Time-dependent dark energy density and holographic DE model with interaction

DOI10.1007/S10773-010-0644-3zbMath1213.83160OpenAlexW1992249649MaRDI QIDQ539592

Hassan Saadat, A. M. Saadat

Publication date: 30 May 2011

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

Full work available at URL: https://doi.org/10.1007/s10773-010-0644-3

zbMATH Keywords

cosmologydark energyholographic

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Einstein's equations (general structure, canonical formalism, Cauchy problems) (83C05) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55)

Related Items (10)

Holographic Ricci dark energy model with non-constant \(c^2\) term ⋮ Stability of dark energy models on the brane universes ⋮ Dark matter density from heavy neutrino decays ⋮ Holographic Ricci dark energy model ⋮ Hubble expansion parameter in a new model of dark energy ⋮ Holographic dark energy model with interaction and cosmological constant in the flat space-time ⋮ Time-dependent density of modified cosmic Chaplygin gas with variable cosmological constant in non-flat universe ⋮ Effect of varying bulk viscosity on generalized Chaplygin gas ⋮ Viscous new varying modified cosmic Chaplygin gas with cosmological constant in non-flat universe ⋮ Holographic dark energy density and JBP parametrization

Cites Work

• The effect of dark matter on solar system and Perihelion precession of earth planet
• Cosmological constant -- the weight of the vacuum
• Relation between the dark energy density and temperature
• Categorizing different approaches to the cosmological constant problem
• de Sitter vacua in string theory
• The cosmological constant and dark energy
• A TRACKER SOLUTION FOR A HOLOGRAPHIC DARK ENERGY MODEL
• 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
• Probable Values of the Cosmological Constant in a Holographic Theory
• Cosmological Imprint of an Energy Component with General Equation of State
• The cosmological constant problem
• Hessence: a new view of quintom dark energy

This page was built for publication: Time-dependent dark energy density and holographic DE model with interaction