The Eternal Recurrence of Classicality - Void Criticality, Repercolation, and Hilbert-Space Inflation within the Stochastic Rupture Framework

We develop a late-time cosmological extension of the Stochastic Rupture (SR) framework addressing three interconnected phenomena: the desclassicalization of cosmic voids, the nucleation of new causal domains through informational repercolation, and an alternative account of early-universe expansion through Hilbert-space inflation. Cosmic voids naturally evolve toward a low-saturation Many-Worlds regime (χ → 0) as the holographic capacity outpaces local entropy production. Black holes and collapsed structures approach the opposite limit (χ → 1), producing a polarized late-time cosmology.We derive the eective free-energy functional from the SR master equation via a gradient- flow construction, obtaining Veff(χ) = Γ2χ2 +α3χ3 − Sχ at tree level. A one-loop Wilsonian renormalization-group analysis of the MSRJD functional shows that stochastic pruning fluctuations generate a positive quartic operator δb ∼ α2∆ΛUV/D, producing metastability in the infrared without any ad hoc assumptions.When the eective potential develops two local minima, standard bubble-nucleation theory applies. We derive the corrected critical radius Rc ~ pD/ΓR, which diverges as the infrared relaxation rate ΓR → 0, naturally placing repercolation at cosmological scales in the late universe. The metastability condition is expressed as an explicit discriminant inequality on the renormalized SR parameters.The framework predicts critical void-size distributions, excess supervoid correlations, suppressed primordial tensor modes, and possible correlations between supermassive black holes and void boundaries.

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Publication Details

Journal
Zenodo (CERN European Organization for Nuclear Research)
Published
2026-05-22
DOI
https://doi.org/10.5281/zenodo.20350373
Primary Topic
Cosmology and Gravitation Theories
Type
preprint
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preprint

The Eternal Recurrence of Classicality - Void Criticality, Repercolation, and Hilbert-Space Inflation within the Stochastic Rupture Framework

GUILHERME ZAMBUZI
Zenodo (CERN European Organization for Nuclear Research)
Cosmology and Gravitation Theories
preprint

The Eternal Recurrence of Classicality - Void Criticality, Repercolation, and Hilbert-Space Inflation within the Stochastic Rupture Framework

GUILHERME ZAMBUZI
preprint en

Abstract

We develop a late-time cosmological extension of the Stochastic Rupture (SR) framework addressing three interconnected phenomena: the desclassicalization of cosmic voids, the nucleation of new causal domains through informational repercolation, and an alternative account of early-universe expansion through Hilbert-space inflation. Cosmic voids naturally evolve toward a low-saturation Many-Worlds regime (χ → 0) as the holographic capacity outpaces local entropy production. Black holes and collapsed structures approach the opposite limit (χ → 1), producing a polarized late-time cosmology.We derive the eective free-energy functional from the SR master equation via a gradient- flow construction, obtaining Veff(χ) = Γ2χ2 +α3χ3 − Sχ at tree level. A one-loop Wilsonian renormalization-group analysis of the MSRJD functional shows that stochastic pruning fluctuations generate a positive quartic operator δb ∼ α2∆ΛUV/D, producing metastability in the infrared without any ad hoc assumptions.When the eective potential develops two local minima, standard bubble-nucleation theory applies. We derive the corrected critical radius Rc ~ pD/ΓR, which diverges as the infrared relaxation rate ΓR → 0, naturally placing repercolation at cosmological scales in the late universe. The metastability condition is expressed as an explicit discriminant inequality on the renormalized SR parameters.The framework predicts critical void-size distributions, excess supervoid correlations, suppressed primordial tensor modes, and possible correlations between supermassive black holes and void boundaries.

Zenodo (CERN European Organization for Nuclear Research)
Universidade Federal de Minas Gerais (BR)
Reduced inequalities
Cosmology and Gravitation Theories
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