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.
Cosmological-model-independent determination of Hubble constant from fast radio bursts and Hubble parameter measurements.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.