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

Abstract: 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 $D \approx 0.0008$, accounting for the observed 99.92% linearity of the trail. Furthermore, the perceived velocity of $1,600 \text{ km/s}$ is identified as an RVT-Metric amplified effect; the USK-corrected real velocity is calculated at $889 \text{ km/s}$ ($\gamma_{RVT} = 1.799$). 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 $D_{\mu\nu}$ tensor. This work extends the empirical validation of RVT from galactic to intergalactic scales.