Anisotropic dark energy models with constant deceleration parameter
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Publication:540521
DOI10.1007/s10714-010-1125-yzbMath1215.83063OpenAlexW2074658025MaRDI QIDQ540521
Publication date: 3 June 2011
Published in: General Relativity and Gravitation (Search for Journal in Brave)
Full work available at URL: https://doi.org/10.1007/s10714-010-1125-y
Relativistic cosmology (83F05) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Astrophysical cosmology (85A40)
Related Items (11)
Bianchi type strange quark cosmological models in a modified theory of gravity ⋮ Kantowski-Sachs universe with anisotropic dark energy in Lyra geometry ⋮ Bianchi-III transitioning space-time in a nonsingular hybrid universe within Lyra's cosmology ⋮ Modeling of Bianchi type I accelerating Universe in Lyra’s manifold ⋮ Invariant Bianchi type I models in f(R,T) gravity ⋮ Cosmological models with linearly varying deceleration parameter ⋮ Non-minimal matter-geometry coupling in the Bianchi-V spacetime within the formalism of f(R, T) = f1(R) + f2(R)f3(T) cosmology ⋮ Kantowski-Sachs cosmological model with anisotropic dark energy in Lyra geometry ⋮ Early decelerating \& late time accelerating anisotropic cosmological models with dynamical EoS parameter ⋮ Cosmological model universe consisting of two forms of dark energy ⋮ Bulk viscous Bianchi-I embedded cosmological model in f(R,T) = f1(R) + f2(R)f3(T) gravity
Cites Work
- Bianchi-I space-time with variable gravitational and cosmological ``constants
- LRS Bianchi type I models with anisotropic dark energy and constant deceleration parameter
- Exact Bianchi type-I cosmological models in a scalar-tensor theory
- de Sitter expansion with anisotropic fluid in Bianchi type-I space-time
- Bianchi type-I space-time with variable cosmological constant
- Viscous fluid cosmology in Bianchi type-I space-time
- Anisotropic Bianchi type-I models with constant deceleration parameter in general relativity
- The cosmological constant and dark energy
- AN EXACT BIANCHI TYPE-I COSMOLOGICAL MODEL IN LYRA'S MANIFOLD
- Exact Solutions of Einstein's Field Equations
- 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
- BIANCHI TYPE-II COSMOLOGICAL MODELS WITH CONSTANT DECELERATION PARAMETER
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