Black Holes as Sector Boundaries in Coherent Gravity Theory (CGT)
Abstract
Proposes a CGT black-hole mechanism paper: the horizon is treated as a commitment surface for eventual delocalization in the internal-sector structure at Planckian curvature, while exterior physics remains Einstein--Hilbert dominated (Wald-entropy route). The visible reduced state can appear mixed by partial trace over dark sectors (assumptions stated explicitly). Specifies a minimal curvature--localization EFT for an order parameter $\sigma$ (localization width in the normal bundle) and states a required mass-gap constraint to suppress dark-sector Hawking power at $\omega\sim T_H$ while allowing interior absorption at blue-shifted $\omega\sim M_P$.For a series overview, reading order, and claim‑hygiene guide, see Coherent Gravity Theory (CGT): An Onboarding Primer: https://doi.org/10.5281/zenodo.18212967
Fields of Study & Subjects
Black Holes and Theoretical Physics
Cosmology and Gravitation Theories
Noncommutative and Quantum Gravity Theories
Publication details
- Journal / source
- Zenodo (CERN European Organization for Nuclear Research)
- Publication date
- 14 January 2026
- Document type
- Preprint