Theoretical exploration unveils Hawking temperature in black holes, suggesting new acoustic horizons.
UCM Paper 37 (Theoretical). In the UCM, the substrate flow v_flow = c√(R_s/r) reaches the speed of light exactly at the Schwarzschild radius (Theorem 1, from Paper 35). This makes every black hole an acoustic black hole for sub-threshold modes: no cell mode escapes for r < R_s (Theorem 2). The surface gravity κ = c⁴/(4GM) follows from the flow gradient, and the Hawking temperature T_H = ℏc³/(8πGMk_B) follows from the Unruh effect applied to the substrate (Theorem 3) — reproducing the known result (6.2×10⁻⁸ K for a solar-mass BH) without postulates. Two physical layers at the horizon: cell modes trapped, membrane phase free (→ Paper 38). UCM preprint series on Zenodo, ORCID 0009-0005-5088-4339.
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Norbert Prebeck (2026) studied this question.
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