Holographic Ricci dark energy model
From MaRDI portal
Publication:427343
DOI10.1007/s10773-011-0952-2zbMath1241.83086OpenAlexW2050791173MaRDI QIDQ427343
Publication date: 13 June 2012
Published in: International Journal of Theoretical Physics (Search for Journal in Brave)
Full work available at URL: https://doi.org/10.1007/s10773-011-0952-2
Relativistic cosmology (83F05) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55)
Related Items (8)
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 ⋮ Time-dependent density of modified cosmic Chaplygin gas with variable cosmological constant in non-flat universe ⋮ Phenomenological fluids from interacting tachyonic scalar fields ⋮ Effect of varying bulk viscosity on generalized Chaplygin gas ⋮ Viscous new varying modified cosmic Chaplygin gas with cosmological constant in non-flat universe
Cites Work
- Unnamed Item
- Hubble expansion parameter in a new model of dark energy
- Time-dependent dark energy density and holographic DE model with interaction
- The effect of dark matter on solar system and Perihelion precession of earth planet
- Holographic dark energy density
- Holographic dark energy density and JBP parametrization
- Relation between the dark energy density and temperature
- Holography, UV/IR Relation, Causal Entropy Bound, 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
This page was built for publication: Holographic Ricci dark energy model
