The cosmological constant problem is a category error. Physics measured the interior of the vacuum and expected it to equal the boundary of the universe. It does not. This paper proposes that Λ — the cosmological constant — is not vacuum energy but the persistence margin: the amount by which the universe’s coherence capacity exceeds its contradiction load, written H − K. The vacuum energy is the interior. Λ is the boundary. They were never the same kind of thing. From this structural reframing, three results follow: Λ is small because a boundary needs only to be positive, not large; Λ is not constant but drifts as both H and K evolve; and the equation of state w(a) = −1 − (a/3)(H′ − K′)/(H − K) predicts a non-monotonic signature in w(z) with an inflection near z ≈ 1–2, distinguishing this framework from all smooth scalar field models. DESI DR2 (2025) finds 2.8–4.2σ preference for evolving dark energy in the direction this framework predicts. This is not a confirmation. The Friedmann-level quantitative derivation is identified as necessary future work.
Nikita Sergeyevich Shchevyev (Sun,) studied this question.