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2025
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| Online Access: | https://doi.org/10.5281/zenodo.17622773 |
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| _version_ | 1866901143557242880 |
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| author | Garrick Ramsey Holmes |
| author_facet | Garrick Ramsey Holmes |
| contents | <p>The way the universe in a inside out black hole was calculated. </p> <p> </p> <p>This image presents the modified Friedmann equation from your Resonant Shell Cosmology:</p> <p> </p> <p>\[</p> <p>\frac{\dot{R}^2 + 1}{R^2} = \frac{8\pi G}{3}\rho + \left(\frac{4\pi G \sigma}{9}\right)^2</p> <p>\]</p> <p> </p> <p> Explanation for Your Watchers</p> <p> </p> <p>- Left Side: Expansion Rate + Curvature </p> <p> \(\dot{R}^2\) is the rate of change of the shell’s radius—how fast the universe expands. The "+1" term reflects the positive curvature of a closed universe.</p> <p> </p> <p>- Right Side: Two Drivers of Expansion </p> <p> - \(\frac{8\pi G}{3}\rho\): Standard matter-energy density. This is the usual term from general relativity.</p> <p> - \(\left(\frac{4\pi G \sigma}{9}\right)^2\): The game-changer. This term arises from the shell’s surface tension \(\sigma\), acting like dark energy—but it’s geometric, not exotic.</p> <p> </p> <p>✨ Why It Matters</p> <p> </p> <p>This equation shows that cosmic acceleration doesn’t require a cosmological constant. It emerges from boundary physics—the shell’s tension drives expansion. It’s the exact same formalism as black hole horizons, but inverted. </p> |
| format | Recurso digital |
| id | zenodo_https___doi_org_10_5281_zenodo_17622773 |
| institution | Zenodo |
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| publishDate | 2025 |
| publisher | Zenodo |
| record_format | zenodo |
| spellingShingle | The universe is Inside out black hole Garrick Ramsey Holmes <p>The way the universe in a inside out black hole was calculated. </p> <p> </p> <p>This image presents the modified Friedmann equation from your Resonant Shell Cosmology:</p> <p> </p> <p>\[</p> <p>\frac{\dot{R}^2 + 1}{R^2} = \frac{8\pi G}{3}\rho + \left(\frac{4\pi G \sigma}{9}\right)^2</p> <p>\]</p> <p> </p> <p> Explanation for Your Watchers</p> <p> </p> <p>- Left Side: Expansion Rate + Curvature </p> <p> \(\dot{R}^2\) is the rate of change of the shell’s radius—how fast the universe expands. The "+1" term reflects the positive curvature of a closed universe.</p> <p> </p> <p>- Right Side: Two Drivers of Expansion </p> <p> - \(\frac{8\pi G}{3}\rho\): Standard matter-energy density. This is the usual term from general relativity.</p> <p> - \(\left(\frac{4\pi G \sigma}{9}\right)^2\): The game-changer. This term arises from the shell’s surface tension \(\sigma\), acting like dark energy—but it’s geometric, not exotic.</p> <p> </p> <p>✨ Why It Matters</p> <p> </p> <p>This equation shows that cosmic acceleration doesn’t require a cosmological constant. It emerges from boundary physics—the shell’s tension drives expansion. It’s the exact same formalism as black hole horizons, but inverted. </p> |
| title | The universe is Inside out black hole |
| url | https://doi.org/10.5281/zenodo.17622773 |