Observational data shows preference for two interaction forms in fractional holographic dark energy, with only the Q=βHρ_m + γHρ_de form able to describe the universe's full evolutionary history via phase space analysis.
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Observational Constraints and Cosmological Dynamics of Interacting Fractional Holographic Dark Energy in Light of DESI DR2
Observational data shows preference for two interaction forms in fractional holographic dark energy, with only the Q=βHρ_m + γHρ_de form able to describe the universe's full evolutionary history via phase space analysis.