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Published January 3, 2026 | Version v33
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Geometric Origin of Macroscopic Gravitational Normalization at Radiative Boundaries

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  • 1. Independent Researcher

Description

Dark energy, the vacuum discrepancy, and the Hubble tension are usually treated as separate problems. This essay argues that they arise from a single dimensional error: modeling cosmic expansion as a bulk 3D fluid rather than a boundary-normalized 2D constraint. Imposing thermodynamic equilibrium strictly at a radiative decoupling surface yields a mass-independent geometric invariant, pi^3/15 ≈ 2.0671. Projecting this boundary limit to the cosmic horizon gives the empirical dark-energy fraction, Omega_Lambda = pi^3/45 ≈ 0.689, without free parameters. Spatial flatness fixes the complementary matter fraction, Omega_m ≈ 0.311. The same partition sets the onset of acceleration at z_acc ≈ 0.642, naturally relaxes early dark matter requirements, and places the H0 tension in an effective topological framework. Gravity is therefore treated not only as a local metric field, but as a macroscopic constraint fixed at radiative boundaries.

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Geometric_Origin_of_Macroscopic_Gravitational_Normalization_at_Radiative_Boundaries__22_ (1).pdf

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Preprint: 10.5281/zenodo.18762247 (DOI)