For the coherent quantum black hole geometry, scalar, electromagnetic, and gravitational quasinormal mode frequencies deviate from Schwarzschild by about 0.5% for a small core and up to roughly 5% in damping for a core at 70% of the Schwarzschild radius.
Black Hole Normal Modes: A WKB Approach. 1. Foundations and Application of a Higher Order WKB Analysis of Potential Barrier Scattering,
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Quasinormal modes for coherent quantum black holes
For the coherent quantum black hole geometry, scalar, electromagnetic, and gravitational quasinormal mode frequencies deviate from Schwarzschild by about 0.5% for a small core and up to roughly 5% in damping for a core at 70% of the Schwarzschild radius.