Resolution of the S8 Tension via Non-Linear Vacuum Hardening: A Generative Proof from the Universal Tension-Driven Lattice (UTDL)
Abstract
The "Clumpiness Tension" (S8)—the statistically significant discrepancy between the amplitude of matter clustering predicted by the Standard Model (ΛCDM, S8 ≈ 0.83) and that observed by weak lensing surveys (KiDS/DES/HSC, S8 ≈ 0.76–0.78)—represents a critical failure of linear gravity on cosmological scales. In this work, we resolve this tension as an emergent phase transition of the Universal Tension-Driven Lattice (UTDL). We introduce the mechanism of Vacuum Jamming (Phenomenon 37), resolving the apparent paradox between the attractive potential required for particle genesis and the repulsive stiffness required for cosmological stability. By performing a bond-wise variational analysis of the UTDL Hamiltonian (H ∼ (∇ ϕ)2 − ϕ4), we demonstrate that the vacuum possesses a topological "Hard Core" (Veff ∼ +R−2) that dominates over the softening potential (Veff ∼ −R−1) at high strains, triggering a divergent stiffening of the manifold. We derive the cosmological hardening coefficient β from first principles as the strain root of the Fine Structure Constant (β = √αfs ≈ 0.085), linking large-scale structure directly to vacuum impedance. Spherical collapse simulations utilizing this parameter-free brake demonstrate that while linear theory is unaffected, non-linear collapse is mechanically suppressed. The model predicts a suppression of the virial radius yielding an emergent S8 ≈ 0.704 at the turnaround epoch, which relaxes to S8 ≈ 0.746 when volume-averaged over a realistic "Fluffy" halo profile. This result, accurate to within 3.1% of observational targets without fitting, suggests that the S8 tension is the observational signature of a self-limiting, non-linear vacuum geometry.
Fields of Study & Subjects
Cosmology and Gravitation Theories
Galaxies: Formation
Evolution
Phenomena
Advanced Mathematical Theories and Applications
Publication details
- Journal / source
- Zenodo (CERN European Organization for Nuclear Research)
- Publication date
- 11 January 2026
- Document type
- Preprint