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| Formaat: | Recurso digital |
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Zenodo
2026
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| Online toegang: | https://doi.org/10.5281/zenodo.19120281 |
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Inhoudsopgave:
- <p>This note follows a single boundary residue from spherical radiative geometry to the holographic state count of the observable universe. Starting from the boundary relation ΛR_H² = π³/15, the horizon radius is fixed directly by the residue π³/15 together with the observed cosmological term Λ. The corresponding horizon area A_H = 4πR_H² then gives a Planck-cell count N = A_H/ℓ_P², with ℓ_P² = ħG/c³, yielding N ∼ 10^122. The standard holographic order of magnitude is therefore recovered, but the horizon area is not taken as an independent input. It is written first from the same boundary residue. Within this ordering, the large number 10^122 is not treated as a catastrophic excess of bulk vacuum states, but as the expected Planck-scale count of a horizon whose size is already fixed by the boundary residue. The physical scale changes; the boundary residue does not.</p>