Published January 14, 2026 | Version v1
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Emergent macroscopiccorrelationsfrom alate-time nonlocalinformationalsector

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Description

The standard ΛCDM paradigm accurately describes the homogeneous expansion history and the quasi-linear statistics of large-scale

structure on scales up to O(102)Mpc, yet it does not naturally generate new macroscopic comoving correlation lengths at late

times once the primordial spectrum and the early-time transfer functions are fixed. Motivated by reports of extreme structures

andlarge-scalecoherencefeatures,andbythebroaderprogramconnectinggravityandinformationviaentanglementandmodular

considerations, we develop a conservative effective framework in which a continuous informational sector 𝜓becomes active only at

latetimesandexhibitscontrollednon-localdynamics. Weshowthatafinitecomovingcorrelationlength 𝐿𝜓 emergesgenerically

when the activated non-local kernel induces a non-analytic structure in the effective dispersion relation, selecting an imaginary pole

thatyields𝐶𝜓(𝑟)∝𝑒−𝑟/𝐿𝜓 /𝑟. Crucially,thecouplingtomatterisimplementedstatisticallyratherthandynamically: 𝜓modulates

large-scalecorrelationsthroughanon-localresponsekernelwithoutintroducingfifthforcesormodifyinglocalgrowthequations.

The resulting phenomenology leaves early-universe observables intact while enhancing the tail of large-scale structure statistics. We

further close the theoretical framework by deriving the Einstein field equations as a condition of local modular equilibrium, with the

spacetime metricemergingunambiguouslyfromquantum–informational structure.

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