Journal
INTERNATIONAL JOURNAL OF THEORETICAL PHYSICS
Volume 50, Issue 6, Pages 1769-1775Publisher
SPRINGER/PLENUM PUBLISHERS
DOI: 10.1007/s10773-011-0685-2
Keywords
Dark energy; Cosmological constant; Holography
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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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