Bulk–brane interaction and holographic dark energy
By M. Setare. 2006
184 citations recorded by the source corpus.
Abstract In this Letter we consider the bulk–brane interaction to obtain the equation of state for the holographic energy density in non-flat universe enclosed by the event horizon measured from the sphere of horizon named L. We assume that the cold dark matter energy density on the brane is conserved, but the holographic dark energy density on the brane is not conserved due to brane–bulk energy exchange. Our calculation shows, taking Ω Λ = 0.73 for the present time, the lower bound of w Λ eff is −0.9. This implies that one cannot generate phantom-like equation of state from an interacting holographic dark energy model in non-flat universe.
Subfields: Astronomy and Astrophysics, Nuclear and High Energy Physics
View Paper: https://www.semanticscholar.org/paper/77b850b9540494268a7045cb63fe6859f26a66a5
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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 holds true for the case of non-flat universe [311, 312].”