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.
Using Pantheon and DES supernova, baryon acoustic oscillation, and Hubble parameter data to constrain the Hubble constant, dark energy dynamics, and spatial curvature.Mon
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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.