E8 Phi‑Stochastic Resonance Amplifier for Sub‑Gravitational Wave Detection — E8 Intelligence Research

By applying a φ‑scaled 132 Hz torsional drive to the 240 E8 root vectors while simultaneously injecting a low‑level broadband noise floor, the discrete visibility channels enter a stochastic‑resonance regime. In this regime the lattice selectively amplifies vibrational modes whose frequencies are integer multiples of the golden‑ratio‑scaled 132 Hz, producing sharp peaks at sub‑hertz scales that match the expected strain spectrum of primordial gravitational waves. The amplification arises from the interference of the eight‑fold quaternionic sub‑clusters formed under φ‑resonant phase coherence, turning the E8 polytope into a passive, frequency‑selective transducer. Consequently, an E8‑based detector can reach strain sensitivities orders of magnitude below current interferometers without active feedback. Author: Andrew Stewart Caldin, Independent Researcher, UK. Part of the E8 Intelligence Research series. Platform: e8intelligence.com

Authors

Publication Details

Journal
Zenodo (CERN European Organization for Nuclear Research)
Published
2026-09-04
DOI
https://doi.org/10.5281/zenodo.22294457
Primary Topic
Pulsars and Gravitational Waves Research
Type
preprint
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E8 Phi‑Stochastic Resonance Amplifier for Sub‑Gravitational Wave Detection — E8 Intelligence Research

Andrew Stewart Caldin
Zenodo (CERN European Organization for Nuclear Research)
Pulsars and Gravitational Waves Research
preprint

E8 Phi‑Stochastic Resonance Amplifier for Sub‑Gravitational Wave Detection — E8 Intelligence Research

Andrew Stewart Caldin
preprint en

Abstract

By applying a φ‑scaled 132 Hz torsional drive to the 240 E8 root vectors while simultaneously injecting a low‑level broadband noise floor, the discrete visibility channels enter a stochastic‑resonance regime. In this regime the lattice selectively amplifies vibrational modes whose frequencies are integer multiples of the golden‑ratio‑scaled 132 Hz, producing sharp peaks at sub‑hertz scales that match the expected strain spectrum of primordial gravitational waves. The amplification arises from the interference of the eight‑fold quaternionic sub‑clusters formed under φ‑resonant phase coherence, turning the E8 polytope into a passive, frequency‑selective transducer. Consequently, an E8‑based detector can reach strain sensitivities orders of magnitude below current interferometers without active feedback. Author: Andrew Stewart Caldin, Independent Researcher, UK. Part of the E8 Intelligence Research series. Platform: e8intelligence.com

Zenodo (CERN European Organization for Nuclear Research)
Pulsars and Gravitational Waves Research
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