A fractional holographic dark energy model in an anisotropic Bianchi I background reduces to the flat wCDM expansion when fit to current data.
Stability aspects of an LRS Bianchi type- I cosmological model in f (Q) gravity
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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.