# Quasinormal modes of regular black holes with non   linear-Electrodynamical sources

**Authors:** Grigoris Panotopoulos, \'Angel Rinc\'on

arXiv: 1904.10847 · 2019-05-24

## TL;DR

This paper calculates the quasinormal mode spectrum of regular black holes influenced by Non-Linear Electrodynamics, analyzing stability and effects of charge, angular momentum, and overtone number using WKB approximation.

## Contribution

It provides the first detailed analysis of quasinormal modes for regular black holes with Non-Linear Electrodynamics, including an analytical eikonal limit expression.

## Key findings

- All modes are stable.
- Charge, angular momentum, and overtone number significantly affect the spectrum.
- Comparison with other charged black holes highlights unique spectral features.

## Abstract

We compute the spectrum of quasinormal frequencies of regular black holes obtained in the presence of Non-Linear Electrodynamics. In particular, we perturb the black hole with a minimally coupled massive scalar field, and we study the corresponding perturbations adopting the 6th order WKB approximation. We analyze in detail the impact on the spectrum of the charge of the black hole, the quantum number of angular momentum and the overtone number. All modes are found to be stable. Finally, a comparison with other charged black holes is made, and an analytical expression for the quasinormal spectrum in the eikonal limit is provided.

## Full text

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## Figures

12 figures with captions in the complete paper: https://tomesphere.com/paper/1904.10847/full.md

## References

88 references — full list in the complete paper: https://tomesphere.com/paper/1904.10847/full.md

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Source: https://tomesphere.com/paper/1904.10847