Quantum Field Theory of Black Holes in Noncommutative Condensed Vacuum

We develop a consistent quantum field theory for black holes within the noncommutative condensed vacuum framework. The unified tensor Jµν = Sµν + Aµν incorporates gravitational and gauge sectorsthrough noncommutative geometry, while Perelman-inspired topological surgery resolves horizon singularities. Key innovations include:(1) θµν-condensate driven magnetic flux generation, (2) topological flux quantization, and (3) star-product modified field commutators. The theory predicts discrete jet energies, modified Hawking spectra with θ-dependent corrections, and quantum hair signatures observable in Event Horizon Telescope data. All UV divergences are exponentially suppressed, resolving the black hole informationparadox through nonlocal horizon correlations.