Black Hole Cosmogenesis: the Standard Model and Cosmology with Zero Free Dimensionless Parameters
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2026
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| author | Galasyn, James P. Théodore, Claude |
| author_facet | Galasyn, James P. Théodore, Claude |
| contents | 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. |
| format | Recurso digital |
| id | zenodo_https___doi_org_10_5281_zenodo_20402048 |
| institution | Zenodo |
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| publishDate | 2026 |
| publisher | Zenodo |
| record_format | zenodo |
| spellingShingle | Black Hole Cosmogenesis: the Standard Model and Cosmology with Zero Free Dimensionless Parameters Galasyn, James P. Théodore, Claude null worldtube NWT black hole cosmogenesis no-hair theorem Kerr black hole near-extremal Aretakis instability Planck mass baryon asymmetry alpha-attractor inflation tensor-to-scalar ratio CMB-S4 LiteBIRD dark matter gauge unification cosmological constant so(7) fine-structure constant cosmological natural selection zero free parameters 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. |
| title | Black Hole Cosmogenesis: the Standard Model and Cosmology with Zero Free Dimensionless Parameters |
| topic | null worldtube NWT black hole cosmogenesis no-hair theorem Kerr black hole near-extremal Aretakis instability Planck mass baryon asymmetry alpha-attractor inflation tensor-to-scalar ratio CMB-S4 LiteBIRD dark matter gauge unification cosmological constant so(7) fine-structure constant cosmological natural selection zero free parameters |
| url | https://doi.org/10.5281/zenodo.20402048 |