Quasinormal modes of self-dual black holes in loop quantum gravity

TL;DR

This paper investigates how loop quantum gravity corrections influence the quasinormal modes of regular black holes, revealing stability and deviations from classical Schwarzschild black holes through various computational methods.

Contribution

The study introduces a detailed analysis of quasinormal modes for loop quantum black holes with two correction parameters, using multiple numerical techniques.

Findings

LQG parameters affect quasinormal frequencies oppositely

LQBHs are dynamically stable

Deviations from Schwarzschild black holes are observed

Abstract

We study the evolution of a test scalar field on the background geometry of a regular loop quantum black hole (LQBH) characterized by two loop quantum gravity (LQG) correction parameters, namely, the polymeric function and the minimum area gap. The calculations of quasinormal frequencies in asymptotically flat spacetime are performed with the help of higher-order WKB expansion and related Pad\'{e} approximants, the improved asymptotic iteration method (AIM), and time-domain integration. The effects of free parameters of the theory on the quasinormal modes are studied and deviations from those of the Schwarzschild BHs are investigated. We show that the LQG correction parameters have opposite effects on the quasinormal frequencies and the LQBHs are dynamically stable.