Constructing the nonlinear Harrison Core, functionality-saturation regime, and exact distribution of infalling matter and energy.
Programme Overview
This program investigates the interior of an HGUT black hole as an extreme structural state of the substrate rather than a geometric singularity. It combines the regular-interior problem with the proposed two-channel distribution of energy between the Harrison Core and the surrounding structural or exhaust response.
Immediate Milestone
Derive a controlled static interior solution that matches the known exterior field while avoiding singular behavior.
Active Objectives
Construct a regular nonlinear interior solution.
Define the Harrison Core mathematically.
Determine whether functionality approaches zero.
Match the interior to the exterior gravitational field.
Derive the exact two-channel partition law.
Track energy, topology, charge, and information.
Recover black-hole thermodynamic behavior.
Identify observable departures from general relativity.
Evidence Trail
This ledger records the mathematical, computational, conceptual, and numerical work already completed within this programme.
An exterior inverse-square gravitational field has been derived.
The structural-well interpretation of black holes has been established conceptually.
The Harrison Core has been proposed as the interior organizing structure.
Functionality saturation has been identified as a candidate horizon mechanism.
A two-channel energy-distribution architecture has been proposed.
The exact nonlinear interior and partition law remain open.
Shared Mathematical Foundation
The master Lagrangian and baseline displacement, phase, interaction, and conservation equations are already established. The work on this page concerns solving, validating, extending, and testing their consequences in this specific physical sector.
Active Research
Successful derivations, failed simulations, replications, corrections, and falsifying evidence all belong in the evidence trail.
