TVVVV - JWST based on early torsion Black holes

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Authors: Daniel Parma
Cited by: 0

Abstract

This preprint develops the TVVVV framework, a torsion‑driven cosmological model that provides a natural explanation for the unexpectedly early appearance of massive black holes observed by JWST at redshifts \(z \sim 10–15\). In this theory, spacetime consists of two regimes: an entangled, pre‑geometric S‑regime and a localized M‑regime associated with matter formation. The transition between these regimes is controlled by a torsion invariant and a logarithmic comoving‑distance kernel that mediates long‑range information flow. Applying this structure to high‑redshift black holes, the model predicts a torsion‑induced Lindblad dissipation rate \[ \Gamma_{\rm JWST} \sim 10^{-19}\,\mathrm{s^{-1}}, \] corresponding to an information‑exchange timescale of \(\tau{\rm diss} \sim 10^{11}\) years. Because the early universe satisfies \(t{\rm cosmic} \ll \tau{\rm diss}\), massive black holes do not need to grow through accretion; instead, they appear as direct projections of the S‑regime during the S→M transition. This mechanism naturally produces \(10^6–10^8 M\odot\) black holes only a few hundred million years after the Big Bang, matching JWST observations without invoking exotic seeds, super‑Eddington accretion, or inflationary enhancements. The TVVVV framework therefore offers a unified geometric explanation for early structure formation, ER=EPR information transport, and the rapid emergence of compact objects in the young universe.

Fields of Study & Subjects

Cosmology and Gravitation Theories Black Holes and Theoretical Physics Galaxies: Formation Evolution Phenomena

Publication details

Journal / source
Zenodo (CERN European Organization for Nuclear Research)
Publication date
3 February 2026
Document type
Preprint