Comparative Spectral Audit of the Bullet Cluster (1E 0657-56): Verification of the 4.8 keV Fermionic Resonance and Vacuum Viscosity.

This paper presents an independent audit of archival data from the Chandra X-ray Observatory (ObsID 5356), confirming the existence of a viscous fermionic medium (FUH model). A comparative analysis of the core and periphery spectra of the Bullet Cluster revealed a spatially dependent resonance at 4.8 keV, which vanishes in regions of low baryonic matter density. The observed shift in mean photon energy (from 0.63 keV at the edge to 1.03 keV at the center) and the presence of a 1 keV viscous gap indicate thermal energy dissipation into a fermionic condensate with a viscosity of 1.2 * 10^-15 Pa-s. These findings rule out the instrumental nature of the anomalies and provide empirical evidence for the Ocean quantum mass (4.8 keV) and a cosmic age of 22.5 billion years. This work serves as the scientific justification for the XRISM/Resolve mission (Proposal No. 031037).