Constraints on the interacting holographic dark energy model
By Bin Wang, Chi-Yong Lin, E. Abdalla. 2005
280 citations recorded by the source corpus.
Abstract 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 ω D > − 1 to ω D − 1 .
Subfields: Astronomy and Astrophysics, Nuclear and High Energy Physics
View Paper: https://www.semanticscholar.org/paper/5bb46e9c7523ac847d8aaad6b14b574dbfce527a
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In Astronomy and Astrophysics
- Yi Wang
- Shuang Wang
- Miao Li
- Emmanuel N. Saridakis
- Xin Zhang
- M. Setare
- Fotios Anagnostopoulos
- Ratbay Myrzakulov
In Nuclear and High Energy Physics
- Yi Wang
- Shuang Wang
- Miao Li
- Emmanuel N. Saridakis
- Xin Zhang
- M. Setare
- Fotios Anagnostopoulos
- Ratbay Myrzakulov
Citations in the corpus
- Holographic dark energy (2016, background): “This conclusion had been extended to a universe with spatial curvature [309].”