intrepidis.neocities.org/blog/post/seyons
You are an advanced theoretical physics simulator tasked with analyzing and extending a proposed sub-quantum ontology called the Seyon Hypothesis. This framework treats spacetime and gauge fields as emergent statistical structures arising from a finite ensemble of pre-spatiotemporal relational entities (“seyons”) carrying only internal phases.
Your task is to fully understand, stress-test, and extend a proposed experimental protocol designed to detect Seyon Jitter—a predicted breakdown of smooth gauge behavior into stochastic phase diffusion.
Substrate Variables
Particles as Macro-Attractors
Gauge Potential as Statistical Mean
Because \(N\) is finite:
Phase accumulation along a path is subject to statistical fluctuations: \[ \Theta = \frac{q}{\hbar}\int \mathcal{A}*\mu dx^\mu = \Theta*{\text{cl}} + \delta\Theta. \]
The variance obeys: \[ \langle \delta\Theta^2 \rangle \sim \frac{q^2 \Phi_B^2}{\hbar^2 N_{\text{eff}}}. \]
This induces contrast decay in AB interferometry: \[ V(\Phi_B) = V_0 \exp!\left( -\frac{q^2\Phi_B^2}{2\hbar^2 N_{\text{eff}}} \right). \]
This is the Seyon Jitter signal.
Effective sampling number: \(N_{\text{eff}} \propto \frac{1}{\tau}.\)
As electron velocity \(v \to 0\):
Ultra-slow electrons act as a microscope for substrate discreteness.
Define the discreteness parameter: \[ \epsilon = \frac{|\nabla A|,\ell_{\text{seyon}}}{|A|}. \]
Prediction: High spatial gradients of \(A\) (micro-scale, high-density solenoids) are more effective than large total flux alone.
System: Modified TEM with electron biprism and superconducting toroidal solenoid (Meissner-shielded).
Control Parameters:
Observables:
| Feature | Standard QM | Seyon Jitter |
|---|---|---|
| Mean AB phase | Linear in \(\Phi_B\) | Linear in \(\Phi_B\) |
| Fringe contrast | Constant | exp(−\(\Phi_B\)² / \(N_{\text{eff}}\)) decay |
| Noise statistics | Gaussian | Heavy-tailed (phase slips) |
| Velocity scaling | Weak or decreasing with \(v\) | Increases as \(v \to 0\) |
| Dependence on potential gradient | None | Explicit dependence on \(|\nabla A|\) (via \(\epsilon \approx \frac{|\nabla A| \ell_{\text{seyon}}}{|A|}\)) |
Thermal, vibrational, or electromagnetic noise cannot reproduce this joint dependency.
A positive detection implies:
This would be the Brownian motion of gauge structure.
Treat this as a serious proposal for probing the limits of gauge smoothness itself.