Holographic Ricci dark energy model with non-constant \(c^2\) term
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Publication:352612
DOI10.1007/S10773-012-1416-ZzbMath1267.83129OpenAlexW1994337435MaRDI QIDQ352612
Publication date: 5 July 2013
Published in: International Journal of Theoretical Physics (Search for Journal in Brave)
Full work available at URL: https://doi.org/10.1007/s10773-012-1416-z
Relativistic cosmology (83F05) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Exact solutions to problems in general relativity and gravitational theory (83C15) Astrophysical cosmology (85A40)
Related Items (4)
Accretion of some classes of holographic DE onto higher-dimensional Schwarzschild black holes ⋮ Thermodynamics of the viscous f(T,B) gravity in the new agegraphic dark energy model ⋮ Interacting entropy-corrected holographic dark energy and IR cut-off length ⋮ Holographic dark energy model with time varying \(G\) as well as \(c^2\) parameter
Cites Work
- Unnamed Item
- Holographic Ricci dark energy model
- 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
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