Dark energy models in plane symmetric space-time with time varying \(\varLambda \) term

DOI10.1007/s10773-012-1316-2zbMath1263.83057OpenAlexW2060620656MaRDI QIDQ1945619

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/s10773-012-1316-2

zbMATH Keywords

Chaplygin gasquintessencedark energyplane symmetrictime varying\(\varLambda \) term

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Exact solutions to problems in general relativity and gravitational theory (83C15)

Related Items (1)

The cosmological constant constrained with Union2.1 supernovae type Ia data

Cites Work

• Dark energy models with anisotropic fluid in Bianchi type-\(VI _{0}\) space-time with time dependent deceleration parameter
• Plane symmetric cosmological models with perfect fluid and dark energy
• Bianchi type-V cosmological models with perfect fluid and dark energy
• Bulk viscous Bianchi type I cosmological models with time-dependent cosmological term \(\Lambda \)
• de Sitter brane universe induced by phantom and quantum effects
• Quantum de Sitter cosmology and phantom matter
• Unification of dark matter and dark energy: the inhomogeneous Chaplygin gas
• Plane-symmetric inhomogeneous magnetized viscous fluid universe with a variable \(\Lambda\)
• Plane symmetric string cosmological models in self-creation theory of gravitation
• Time-dependent wormhole in an inhomogeneous spherically symmetric space time with a cosmological constant
• Some Bianchi type I viscous fluid cosmological models with a variable cosmological constant
• Plane symmetric viscous fluid cosmological models with varying \(\Lambda\)-term
• HOLOGRAPHIC CHAPLYGIN DGP COSMOLOGIES
• BIANCHI TYPE I MAGNETOFLUID COSMOLOGICAL MODELS WITH VARIABLE COSMOLOGICAL CONSTANT REVISITED
• Anisotropic Bianchi Type-I Magnetized String Cosmological Models with Decaying Vacuum Energy Density Λ( t )
• 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
• An alternative to quintessence

This page was built for publication: Dark energy models in plane symmetric space-time with time varying \(\varLambda \) term