Quantum Mapping of Local Dark Matter Filaments: Subhalo Density Structures Within 10 Parsecs of the Solar System

This study performs a high-precision quantum-field gradient reconstruction of dark matter density in the immediate Solar neighborhood. Using the Lumenis IO Earth Engine’s quantum tensor solver, the simulation resolved fine-scale subhalo filaments and vacuum energy gradients within a radius of 10 parsecs.The results indicate subtle anisotropies in the local dark matter field, with detectable interference between electroweak residuals and quantum vacuum energy. This provides the most detailed spatial model to date of dark-matter filamentation near the Solar System, revealing potential coupling between baryonic mass distribution and subhalo dynamics on microparsec scales.