This 3D numerical framework introduces the Dynamic Local Mass Clustering (DLMC) paradigm as a robust alternative to collisionless dark matter particles. Unlike traditional MOND or CDM models, the DLMC hypothesis resolves the Bullet Cluster (1E 0657-56) paradox through Flux Inertia. The observed spatial decoupling between baryons and potential peaks corresponds to a dynamic lag of the local curvature response, rather than a particle-based separation. By unifying the Radial Acceleration Relation (RAR) at the galactic scale with gravitational lensing at the cluster scale via vacuum coupling coefficients, this model provides a continuous hybrid solution to the "Missing Mass" problem across all cosmic scales. Included files: Jupyter Notebook (.ipynb) Python scripts (.py) CSV files of DLMC analyses and maps PNG images of outputs PDF of the full report HTML and Markdown files for reference This resource allows researchers to reproduce, analyze, and extend the DLMC framework, offering a complete tool for studying galactic structures and clusters under modified gravity conditions.