摘要
The fundamental quasinormal resonances of charged Reissner-Nordstr枚m black holes due to charged scalar perturbations are derived analytically. In the WKB regime, , we obtain a simple expression for the fundamental quasinormal resonances: , where and Q are the temperature and electric charge of the black hole and q is the electric charge of the field. Remarkably, our results show that the relaxation dynamics of a perturbed Reissner-Nordstr枚m black hole may saturate the recently proposed universal relaxation bound.