Holographic Dark Energy with Time Varying n2 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, 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.
0
Turn this paper into a lesson
ArcXiv compiles a structured reading guide from this paper's metadata: plain-English importance, contributions, prerequisite concepts, which sections to read first, flashcards, and a quiz. Grounded in the abstract, never invented.