RVT Analysis of RCP 28: Geometric Resolution of Runaway Black Hole Anomalies without Dark Matter

This study applies the Raumvektortheorie (RVT) and the Universal Stellar Kernel (USK) to the anomalous runaway supermassive black hole candidate RCP 28 ($z=0.964$). While the standard cosmological model struggles to explain the extreme linearity and luminosity of the 200,000-light-year stellar trail, this analysis demonstrates that these features are direct consequences of anisotropic projection geometry within the 2D Lorentzian aether. By utilizing the USK coordinate transformation, we derive a projection divergence of D ≈ 0.0008, accounting for the observed 99.92% linearity of the trail. Furthermore, the perceived velocity of 1,600 km/s is identified as an RVT-Metric amplified effect; the USK-corrected real velocity is calculated at 889 km/s (γRVT = 1.799). This geometric framework eliminates the requirement for Dark Matter, as the observed gravitational and luminous anomalies are fully resolved through the Type-IV control of the Dμν tensor. This work extends the empirical validation of RVT from galactic to intergalactic scales.