Authors: M KaramiFard M R Tanhayi M V Takook
Publish Date: 2015/06/14
Volume: 55, Issue: 2, Pages: 722-729
Abstract
We use the dark energy density of holographic methods to reconstruct fR in Weyl fR gravity We analyse fR by assuming that the combination of fR together with the Weyl gravity might actually be an effective description of dark energy models The reconstructed model in the spatially flat FRW universe is considered for three version of scale factors phantom quintessence and de Sitter scale factors For the de Sitter scale factor we also obtain the equationofstate parameter
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