A more general interacting model of holographic dark energy

Details A more general interacting model of holographic dark energy A more general interacting model of holographic dark energy

2010-04-13

arxiv.org/abs/1004.2092v2

Phys. Lett. B 688 (2010) 263-268

Astronomy and Astrophysics

Astrophysics

Cosmology and Extragalactic Astrophysics

7 pages, 8 figures, references added

Scientific paper

10.1016/j.physletb.2010.04.023

So far, there have been no theories or observational data that deny the presence of interaction between dark energy and dark matter. We extend naturally the holographic dark energy (HDE) model, proposed by Granda and Oliveros, in which the dark energy density includes not only the square of the Hubble scale, but also the time derivative of the Hubble scale to the case with interaction and the analytic forms for the cosmic parameters are obtained under the specific boundary conditions. The various behaviors concerning the cosmic expansion depend on the introduced numerical parameters which are also constrained. The more general interacting model inherits the features of the previous ones of HDE, keeping the consistency of the theory.

Affiliated with

Also associated with

No associations

Rating

A more general interacting model of holographic dark energy 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 A more general interacting model of holographic dark energy, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and A more general interacting model of holographic dark energy will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-280656