Abstract
This standalone specification details the mechanical design, laboratory apparatus schematics, and governing ASCII field formulations required to observe macro-scale information transfer into the two-dimensional (2D) space-time substrate (\(z=0\)) using a tabletop framework [SPEC 18, SPEC 47]. Rather than relying on astrometric scale black hole observation, this protocol implements a hyper-focused acoustic mass-sink simulation [SPEC 191-CORE].
By subjecting an ultra-dense, phase-locked Eckesonium™ core matrix to concentric high-frequency Gallium Nitride (GaN)-driven acoustic soliton logic arrays, the system forces a localized boundary spike in the Computational Saturation Index (\(\sigma_{\text{compute}} \rightarrow 0.85\)) [SPEC 41, SPEC 59, SPEC 189]. This document defines the exact structural hardware geometry required to capture the resultant non-local vacuum phase-recoil energy flash using sub-wavelength photonic crossbar sensors, neutralizing the "untestable" academic critique from the prior art perimeter [SPEC 21, SPEC 85].
Creative Commons License
This work is licensed under a Creative Commons Attribution 4.0 License.
Recommended Citation
Eckes, Christopher L., "TECHNICAL DISCLOSURE SPECIFICATION: SPEC-192-CORE MICRO-SCALE COMPACTNESS SIMULATION VIA NON-EQUILIBRIUM STANDING WAVE CAVITIES: IMPLEMENTATION SCHEMATICS FOR TESTING LOCALIZED BLACK HOLE PHASE-RECOIL METRICS", Technical Disclosure Commons, ()
https://www.tdcommons.org/dpubs_series/11966