Data Analysis of Cassiopeia A (Cas A) Based on XRISM Resolve Observations (FUH)

This paper presents an independent audit of XRISM Resolve X-ray data for the Cassiopeia A (Cas A) supernova remnant. The analysis identifies systemic anomalies that support the Fermion Ocean Hypothesis (FUH). Key findings include the detection of differential viscous broadening in heavy iron spectral lines and the recording of a background medium resonance at 4.8 keV. The study theoretically explains the anomalously high shell temperature as a "friction tax" — the dissipation of kinetic energy within the viscous spatial medium. Imaging in the 4–7 keV range confirms the Potter Effect, manifested as the suppression of thermal plasma diffusion.