Quasinormal modes of dilatonic Reissner-Nordstr\"om black holes

TL;DR

This paper computes the quasinormal modes of dilatonic Reissner-Nordstr"om black holes, revealing how their spectra depend on charge and dilaton coupling, with significant deviations from classical modes at high charge and coupling.

Contribution

It provides the first detailed analysis of quasinormal modes for dilatonic Reissner-Nordstr"om black holes across various parameters, highlighting deviations from standard black hole spectra.

Findings

Spectrum includes five families of modes: gravitational, electromagnetic, and scalar.

Large charge and dilaton coupling cause strong deviations from Reissner-Nordstr"om modes.

Isospectrality is broken at high charge values.

Abstract

We calculate the quasinormal modes of static spherically symmetric dilatonic Reissner-Nordstr\"om black holes for general values of the electric charge and of the dilaton coupling constant. The spectrum of quasinormal modes is composed of five families of modes: polar and axial gravitational-led modes, polar and axial electromagnetic-led modes, and polar scalar-led modes. We make a quantitative analysis of the spectrum, revealing its dependence on the electric charge and on the dilaton coupling constant. For large electric charge and large dilaton coupling, strong deviations from the Reissner-Nordstr\"om modes arise. In particular, isospectrality is strongly broken, both for the electromagnetic-led and the gravitational-led modes, for large values of the charge.