The Reissner-Nordstr\"om black hole with the fastest relaxation rate

Numerous {\it numerical} investigations of the quasinormal resonant spectra of Kerr-Newman black holes have revealed the interesting fact that the characteristic relaxation times $\tau (\bar{a},\bar{Q})$ of these canonical black-hole spacetimes can be described by a two-dimensional function ${\bar \tau}\equiv \tau/M$ which increases monotonically with increasing values of the dimensionless angular-momentum parameter $\bar{a}\equiv J\mathrm{/}{M}^2$ and, in addition, is characterized by a non-trivial ({\it non}-monotonic) functional dependence on the dimensionless charge parameter $\bar{Q}\equiv Q\mathrm{/}M$. In particular, previous numerical investigations have indicated that, within the family of spherically symmetric charged Reissner-Nordstr"om spacetimes, the black hole with $\bar{Q}\simeq 0.7$ has the {\it fastest} relaxation rate. In the present paper we use {\it analytical} techniques in order to investigate this intriguing non-monotonic functional dependence of the Reissner-Nordstr"om black-hole relaxation rates on the dimensionless physical parameter $\bar{Q}$. In particular, it is proved that, in the eikonal (geometric-optics) regime, the black hole with $\bar{Q}=\frac{\sqrt{51-3\sqrt{33}}}{8}\simeq 0.73$ is characterized by the {\it fastest} relaxation rate (the smallest dimensionless relaxation time $\bar{\tau }$) within the family of charged Reissner-Nordstr"om black-hole spacetimes.