Superradiance and Quasinormal Modes of Massive Scalar Fields around Kerr Black Holes in Einstein-Maxwell-Dilaton-Axion Theory with Perfect Fluid Dark Matter

TL;DR

This study explores how perfect fluid dark matter influences superradiance and quasinormal modes of massive scalar fields around Kerr black holes in Einstein-Maxwell-Dilaton-Axion theory, revealing contrasting effects of different parameters.

Contribution

It provides the first detailed analysis of the combined effects of PFDM and EMDA parameters on superradiance and QNMs in Kerr black holes.

Findings

Increasing dilaton parameter $r_2$ enhances superradiance and raises QNM frequencies.

Increasing PFDM parameter $mbda$ suppresses superradiance and lowers QNM frequencies.

The influence of $mbda$ dominates when both parameters vary simultaneously.

Abstract

We investigate the dynamics of massive scalar fields around Kerr black holes in the Einstein-Maxwell-Dilaton-Axion (EMDA) theory, incorporating the effects of perfect fluid dark matter (PFDM), characterized by the dilaton parameter $r_2$ and the PFDM parameter $\lambda$. These parameters modify both the ergosphere and the effective potential experienced by the scalar field. Using the asymptotic matching method, we compute superradiant amplification factors, while quasinormal mode (QNM) frequencies are obtained via the asymptotic iteration method (AIM). Our results reveal contrasting effects: increasing $r_2$ enhances superradiance and leads to higher QNM frequencies with greater damping, whereas increasing $\lambda$ suppresses superradiance and reduces QNM frequencies with weaker damping. In combined scenarios, the influence of $\lambda$ is found to be dominant. These findings extend the understanding of Kerr black holes in EMDA backgrounds and highlight the stabilizing role of PFDM in such systems.