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.
Wilkinson Microwave Anisotropy Probe (WMAP) Three Year Results: Implications for Cosmology.Astrophys
1 Pith paper cite this work. Polarity classification is still indexing.
1
Pith paper citing it
fields
physics.gen-ph 1years
2026 1verdicts
CONDITIONAL 1representative citing papers
citing papers explorer
-
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.