Zhan-Feng Mai, Run-Qiu Yang

This paper numerically studies the time evolution of s-wave scalar probe field in a black hole of which the event horizon is surrounded by matter. As a toy model, it encodes the effects of matter into deformations of Regge-Wheeler potential. It considers three different types of local deformations in the vicinity of the event horizon, the negative static bump potential, the stochastic potential and bump potential modulated by time function in low frequency limit. Our numerical results show that infinitesimal local deformations on Regge-Wheeler potential near the horizon can overturn stability of an arbitrarily strongly stable black hole, implying that late-time behavior of a stable black hole is extremely sensitive to geometry near horizon. Specially, certain deformations that stabilize systems in flat backgrounds can destabilize otherwise stable black holes. It also shows that horizon-induced redshift transforms near-horizon quantum fluctuations into classical-scale stochastic deformations capable of triggering instability, implying that even an isolated black hole cannot keep stable in extended timescales.