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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.19510839 |
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Table of Contents:
- <p>Recent observations of high-redshift galaxies by the James Webb Space Telescope (JWST)<br>reveal systems exhibiting unexpectedly advanced chemical maturity, organized<br>morphology, and rapid star formation histories within the first few hundred million years<br>after the Big Bang. These findings challenge the standard ΛCDM framework, which predicts<br>gradual, hierarchical assembly and delayed enrichment through multiple stellar<br>generations.<br>This paper proposes an alternative interpretation grounded in the Space-Phase (SP3)<br>framework, wherein the universe is permeated by a physically real, conditionable medium<br>possessing a pressure-like field with memory and anisotropic response. Within this<br>framework, early matter distribution is not random but guided into coherence corridors and<br>node intersections formed by gradients in the space-phase pressure field.<br>These corridors direct gas and dust into concentrated regions, accelerating gravitational<br>collapse, star formation, and nucleosynthesis. Subsequent supernova events distribute<br>chemically enriched material locally while further conditioning the surrounding spacephase, reinforcing corridor-node structures. This feedback loop yields rapid chemical<br>maturation without requiring extended cosmological time or repeated stochastic<br>processes.<br>The SP3 model reframes early galaxy maturity not as a temporal anomaly but as evidence<br>of efficient, guided structure formation. Predictions are provided to distinguish this model<br>observationally from standard cosmology, including anisotropic inflow signatures,<br>metallicity-node correlations, and enhanced alignment with filamentary structures.</p>