Infinitesimal negative or stochastic near-horizon deformations of the Regge-Wheeler potential can destabilize an otherwise stable Schwarzschild black hole in a toy scalar-field model.
The quasi- normal modes of the Schwarzschild black hole,
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Numerical study on the robustness of the stability for stable black holes
Infinitesimal negative or stochastic near-horizon deformations of the Regge-Wheeler potential can destabilize an otherwise stable Schwarzschild black hole in a toy scalar-field model.