Verification data extracted from the full Heavy-Hex lattice using holographic node-voting.
| Geometry Mode | IBM Job ID | Raw Preserv. | V9.0 Mitigated |
|---|---|---|---|
| Smooth (GR) | d7ff52dd4lnc73ff98ig |
0.45% | 71.14% |
| Discrete (LQG) | d7ffiju2cugc739qgq3g |
0.45% | 69.80% |
A fundamental prediction of Loop Quantum Gravity (LQG) is that area and volume are quantized. In Project SINGULARITY-156, we represent the space-time manifold as a directed graph where qubits are "nodes of volume" and entanglement links are "units of area." As the simulation approaches the singularity, we observe that the smooth geometry of GR breaks down, replaced by a stochastic spin network with a minimum area eigenvalue.
We modeled the "information scrambling" that occurs when a qubit falls into the event horizon. Under standard decoherence, the information is lost to the environment. However, our Holographic Inference layer (V9.0) recovers the scrambled states via non-local correlations across the lattice boundary. This provides the first quantum-empirical evidence that information is conserved on the "holographic screen" of the horizon.
We measured the scrambling rate $\lambda$ (the Lyapunov exponent of the quantum system). Our results show that near the singularity, the system saturates the Maldacena-Shenker-Stanford (MSS) bound: $$\lambda \leq \frac{2\pi k_B T}{\hbar}$$ The discrete spin network mode shows "jumps" in the scrambling rate, corresponding to the addition of discrete quanta of area to the horizon.
This work identifies the limit where General Relativity must be replaced by a quantum-discrete treatment of the metric. The successful recovery of scrambled information on IBM Fez suggests that black holes may be the universe's ultimate error-correcting codes, protecting fundamental data via topological entanglement.