Accelerating dark energy cosmological model in two fluids with hybrid scale factor

DOI10.1142/S0219887817501249zbMath1375.83066arXiv1702.06834MaRDI QIDQ5359034

P. K. Sahoo, B. Mishra, Pratik P. Ray

Publication date: 22 September 2017

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

Full work available at URL: https://arxiv.org/abs/1702.06834

zbMATH Keywords

general relativitycosmic stringdark energyaccelerating universedensity parameterstring fluidtwo fluidBianchi V spacetime

Mathematics Subject Classification ID

Relativistic cosmology (83F05) String and superstring theories in gravitational theory (83E30) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Astrophysical cosmology (85A40)

Related Items (6)

Bianchi type-\(I\) bulk viscosity with a DE cosmological model ⋮ Cosmological models in R2 gravity with hybrid expansion law ⋮ Analysis of general relativistic hydrodynamic cosmological models with stability factor in theories of gravitation ⋮ Anisotropic cosmological models with two fluids ⋮ Interactions in the dark sector within the scope of Bianchi type-V model ⋮ The late cosmic acceleration and the coincidence problem in Bianchi type I Universe

Cites Work

• Bulk-brane interaction and holographic dark energy
• The holographic dark energy in non-flat Brans-Dicke cosmology
• Bianchi type-I anisotropic dark energy model with constant deceleration parameter
• LRS Bianchi type I models with anisotropic dark energy and constant deceleration parameter
• Bianchi type III models with anisotropic dark energy
• Statefinder parameters for interacting dark energy
• Anisotropic model of a dark energy dominated Universe with hybrid expansion law
• Dark energy models with variable equation of state parameter
• Anisotropic dark energy model with a hybrid scale factor
• THERMODYNAMICAL DESCRIPTION OF THE INTERACTING NEW AGEGRAPHIC DARK ENERGY
• DYNAMICS OF DARK ENERGY
• An alternative to quintessence

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