ⋮ Bianchi type V universe models with specific expansion anisotropy ⋮ Spatially homogeneous Bianchi type IX dust filled universe with time dependent displacement vector in Lyra geometry ⋮ Bianchi type I magnetized stiff fluid models with bulk viscosity in Lyra geometry ⋮ Bianchi type-IX barotropic fluid model with time-dependent displacement vector in Lyra geometry

Cites Work

• Exact spatially homogeneous cosmologies
• Generalized expanding and shearing anisotropic Bianchi type I magnetofluid cosmological model in general relativity
• Über eine Modifikation der Riemannschen Geometrie
• Magneto-dilatonic Bianchi-I cosmology: isotropization and singularity problems
• 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
• BIANCHI TYPE V COSMOLOGICAL MODELS WITH PERFECT FLUID AND HEAT CONDUCTION IN LYRA'S GEOMETRY
• Mach’s principle and the creation of matter

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