期刊
INTERNATIONAL JOURNAL OF THEORETICAL PHYSICS
卷 49, 期 5, 页码 1118-1126出版社
SPRINGER/PLENUM PUBLISHERS
DOI: 10.1007/s10773-010-0291-8
关键词
Holography; Dark energy; Redshift
资金
- Research Institute for Astronomy AMP
- Astrophysics of Maragha (RIAAM), Maragha, Iran
Motivated by Granda and Oliveros (GO) model, we generalize their work to the non-flat case. We obtain the evolution of the dark energy density, the deceleration and the equation of state parameters for the holographic dark energy model in a non-flat universe with GO cut-off. In the limiting case of a flat universe, i.e. k=0, all results given in GO model are obtained.
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