3 research outputs found
Constraints on the interacting holographic dark energy model
We examined the interacting holographic dark energy model in a universe with
spatial curvature. Using the near-flatness condition and requiring that the
universe is experiencing an accelerated expansion, we have constrained the
parameter space of the model and found that the model can accommodate a
transition of the dark energy from to .Comment: 9 pages, 6 figure
Transition of the dark energy equation of state in an interacting holographic dark energy model
A model of holographic dark energy with an interaction with matter fields has
been investigated. Choosing the future event horizon as an IR cutoff, we have
shown that the ratio of energy densities can vary with time. With the
interaction between the two different constituents of the universe, we observed
the evolution of the universe, from early deceleration to late time
acceleration. In addition, we have found that such an interacting dark energy
model can accommodate a transition of the dark energy from a normal state where
to phantom regimes. Implications of interacting dark energy
model for the observation of dark energy transition has been discussed.Comment: revised version, references added. Accepted for publication in PL
Super-acceleration on the Brane by Energy Flow from the Bulk
We consider a brane cosmological model with energy exchange between brane and
bulk. Parameterizing the energy exchange term by the scale factor and Hubble
parameter, we are able to exactly solve the modified Friedmann equation on the
brane. In this model, the equation of state for the effective dark energy has a
transition behavior changing from to , while
the equation of state for the dark energy on the brane has . Fitting data
from type Ia supernova, Sloan Digital Sky Survey and Wilkinson Microwave
Anisotropy Probe, our universe is predicted now in the state of
super-acceleration with .Comment: Revtex, 11 pages including 2 figures,v2: tpos fixed, references
added, to appear in JCA
