We analyze the physical state inside a CCEGA black star. The interior has three defining properties: uniform density ρ = ρc, saturated radion field φ = 1, and suppressed coupling Gₑff = GN e⁻¹. We term this a geometric equilibrium state (GES): baryonic matter sustained by brane geometry rather than pressure. It resembles a BEC (uniform order parameter, T ~ 10⁻³⁵ K) but differs fundamentally: coherence length ξ ~ 1974 fm (sub-nuclear), baryonic matter, non-zero Gₑff. The open problem is computing the radion fluctuation spectrum δφ (r, t) to determine the energy gap. Near Mcrit, this gap is predicted to vanish (zero mode), connecting to the critical transition of P66.
Marc López Sánchez (Sun,) studied this question.