Black Holes and Horizon Structure

This research area studies horizon-like behavior in Coherence Geometry, including curvature trapping, boundary emission, information flow, gravitational analogues, and radiative flux from coherence-bound regions. Rather than treating horizons only through the standard spacetime or semiclassical formulations, these papers investigate how horizon-like interfaces can arise from internal amplitude-phase dynamics, curvature strain, coherence confinement, and projection.

Representative peak-emission frame from the horizon-like coherence simulation. A curvature-bound coherence region emits outward radial structure from its rim, producing a visible radiative shell. In the associated paper, these time-resolved fields are analyzed through rim-flux measurements that exhibit inverse-square scaling with boundary radius.

The goal is to understand which features of black-hole and horizon physics may reflect more general geometric mechanisms within structured coherence fields.

Publication List