Emergent Gravity at the Critical Point L/λ = 4: Finite‑Size Scaling, Chameleon Screening, and Falsifiable Predictions from Discrete Networks to CSTG Cosmology

We strengthen the unified model of emergent gravity (discrete relational networks + Chameleon Scalar-Tensor Gravity) by providing an analytical estimate of the scaling relation γ = ½(L/λ), a comprehensive finite-size scaling analysis, and quantitative observational predictions. Using simulations of Watts–Strogatz networks with up to N∼10⁴ nodes, we show that the critical attractor L/λ = 4 is approached as N → ∞, with an extrapolated infinite-size value L/λ = 3.894 ± 0.009 (deviation 2.6%). We compute the growth rate fσ₈(z), the scale-dependent matter power spectrum P(k), the stochastic gravitational wave background Ω_GW, the time variation of G, and discuss how the discrete nature of the network avoids curvature singularities. A new appendix validates numerically the conjecture that local clustering maps to Ollivier–Ricci curvature (Pearson correlation r → 0.964 for N=500), supporting the conformal coupling ξ = 1/6. All predictions are presented with realistic uncertainty ranges and are falsifiable with upcoming surveys (DESI, Euclid, LISA, SKA).

Authors

Publication Details

Journal
Zenodo (CERN European Organization for Nuclear Research)
Published
2026-05-09
DOI
https://doi.org/10.5281/zenodo.20100817
Primary Topic
Cosmology and Gravitation Theories
Type
article
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article

Emergent Gravity at the Critical Point L/λ = 4: Finite‑Size Scaling, Chameleon Screening, and Falsifiable Predictions from Discrete Networks to CSTG Cosmology

Juan Carlos Alves Tabernero
Zenodo (CERN European Organization for Nuclear Research)
Cosmology and Gravitation Theories
article

Emergent Gravity at the Critical Point L/λ = 4: Finite‑Size Scaling, Chameleon Screening, and Falsifiable Predictions from Discrete Networks to CSTG Cosmology

Juan Carlos Alves Tabernero
article en

Abstract

We strengthen the unified model of emergent gravity (discrete relational networks + Chameleon Scalar-Tensor Gravity) by providing an analytical estimate of the scaling relation γ = ½(L/λ), a comprehensive finite-size scaling analysis, and quantitative observational predictions. Using simulations of Watts–Strogatz networks with up to N∼10⁴ nodes, we show that the critical attractor L/λ = 4 is approached as N → ∞, with an extrapolated infinite-size value L/λ = 3.894 ± 0.009 (deviation 2.6%). We compute the growth rate fσ₈(z), the scale-dependent matter power spectrum P(k), the stochastic gravitational wave background Ω_GW, the time variation of G, and discuss how the discrete nature of the network avoids curvature singularities. A new appendix validates numerically the conjecture that local clustering maps to Ollivier–Ricci curvature (Pearson correlation r → 0.964 for N=500), supporting the conformal coupling ξ = 1/6. All predictions are presented with realistic uncertainty ranges and are falsifiable with upcoming surveys (DESI, Euclid, LISA, SKA).

Zenodo (CERN European Organization for Nuclear Research)
Openalex Percentile: Top 5%
Cosmology and Gravitation Theories
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Emergent Gravity at the Critical Point L/λ = 4: Finite‑Size Scaling, Chameleon Screening, and Falsifiable Predictions from Discrete Networks to CSTG Cosmology — Juan Carlos Alves Tabernero · Zenodo (CERN European Organization for Nuclear Research) (2026) | TGRS Research Map | TGRS