This paper derives the ideal de Sitter fixed-point reading of the Cohen-Kaplan-Nelson (CKN) holographic coefficient. By selecting the natural boundary-saturation unit (τ = 1) determined by the Bekenstein-Hawking entropy bound, the framework calculates a geometric fixed point of C₁ = π²/ (16e²). This derivation yields a theoretical dark energy density fraction of Ω_Λ^ (fp) ≈ 0. 6994, which is strictly independent of the Hubble constant (H₀) and the gravitational constant (G).
Yiling Zhu (Sat,) studied this question.