Emergent Cosmological Constant from Self-Organized Quantum Vacuum Boundary Conditions

his paper presents an emergent formulation of the cosmological constant ($\Lambda$) derived from macroscopic quantum vacuum boundary conditions at the Hubble horizon. Regulated by a critical acceleration threshold $a_0 \approx 1.2 \times 10^{-10}\text{ m/s}^2$, the model yields an exact vacuum energy density $\rho_{\text{vac}} = 3a_0 H_0 / (8\pi G c) \approx 5.3 \times 10^{-27}\text{ kg/m}^3$, perfectly matching Planck observational data without fine-tuning. Includes a 5-test quantitative numerical validation suite and full code reproducibility.

Authors

Publication Details

Journal
Zenodo (CERN European Organization for Nuclear Research)
Published
2026-07-25
DOI
https://doi.org/10.5281/zenodo.21540551
Primary Topic
Cosmology and Gravitation Theories
Type
article
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article

Emergent Cosmological Constant from Self-Organized Quantum Vacuum Boundary Conditions

robinson bueno parra
Zenodo (CERN European Organization for Nuclear Research)
Cosmology and Gravitation Theories
article

Emergent Cosmological Constant from Self-Organized Quantum Vacuum Boundary Conditions

robinson bueno parra
article en

Abstract

his paper presents an emergent formulation of the cosmological constant ($\Lambda$) derived from macroscopic quantum vacuum boundary conditions at the Hubble horizon. Regulated by a critical acceleration threshold $a_0 \approx 1.2 \times 10^{-10}\text{ m/s}^2$, the model yields an exact vacuum energy density $\rho_{\text{vac}} = 3a_0 H_0 / (8\pi G c) \approx 5.3 \times 10^{-27}\text{ kg/m}^3$, perfectly matching Planck observational data without fine-tuning. Includes a 5-test quantitative numerical validation suite and full code reproducibility.

Zenodo (CERN European Organization for Nuclear Research)
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Cosmology and Gravitation Theories
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Emergent Cosmological Constant from Self-Organized Quantum Vacuum Boundary Conditions — robinson bueno parra · Zenodo (CERN European Organization for Nuclear Research) (2026) | TGRS Research Map | TGRS