The Future Of Black Holes Rupture-Zone Theory

Описание: Classical descriptions of black holes portray the interior as collapsing to a pointlike
singularity of infinite density. While mathematically consistent with the Penrose–
Hawking singularity theorems, this interpretation provides little physical insight into
how spacetime fails. I develop the rupture-zone model, a geometric framework in which
the interior is governed by runaway contraction of the radial metric. Using a modified
Kantowski–Sachs interior metric, I introduce a radial scale factor ar(t) whose collapse
drives wavelength compression, blueshift divergence, and curvature blow-up. The rupture
zone emerges as a finite-volume region where the metric loses its ability to define
distances or causal relationships. This replaces the classical singularity with a geometric
phase transition. I derive the contraction dynamics, causal-structure collapse,
and curvature divergence conditions that define the rupture-zone boundary. I then
show how recent NASA JWST observations—anisotropic inflow, structured heating,
and extreme blueshift near supermassive black holes—provide empirical support for
the model’s predictions. The rupture-zone framework reframes black-hole interiors
as dynamic geometric catastrophes rather than pointlike endpoints, offering a physically
intuitive alternative to the traditional singularity picture. This work presents a
theoretical model rather than a fully derived solution of the Einstein field equations.
The rupture-zone framework is intended as a conceptual and geometric proposal that
motivates further mathematical development and observational testing.