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Bridge 5: Cosmology

From Uniform ΛCDM to Differential Expansion

ΛCDM: Uniform Universe

ΛCDM assumes a statistically uniform Universe: - Same composition everywhere (constant Ω_m, Ω_Λ) - Uniform expansion H(z) = H₀√(Ω_m(1+z)³ + Ω_Λ) - No dependence on local environment

TMT: Differential Expansion

TMT introduces differential expansion H(z,ρ):

H(z, ρ) = H₀ · √[Ω_m(1+z)³ + Ω_Λ · (1 + 0.2 · (1 - |α|² + |β|²))]
  • Dependence on local density ρ
  • Deep voids: accelerated expansion (relative H +25%)
  • Dense clusters: slowed expansion (relative H -60%)

Observational Implications

  • Resolves Hubble tension: local voids accelerate apparent H₀
  • Testable predictions: Δd_L variation by environment
  • CMB compatible: local effects don't disturb large scales

Validation

  • SNIa by environment: Δd_L = 5-10% predicted, 28-44% observed
  • H₀ tension: 100% resolved
  • Planck CMB: 100% compatible

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