Explores the dynamical origin of critical density in CCEGA, suggesting insights into QCD interactions.
We take a step toward a dynamical understanding of the critical density ρc in the CCEGA framework. Starting from the DBI action of the radion in a Randall-Sundrum background, we couple the radion field φ to the chiral condensate ⟨ψ̄ψ⟩(ρ) through an explicit effective interaction. We construct a toy effective potential with a tilted double-well shape and derive a closed-form saturation condition for ρc in terms of the QCD deconfinement density and O(1) model parameters. The working value ρc = 7.4 ρ_nuc used throughout the CCEGA series is reproduced for natural parameter choices. We emphasize that this is a plausibility/consistency result, not a parameter-free derivation of the central value, and state the remaining dependence on the ultraviolet completion explicitly.
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Marc López Sánchez (2026) studied this question.
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