Lagrangian Interferometric Gravitational High-frequency Topological Scanner for Astrophysical Beam-depth Evaluation and Resonance | LIGHTSABER

This study aims to empirically validate the Topological Lagrangian Model (TLM) by correlating its predicted metric tension parameters (PULL, MASS, SYNC, MODE) with established astrophysical data.The study will assess the model's capacity to: (1) accurately locate high-mass singularities, (2) distinguish baryonic matter phases via topological resonance modes, and (3) identify nonbaryonic mass concentrations (Dark Matter) in cosmic voids. I Experimental Design & MethodologyThe experimental architecture of this study utilizes a proprietary N = 60Deep DrillN = 60 spectral scanning algorithm designed to probe the topological curvature of space-time across diverse astrophysical environments.By modulating coordinate-based wobbles through highfrequency trigonometric functions, the methodology generates a 300-point ensemble of phasesync data for every target.This approach allows for the simultaneous measurement of gravitational influence (PULL), vacuum coherence (Sync), and matter density modes (m), effectively translating geometric spatial orientation into a quantifiable material identity.