Holographic Dark Energy with Time Varying n^2 Parameter in Non-Flat Universe

Abstract

We consider a holographic dark energy model, with a varying parameter, n, which evolves slowly with time. We obtain the differential equation describing evolution of the dark energy density parameter, ${\Omega }_d$, for the flat and non-flat FRW universes. The equation of state parameter in this generalized version of holographic dark energy depends on n.

8 pages, 2 figures, Published in: International Journal of Theoretical Physics

References in corpus (3)

• Holographic dark energy with varying gravitational constant
• Reconstructing interacting entropy-corrected holographic scalar field models of dark energy in non-flat universe
• Power-Law Entropy Corrected Ricci Dark Energy and Dynamics of Scalar Fields

Cited by in corpus (1)

• Dynamics of Particles Around a Schwarzschild-like Black Hole in the Presence of Quintessence and Magnetic Field