A fractional holographic dark energy model in an anisotropic Bianchi I background reduces to the flat wCDM expansion when fit to current data.
Perlmutter et al, Bull.Am.Astron.Soc., 29, 1351, (1997)
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Observational viability of fractional holographic dark energy in LRS Bianchi type-I cosmological model
A fractional holographic dark energy model in an anisotropic Bianchi I background reduces to the flat wCDM expansion when fit to current data.