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2026
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| Online Access: | https://doi.org/10.5281/zenodo.18723711 |
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| _version_ | 1866901884324806656 |
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| author | Bashan, Nadav |
| author_facet | Bashan, Nadav |
| contents | <p>In this work, we present a geometric boundary framework that explicitly derives the gravitational relation (G) from the cosmological constant (Λ) through a scale-independent surface normalization. Starting from radiative decoupling surfaces, we identify a dimensionless boundary relation converging to the exact mass-independent identity π³/15. Extending this boundary condition to the cosmic horizon yields the master constraint ΛR_H² = π³/15. By incorporating holographic tiling of the horizon area, we extract an explicit algebraic expression for G, governed entirely by the discrete information bound (N) of the macroscopic surface. Within this formulation, the canonical ~ 10^120 vacuum-energy discrepancy is mathematically resolved not as an energy divergence, but as the exact dimensional scaling factor required to map the macroscopic horizon area to Planck-scale elements. Consequently, the dark-energy fraction and Hubble-scale kinematics emerge as rigid geometric imperatives of the identical boundary condition.</p> <p> </p> <p> </p> |
| format | Recurso digital |
| id | zenodo_https___doi_org_10_5281_zenodo_18723711 |
| institution | Zenodo |
| language | |
| publishDate | 2026 |
| publisher | Zenodo |
| record_format | zenodo |
| spellingShingle | The Holographic Boundary Principle: A Geometric Normalization from Stellar Photospheres to the Cosmic Horizon Bashan, Nadav <p>In this work, we present a geometric boundary framework that explicitly derives the gravitational relation (G) from the cosmological constant (Λ) through a scale-independent surface normalization. Starting from radiative decoupling surfaces, we identify a dimensionless boundary relation converging to the exact mass-independent identity π³/15. Extending this boundary condition to the cosmic horizon yields the master constraint ΛR_H² = π³/15. By incorporating holographic tiling of the horizon area, we extract an explicit algebraic expression for G, governed entirely by the discrete information bound (N) of the macroscopic surface. Within this formulation, the canonical ~ 10^120 vacuum-energy discrepancy is mathematically resolved not as an energy divergence, but as the exact dimensional scaling factor required to map the macroscopic horizon area to Planck-scale elements. Consequently, the dark-energy fraction and Hubble-scale kinematics emerge as rigid geometric imperatives of the identical boundary condition.</p> <p> </p> <p> </p> |
| title | The Holographic Boundary Principle: A Geometric Normalization from Stellar Photospheres to the Cosmic Horizon |
| url | https://doi.org/10.5281/zenodo.18723711 |