BIANCHI TYPE V COSMOLOGICAL MODELS WITH PERFECT FLUID AND HEAT CONDUCTION IN LYRA'S GEOMETRY

DOI10.1142/S0217751X08042584zbMath1165.83303OpenAlexW1980772003MaRDI QIDQ5322491

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

Publication date: 21 July 2009

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

Full work available at URL: https://doi.org/10.1142/s0217751x08042584

zbMATH Keywords

heat conductionperfect fluidLyra geometryHubble's parameterBianchi V

Mathematics Subject Classification ID

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 (7)

TILTED BIANCHI TYPE-V BAROTROPIC FLUID COSMOLOGICAL MODELS WITH VARIABLE BULK VISCOSITY IN GENERAL RELATIVITY ⋮ Spatially homogeneous Bianchi type IX dust filled universe with time dependent displacement vector in Lyra geometry ⋮ Anisotropic Bianchi type-I string cosmological models in normal gauge for Lyra's manifold with constant deceleration parameter ⋮ LRS Bianchi type II perfect fluid cosmological models in normal gauge for Lyra's manifold ⋮ BIANCHI TYPE I MAGNETIZED DUST FILLED UNIVERSE IN LYRA GEOMETRY ⋮ Bianchi type-I string dust models with bulk viscosity in Lyra geometry ⋮ Bianchi type-IX barotropic fluid model with time-dependent displacement vector in Lyra geometry

Cites Work

• A new class of LRS Bianchi type-I cosmological models in Lyra geometry
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• Some cosmological models with heat and null radiation flow
• Anisotropic Bianchi type-I models with constant deceleration parameter in general relativity
• Bianchi type in universe with viscous fluid and a \(\Lambda\) term: a qualitative analysis
• Über eine Modifikation der Riemannschen Geometrie
• Time-dependent, finite, rotating universes
• Bianchi type-I cosmological models in Lyra’s geometry
• Qualitative analysis of a class of Bianchi V imperfect fluid cosmologies
• Qualitative analysis of diagonal Bianchi type V imperfect fluid cosmological models
• Measurements of Ω and Λ from 42 High‐Redshift Supernovae
• BIANCHI TYPE-II COSMOLOGICAL MODELS WITH CONSTANT DECELERATION PARAMETER
• A Scalar-Tensor Theory of Gravitation in a Modified Riemannian Manifold
• The Thermodynamics of Irreversible Processes. III. Relativistic Theory of the Simple Fluid

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