Observational constraints on interacting fractional holographic dark energy models show that Q=βHρ_m + γHρ_de best matches data and reproduces the universe's evolutionary history.
A Comprehensive Measurement of the Local Value of the Hubble Constant with 1 km s −1 Mpc−1 Uncertainty from the Hubble Space Telescope and the SH0ES Team.Astrophys
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Observational Constraints and Cosmological Dynamics of Interacting Fractional Holographic Dark Energy in Light of DESI DR2
Observational constraints on interacting fractional holographic dark energy models show that Q=βHρ_m + γHρ_de best matches data and reproduces the universe's evolutionary history.