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Dettagli Bibliografici
Autore principale: Matuchaki
Natura: Recurso digital
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Pubblicazione: Zenodo 2025
Accesso online:https://doi.org/10.5281/zenodo.14787338
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  • <p><strong>Title:</strong> <em>Comparison of the Unified Informational Spin Theory (TGU) with the <span><span>Λ\Lambda</span><span><span><span>Λ</span></span></span></span>CDM Model: An Approach Based on Three Experiments</em></p> <p><strong>Abstract:</strong><br>This paper investigates the potential of the <strong>Unified Informational Spin Theory (TGU)</strong> as an alternative to the <strong><span><span>Λ\Lambda</span><span><span><span>Λ</span></span></span></span>CDM model</strong>, aiming to describe gravitational phenomena without the need for dark matter. The study employs <strong>three experiments</strong> to compare the two models:</p> <ol> <li><strong>Cosmic Structures</strong> – Examining the gravitational stability of the <strong>Hercules–Corona Borealis Great Wall</strong>.</li> <li><strong>Planetary System Dynamics</strong> – Analyzing orbital period predictions for <strong>TRAPPIST-1</strong> and <strong>Kepler-90</strong>.</li> <li><strong>Gravitational Lensing</strong> – Comparing Einstein radii predictions in gravitational lensing systems.</li> </ol> <p>The results demonstrate that <strong>TGU accurately models large-scale cosmic structures, planetary orbits, and gravitational lensing effects without invoking dark matter</strong>. Instead, it explains these phenomena through <strong>informational coherence</strong>, a concept that replaces the need for unseen mass. Statistical analysis shows that <strong>TGU predictions align closely with observational data</strong>, often outperforming <span><span>Λ\Lambda</span><span><span><span>Λ</span></span></span></span>CDM, especially in planetary system dynamics.</p> <p>The study concludes that <strong>TGU provides a viable alternative to the standard cosmological model</strong>, redefining gravitational interactions through informational structures. Future research will further test this approach with observational data and explore its broader astrophysical applications.</p>