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| 主要な著者: | , |
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| フォーマット: | Recurso digital |
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Zenodo
2026
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| 主題: | |
| オンライン・アクセス: | https://doi.org/10.5281/zenodo.20402048 |
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目次:
- Cosmogenic companion (Paper 22) of the NWT program. A black-hole cosmogenesis scenario in which a daughter universe nucleates from a near-extremal Kerr black hole and inherits a no-hair tuple (Planck mass, spin axis, so(7) substrate algebra, chirality sign). From the single dimensional anchor M_Pl plus the inherited substrate algebra, Standard-Model and cosmological observables follow with zero free continuously-adjustable dimensionless parameters: eta_B = (3/14) alpha^4, Omega_b/Omega_c = 25 alpha + 75 alpha^2, n_s = 1 - h_v alpha, r = 48 alpha^2, the electroweak/Higgs sector, gauge unification at alpha_GUT^-1 = 25, and a discrete dark-matter mass tower. Companion to Papers 21a and 21b.