Massive scalar perturbations on Myers-Perry–de Sitter black holes with a single rotation

Supakchai Ponglertsakul, Bogeun Gwak

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18 Scopus citations

Abstract

This study investigates the stability of higher-dimensional singly rotating Myers-Perry–de Sitter (MP–dS) black holes against scalar field perturbations. The phase spaces of MP-dS black holes with one spin parameter are discussed. Additionally, the quasinormal modes (QNMs) of MP-dS black holes are calculated via the asymptotic iteration method and sixth-order Wentzel–Kramers–Brillouin approximation. For near-extremal MP-dS black holes, the event horizon may be considerably close to the cosmological horizon. In such cases, the Pöschl–Teller technique yields an accurate analytic formula for the QNMs. It is found that when the spin parameter of a black hole increases, the scalar perturbation modes oscillate at higher frequencies and decay faster. Furthermore, the MP-dS black hole with a single rotation is found to be stable under perturbation.

Original languageEnglish
Article number1023
JournalEuropean Physical Journal C
Volume80
Issue number11
DOIs
StatePublished - 1 Nov 2020

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