Theoretical analysis reveals geometric accumulation of spacetime jitter in discrete D4 models, indicating Michelson interferometers inherently filter noise into instrument blind spots.
This addendum addresses the false dichotomy between broadband stochastic noise and narrow-line kinematic harmonics in discrete D4 spacetime models. It demonstrates that the spatial jitter inherent to a computational substrate does not require the universe to tune its fundamental frequency to a specific macroscopic instrument. Rather, the interferometer’s own causal baseline acts as a physical matched filter, forcing the geometric accumulation of the broadband jitter to peak precisely at the inverse light-crossing time (fc = c/2L), which perfectly coincides with the Michelson topology’s mathematical blind spot.
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Paul Masic Jr. (2026) studied this question.
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