Perturbations and quasi-normal modes of black holes with time-dependent scalar hair in shift-symmetric scalar-tensor theories

TL;DR

This paper derives a generalized Regge-Wheeler equation for odd parity perturbations of black holes with time-dependent scalar hair in shift-symmetric scalar-tensor theories, analyzing stability and computing quasi-normal modes.

Contribution

It provides a general framework for analyzing odd parity perturbations without degeneracy assumptions, extending stability analysis and quasi-normal mode calculations in scalar-tensor theories.

Findings

Derived a second-order master equation for perturbations.

Identified stability conditions for black holes with scalar hair.

Computed quasi-normal modes for a specific black hole solution.

Abstract

We study odd parity perturbations of spherically symmetric black holes with time-dependent scalar hair in shift-symmetric higher-order scalar-tensor theories. The analysis is performed in a general way without assuming the degeneracy conditions. Nevertheless, we end up with second-order equations for a single master variable, similarly to cosmological tensor modes. We thus identify the general form of the quadratic Lagrangian for the odd parity perturbations, leading to a generalization of the Regge-Wheeler equation. We also investigate the structure of the effective metric for the master variable and refine the stability conditions. As an application of our generalized Regge-Wheeler equation, we compute the quasi-normal modes of a certain nontrivial black hole solution. Finally, our result is extended to include the matter energy-momentum tensor as a source term.