期刊
INTERNATIONAL JOURNAL OF THEORETICAL PHYSICS
卷 51, 期 6, 页码 1932-1937出版社
SPRINGER/PLENUM PUBLISHERS
DOI: 10.1007/s10773-011-1070-x
关键词
Dark energy; Cosmological constant; Holography; Cosmology
资金
- Islamic Azad University, Marvdasht Branch
In this paper we consider holographic dark energy model with interaction in the flat space-time with non-zero cosmological constant. We calculate cosmic scale factor and Hubble expansion parameter by using the time-dependent dark energy density. Then, we obtain phenomenological interaction between holographic dark energy and matter. We fixed our solution by using the observational data.
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