Holographic dark energy density
From MaRDI portal
Publication:644348
DOI10.1007/s10773-011-0685-2zbMath1225.83107OpenAlexW2134974262MaRDI QIDQ644348
Publication date: 4 November 2011
Published in: International Journal of Theoretical Physics (Search for Journal in Brave)
Full work available at URL: https://doi.org/10.1007/s10773-011-0685-2
Related Items (11)
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 ⋮ Accretion of some classes of holographic DE onto higher-dimensional Schwarzschild black holes ⋮ 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
- Unnamed Item
- 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
- The cosmological constant problem
This page was built for publication: Holographic dark energy density
