TILTED BIANCHI TYPE-V BAROTROPIC FLUID COSMOLOGICAL MODELS WITH VARIABLE BULK VISCOSITY IN GENERAL RELATIVITY

DOI10.1142/S0217751X11054462zbMath1247.83067OpenAlexW2062448669MaRDI QIDQ2919101

Pramila Kumawat, Raj Bali, Shalini Sharma

Publication date: 2 October 2012

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

Full work available at URL: https://doi.org/10.1142/s0217751x11054462

zbMATH Keywords

heat conductionbulk viscositybarotropicBianchi V

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)

Cites Work

• Bulk viscous L.R.S. Bianchi type V tilted stiff fluid cosmological model in general relativity
• Biachi type-II cosmological model with viscous fluid
• Homogeneous anisotropic cosmological models with viscous fluid and magnetic field
• Viscous fluid universe filled with stiff fluid in general relativity
• Cosmological constant -- the weight of the vacuum
• Time-dependent, finite, rotating universes
• Qualitative analysis of a class of Bianchi V imperfect fluid cosmologies
• Qualitative analysis of diagonal Bianchi type V imperfect fluid cosmological models
• A dynamical systems approach to the tilted Bianchi models of solvable type
• BIANCHI TYPE V COSMOLOGICAL MODELS WITH PERFECT FLUID AND HEAT CONDUCTION IN LYRA'S GEOMETRY
• BIANCHI TYPE I UNIVERSE WITH VISCOUS FLUID

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