Quasinormal modes of rotating black holes in shift-symmetric Einstein-scalar-Gauss-Bonnet theory

TL;DR

This paper computes the full non-perturbative spectrum of quasinormal modes for rapidly rotating black holes in shift-symmetric Einstein-scalar-Gauss-Bonnet theory using a spectral method, comparing with perturbative and Einstein-dilaton-Gauss-Bonnet results.

Contribution

It introduces a spectral method to obtain non-perturbative quasinormal modes of rotating black holes in this theory, extending previous perturbative analyses.

Findings

Full non-perturbative quasinormal mode spectrum obtained.

Comparison with perturbative results shows good agreement within certain domains.

Differences observed with Einstein-dilaton-Gauss-Bonnet black holes.

Abstract

We employ a recently developed spectral method to obtain the spectrum of quasinormal modes of rapidly rotating black holes in alternative theories of gravity and apply it to the black holes of shift-symmetric Einstein-scalar-Gauss-Bonnet theory. In this theory the quasinormal modes were recently obtained by employing perturbation theory in quadratic order in the Gauss-Bonnet coupling constant. Here we present the full non-perturbative results for the spectrum within the domain of existence of rotating black holes and compare with the perturbative results. We also compare with the quasinormal mode spectrum of rapidly rotating Einstein-dilaton-Gauss-Bonnet black holes.