On destabilising quasi-normal modes with a radially concentrated perturbation

Fuente: arXiv
Gespeichert in:
Bibliographische Detailangaben
1. Verfasser: Boyanov, Valentin
Format: Preprint
Veröffentlicht: 2024
Schlagworte:
Online-Zugang:
Tags: Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
_version_ 1866913638890078208
author Boyanov, Valentin
author_facet Boyanov, Valentin
contents In this work we explore some aspects of the spectral instability of back hole quasi-normal modes, using a specific model as an example. The model is that of a small bump perturbation to the effective potential of linear axial gravitational waves on a Schwarzschild background, and our focus is on three different aspects of the instability: identifying and distinguishing between the two different types of instabilities studied previously in the literature, quantifying the size of the perturbations applied to the system and testing the validity of the pseudospectral numerical method in providing a convergent result for this measure, and finally, relating the size and other features of the perturbation to the degree of destabilisation of the spectrum.
format Preprint
id arxiv_https___arxiv_org_abs_2410_11547
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle On destabilising quasi-normal modes with a radially concentrated perturbation
Boyanov, Valentin
General Relativity and Quantum Cosmology
High Energy Physics - Theory
In this work we explore some aspects of the spectral instability of back hole quasi-normal modes, using a specific model as an example. The model is that of a small bump perturbation to the effective potential of linear axial gravitational waves on a Schwarzschild background, and our focus is on three different aspects of the instability: identifying and distinguishing between the two different types of instabilities studied previously in the literature, quantifying the size of the perturbations applied to the system and testing the validity of the pseudospectral numerical method in providing a convergent result for this measure, and finally, relating the size and other features of the perturbation to the degree of destabilisation of the spectrum.
title On destabilising quasi-normal modes with a radially concentrated perturbation
topic General Relativity and Quantum Cosmology
High Energy Physics - Theory
url https://arxiv.org/abs/2410.11547