Bianchi type-III cosmological models with anisotropic dark energy (DE) in lyra geometry

DOI10.1007/s10773-013-1645-9zbMath1274.83176OpenAlexW2093687824MaRDI QIDQ379351

G. C. Samanta

Publication date: 11 November 2013

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

Full work available at URL: https://doi.org/10.1007/s10773-013-1645-9

zbMATH Keywords

anisotropic fluidLyra geometryBianchi type-IIIdark energy (DE)

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)

Related Items (4)

Toy models of universe with an effective varying \(\Lambda\)-term in Lyra manifold ⋮ Bianchi-III transitioning space-time in a nonsingular hybrid universe within Lyra's cosmology ⋮ Anisotropic cosmological model in presence of holographic dark energy and quintessence ⋮ Universe described by variable modified Chaplygin gas with statefinder diagnostic in general relativity

Cites Work

• Unnamed Item
• Unnamed Item
• Tilted Bianchi type-I cosmological model in Lyra geometry
• A new class of Bianchi cosmological models in Lyra's geometry
• Dark energy model in anisotropic Bianchi type-III space-time with variable eos parameter
• Dynamics of Bianchi \(I\) universe with magnetized anisotropic dark energy
• Bianchi type III models with anisotropic dark energy
• Bianchi type V cosmological models with constant deceleration parameter in general relativity
• Tilted electromagnetic Bianchi type III cosmological solution
• Plane symmetric domain wall in Lyra geometry
• Bianchi type-III cosmological model with negative constant deceleration parameter in Brans Dicke theory of gravitation
• Anisotropic Bianchi type-I models with constant deceleration parameter in general relativity
• Dark energy and gravity
• The Bianchi models: then and now
• Über eine Modifikation der Riemannschen Geometrie
• GLOBAL MONOPOLES IN LYRA GEOMETRY
• EFFECTS OF ELECTROMAGNETIC FIELD ON THE DYNAMICS OF BIANCHI TYPE VI₀UNIVERSE WITH ANISOTROPIC DARK ENERGY
• The cosmological constant and dark energy
• Vector field as a quintessence partner
• DYNAMICS OF DARK ENERGY
• RECONSTRUCTING DARK ENERGY
• Bianchi type-I cosmological models in Lyra’s geometry
• Cosmological parameters from SDSS and WMAP
• 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
• Inflationary universe: A possible solution to the horizon and flatness problems
• A Scalar-Tensor Theory of Gravitation in a Modified Riemannian Manifold

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