Demonstrates emergent cosmological constant using quantum vacuum, indicating theoretical implications for cosmology.
his paper presents an emergent formulation of the cosmological constant (Λ) derived from macroscopic quantum vacuum boundary conditions at the Hubble horizon. Regulated by a critical acceleration threshold a₀ ≈ 1.2 × 10⁻¹⁰ m/s², the model yields an exact vacuum energy density ρvac = 3a₀ H₀ / (8π G c) ≈ 5.3 × 10⁻²⁷ kg/m³, perfectly matching Planck observational data without fine-tuning. Includes a 5-test quantitative numerical validation suite and full code reproducibility.
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robinson bueno parra (2026) studied this question.
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