Origin of holographic dark energy models

Details Origin of holographic dark energy models Origin of holographic dark energy models

2008-03-20

arxiv.org/abs/0803.2913v2

Phys.Lett.B671:435-439,2009

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

14 pages, version to appear in PLB

Scientific paper

10.1016/j.physletb.2009.01.001

We investigate the origin of holographic dark energy models which were recently proposed to explain the dark energy-dominated universe. For this purpose, we introduce the spacetime foam uncertainty of $\delta l \ge l_{\rm p}^{\alpha}l^{\alpha-1}$. It was argued that the case of $\alpha=2/3$ could describe the dark energy with infinite statistics, while the case of $\alpha=1/2$ can describe the ordinary matter with Bose-Fermi statistics. However, two cases may lead to the holographic energy density if the latter recovers from the geometric mean of UV and IR scales. Hence the dark energy with infinite statistics based on the entropy bound is not an ingredient for deriving the holographic dark energy model. Furthermore, it is shown that the agegraphic dark energy models are the holographic dark energy model with different IR length scales.

Affiliated with

Also associated with

No associations

Rating

Origin of holographic dark energy models does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Origin of holographic dark energy models, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Origin of holographic dark energy models will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-577377