An interacting and non-interacting two-fluid dark energy models in FRW universe with time dependent deceleration parameter

DOI10.1007/s10773-011-0861-4zbMath1242.83110OpenAlexW1969391443MaRDI QIDQ429910

Anirudh Pradhan, Hishamuddin Zainuddin, Hassan Amirhashchi

Publication date: 20 June 2012

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

Full work available at URL: http://psasir.upm.edu.my/id/eprint/25147/1/An%20interacting%20and%20non.pdf

zbMATH Keywords

dark energyFRW universetime dependent deceleration parameter

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Exact solutions to problems in general relativity and gravitational theory (83C15)

Related Items (18)

Two-fluid dark energy models in Bianchi type-III universe with variable deceleration parameter ⋮ Kaluza-Klein cosmological model in \(f(R,T)\) gravity ⋮ Non-interacting Barrow-holographic dark energy in FRW-universe with quintessence behavior ⋮ Accelerating Bianchi type-V cosmology with perfect fluid and heat flow in Sáez-Ballester theory ⋮ Transit cosmological models with domain walls in \(f(R,T)\) gravity ⋮ Two fluid scenario for dark energy model in a scalar-tensor theory of gravitation ⋮ Scenario of two-fluid dark energy models in Bianchi type-III Universe ⋮ Transit cosmological models in FRW universe under the two-fluid scenario ⋮ Bianchi type-\(V\) cosmology in \(f(R,T)\) gravity with \(\varLambda (T)\) ⋮ Universe described by variable modified Chaplygin gas with statefinder diagnostic in general relativity ⋮ Bianchi type-I cosmological models with time dependent \(q\) and \(\Lambda\)-term in general relativity ⋮ Dark energy models in LRS Bianchi type-II space-time in the new perspective of time-dependent deceleration parameter ⋮ Interacting modified cosmic Chaplygin gas with variable cosmological constant and viscosity ⋮ Unnamed Item ⋮ A dark energy quintessence model of the universe ⋮ Particle creation in Friedmann-Robertson-Walker universe ⋮ Cosmological models with squared trace in modified gravity ⋮ Two fluid FRW inflationary dark energy model coupled with mass less scalar field

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