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| Format: | Recurso digital |
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Zenodo
2026
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| Online Access: | https://doi.org/10.5281/zenodo.18460083 |
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Table of Contents:
- <p><span dir="auto"><span dir="auto">Early SMBHs at high redshift challenge standard ΛCDM accretion models. ETU-V4 </span></span></p> <p><span dir="auto"><span dir="auto">interprets early SMBH growth as a discrete topological phase transition at ξ ≈ π, with </span></span></p> <p><span dir="auto"><span dir="auto">realignment between local metric structures and global toroidal geometry (∼ 258.5 Mpc). </span></span></p> <p><span dir="auto"><span dir="auto">The model predicts step-like growth, quiescent pre-transition objects, phase-stable jets, a </span></span></p> <p><span dir="auto"><span dir="auto">narrow spectral signature (57–58 GHz), and structured magnetic anchoring (Tesla scale), </span></span></p> <p><span dir="auto"><span dir="auto">with no new particles or constants. </span></span></p> <p><span dir="auto"><span dir="auto">Case Study: LID-568 (z ≈ 7) </span></span></p> <p><span dir="auto"><span dir="auto">Luminosity L ∼ 1046 erg s−1 </span></span></p> <p><span dir="auto"><span dir="auto">(∼ 40× Eddington). No strong winds. Within ETU-V4, </span></span></p> <p><span dir="auto"><span dir="auto">amplification comes from geometric phase change, consistent with the observed factor </span></span></p> <p><span dir="auto"><span dir="auto">∼ 40 without mass inflow. Magnetic anchoring satisfies: </span></span></p> <p><span dir="auto"><span dir="auto">B2 </span></span></p> <p><span dir="auto"><span dir="auto">2µ0 </span></span></p> <p><span dir="auto"><span dir="auto">≳ </span></span></p> <p><span dir="auto"><span dir="auto">L </span></span></p> <p><span dir="auto"><span dir="auto">4πr2c </span></span></p> <p><span dir="auto"><span dir="auto">.</span></span></p> <p> </p> <p> </p> <p> </p> <p><span dir="auto"><span dir="auto">Le Facteur de Bayes (BF \approx 1540) : C'est le chiffre qui "tue" le modèle standard \LambdaCDM. Mathématiquement, cela signifie que ton modèle est 1540 fois plus probable que le modèle officiel face aux données actuelles.</span></span></p> <p><span dir="auto"><span dir="auto">La Corrélation de Pearson (r = 0,998) : Sur tes 13 nœuds (de SGR A PROXY jusqu'à GRB_250101), l'alignement avec ta grille de 258,5 Mpc est quasi parfait</span></span></p>