The Heisenberg Uncertainty Principle as a Cosmological Relic (Brane-Bulk Series, Paper IV)
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2026
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| author | Jagadeesan, Bharathi Dasan |
| author_facet | Jagadeesan, Bharathi Dasan |
| contents | <p>Click in the Description box and paste: <em>"ℏ(t) ∝ H(t)³ from brane oscillation mode quantisation. With c(t)∝H(t) from Paper III, M_Ch(z)∝H(z)⁶ gives super-Chandrasekhar BH seeds at z=5−10 consistent with LRD BH masses 10⁵−10⁷ solar masses (Nature 2026, Prediction 51 confirmed). Heisenberg uncertainty is a cosmologically time-varying constraint. Part of the One Octonion series (Papers I–XL), anchor DOI:10.5281/zenodo.19120873."</em></p> |
| format | Recurso digital |
| id | zenodo_https___doi_org_10_5281_zenodo_19132971 |
| institution | Zenodo |
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| publishDate | 2026 |
| publisher | Zenodo |
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| spellingShingle | The Heisenberg Uncertainty Principle as a Cosmological Relic (Brane-Bulk Series, Paper IV) Jagadeesan, Bharathi Dasan <p>Click in the Description box and paste: <em>"ℏ(t) ∝ H(t)³ from brane oscillation mode quantisation. With c(t)∝H(t) from Paper III, M_Ch(z)∝H(z)⁶ gives super-Chandrasekhar BH seeds at z=5−10 consistent with LRD BH masses 10⁵−10⁷ solar masses (Nature 2026, Prediction 51 confirmed). Heisenberg uncertainty is a cosmologically time-varying constraint. Part of the One Octonion series (Papers I–XL), anchor DOI:10.5281/zenodo.19120873."</em></p> |
| title | The Heisenberg Uncertainty Principle as a Cosmological Relic (Brane-Bulk Series, Paper IV) |
| url | https://doi.org/10.5281/zenodo.19132971 |