期刊
INTERNATIONAL JOURNAL OF THEORETICAL PHYSICS
卷 50, 期 6, 页码 1769-1775出版社
SPRINGER/PLENUM PUBLISHERS
DOI: 10.1007/s10773-011-0685-2
关键词
Dark energy; Cosmological constant; Holography
In this article we consider the cosmological model based on the holographic dark energy. We study dark energy density in Universe with arbitrary spatially curvature described by the Friedmann-Robertson-Walker metric. We use Chevallier-Polarski-Linder parametrization to specify dark energy density.
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