Quasi-normal mode of dyonic hairy black hole and its interplay with phase transitions

TL;DR

This paper investigates the stability and quasinormal modes of dyonic hairy black holes, revealing their potential as probes for black hole phase transitions through detailed numerical analysis of scalar perturbations.

Contribution

It provides a comprehensive numerical study of QNMs in dyonic hairy black holes and explores their connection with black hole phase transitions, highlighting differences between small and large black hole phases.

Findings

QNMs indicate stability of the black holes against scalar perturbations.

QNM behavior varies between small and large black hole phases.

QNM properties can serve as probes for black hole phase transitions.

Abstract

We study the dynamical stability of hairy dyonic black holes in the Einstein-Maxwell-scalar gravity system against the massless scalar field perturbation. We numerically obtain the corresponding quasinormal modes (QNMs) using the series solution and shooting methods for various black hole parameters. We find that the numerical values obtained from these two methods agree well with each other. The imaginary part of the QNM is always negative, indicating the stability of the dyonic hairy black hole against the scalar perturbation. We find that the decay and oscillatory modes of the scalar field perturbation increase linearly with the horizon radius for large black holes. We thoroughly investigate the behaviour of QNMs for different values of black hole parameters, including the electric charge, magnetic charge, horizon radius and hairy parameter, etc. Moreover, we also analyse the QNM near the small/large black hole phase transition and find that the nature of the QNMs is different for large and small black hole phases, suggesting QNMs as the possible probe of black hole phase transition.