The Reissner-Nordström black hole with the fastest relaxation rate

Abstract

Numerous {\it numerical} investigations of the quasinormal resonant spectra of Kerr-Newman black holes have revealed the interesting fact that the characteristic relaxation times $τ({\bar a},{\bar Q})$ of these canonical black-hole spacetimes can be described by a two-dimensional function ${\bar τ}\equiv τ/M$ which increases monotonically with increasing values of the dimensionless angular-momentum parameter ${\bar a}\equiv J/M^2$ and, in addition, is characterized by a non-trivial ({\it non}-monotonic) functional dependence on the dimensionless charge parameter ${\bar Q}\equiv Q/M$. In particular, previous numerical investigations have indicated that, within the family of spherically symmetric charged Reissner-Nordström 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-Nordström 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 ${\bar Q}={\sqrt{51-3\sqrt{33}}\over{8}}\simeq 0.73$ is characterized by the {\it fastest} relaxation rate (the smallest dimensionless relaxation time ${\bar τ}$) within the family of charged Reissner-Nordström black-hole spacetimes.