Black Holes as Sector Boundaries in Coherent Gravity Theory (CGT)

Black Holes as Sector Boundaries in CGT Proposes a CGT-specific black-hole mechanism paper: the event horizon is treated as a commitment surface for eventual delocalization in the internal sector structure at Planckian curvature. The visible reduced state appears thermal by partial trace over dark sectors (typicality/scrambling assumption), while the exterior remains Einstein–Hilbert dominated (Wald entropy route). The paper specifies a minimal curvature–localization EFT for an order parameter σ (localization width in the normal bundle) and states a required mass-gap constraint to avoid dark-sector Hawking power at \(\omega\sim T_H\) while allowing interior absorption at blue-shifted \(\omega\sim M_P\). A KK-first twisted-boundary mechanism and a semi-explicit flux-quantized proxy estimate are included as scale guidance; coefficient-level UV derivations are explicitly marked as future work.