2021
DOI: 10.1063/5.0048929
|View full text |Cite
|
Sign up to set email alerts
|

Stealth black hole perturbations in kinetic gravity braiding

Abstract: We study stealth black hole perturbations in shift symmetric kinetic gravity braiding and obtain its analogous Regge–Wheeler and Zerilli master equations for the odd and even parity sectors. We show that the nontrivial hair of static and spherically symmetric stealth black holes contributes only an additional source term to the even parity master equation. Furthermore, we derive exact solutions to the monopolar and dipolar perturbations and show that they are generally pathological non-gauge modes or else redu… Show more

Help me understand this report
View preprint versions

Search citation statements

Order By: Relevance

Paper Sections

Select...
1

Citation Types

0
1
0

Year Published

2021
2021
2024
2024

Publication Types

Select...
4

Relationship

0
4

Authors

Journals

citations
Cited by 4 publications
(1 citation statement)
references
References 91 publications
0
1
0
Order By: Relevance
“…With this vast landscape of exact solutions, it becomes crucial to find methods to classify them and characterize their physical properties. To a large extent, most of the investigations have focused on perturbative analysis of black hole and cosmological stealth solutions, revealing crucial information on the quasinormal modes as well as the issues of the strong coupling [75][76][77][78][79][80][81][82][83][84][85]. However, some key information about these solutions can be revealed only by mean of non-perturbative methods, such as the nature of their principal null directions (PNDs), which in turn, is intimately related to the non-perturbative gravitational waves carried in the non-stationary regime.…”
Section: Introductionmentioning
confidence: 99%
“…With this vast landscape of exact solutions, it becomes crucial to find methods to classify them and characterize their physical properties. To a large extent, most of the investigations have focused on perturbative analysis of black hole and cosmological stealth solutions, revealing crucial information on the quasinormal modes as well as the issues of the strong coupling [75][76][77][78][79][80][81][82][83][84][85]. However, some key information about these solutions can be revealed only by mean of non-perturbative methods, such as the nature of their principal null directions (PNDs), which in turn, is intimately related to the non-perturbative gravitational waves carried in the non-stationary regime.…”
Section: Introductionmentioning
confidence: 99%