Two-fluid cosmological model of Bianchi type-V with negative constant deceleration parameter

DOI10.1007/s10773-012-1323-3zbMath1263.83199OpenAlexW2007794104MaRDI QIDQ1945641

Yanyan Li

Publication date: 8 April 2013

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

Full work available at URL: https://doi.org/10.1007/s10773-012-1323-3

zbMATH Keywords

cosmological modeltwo-fluidBianchi type-Vnegative deceleration parameter

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55)

Related Items (5)

Two-fluid cosmological models in Kaluza-Klein space time ⋮ Two-fluid anisotropic cosmological model with variable \(G\) and \(\varLambda\) ⋮ Interacting holographic dark energy in Bianchi type-V and IX universes with variable deceleration parameter ⋮ Two-fluid sources in F (T ) theory of gravity ⋮ Mesonic cosmological model with two-fluid source in Lyra geometry

Cites Work

• A new class of LRS Bianchi type-I cosmological models in Lyra geometry
• Two-fluid cosmological models in Bianchi type-V space-time
• Two-fluid cosmological models in a Bianchi type I space-times
• Two-fluid Bianchi type II cosmological models
• Bianchi type V barotropic perfect fluid cosmological model in Lyra geometry
• HOMOGENEOUS ANISOTROPIC COSMOLOGICAL MODELS WITH VISCOUS FLUID AND HEAT FLOW 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
• Type Ia Supernova Discoveries atz> 1 from theHubble Space Telescope: Evidence for Past Deceleration and Constraints on Dark Energy Evolution

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