Gluonic Confinement and Tidal Forces Near Black Holes

We analyze tidal disruption of quark confinement near black holes using Kruskal-Szekeres coordinates and quantum gravity frameworks. Externally, tidal forces remain 1025× weaker than QCD binding requirements. Within the event horizon, rip reactions (quark-antiquark pair cascades) become geometrically possible but are suppressed by Planck-scale effects. Using multi-scale analysis, we demonstrate no observable mass loss occurs due to horizon confinement, preserving black hole thermodynamics. This work bridges quantum chromodynamics and general relativity in extreme gravitational regimes.