Quasinormal modes of dilaton-de Sitter black holes: scalar perturbations

TL;DR

This paper investigates the quasinormal modes of dilaton-de Sitter black holes under scalar perturbations, revealing unique resonance behaviors and providing exact frequency calculations through approximation methods.

Contribution

It introduces a detailed analysis of scalar perturbations in dilaton-de Sitter black holes, including the use of WKB and Pöschl-Teller potential approximations for frequency computation.

Findings

No quasi resonance modes for massive scalar fields in this black hole.

Exact quasinormal frequencies obtained via Pöschl-Teller potential approximation.

Parameter variations significantly affect quasinormal mode frequencies.

Abstract

Dilaton black hole solutions in low energy string theory (well known as GMGHS black holes) have analogue black holes with a cosmological constant derived by Gao and Zhang. Here, we study quasi normal modes of this dilaton-de Sitter black hole under neutral scalar field perturbations. We have employed the sixth order WKB analysis to compute the quasi normal mode frequencies. A detailed study is done for the quasi normal mode frequencies by varying the parameters in the theory such as the mass, cosmological constant, dilaton charge and the spherical harmonic index. For the massive scalar field we observed that the usual quasi resonance modes that exists for asymptotically flat black holes do not exist for this particular black hole. We have approximated the scalar field potential of the near-extreme dilaton de Sitter black hole with the P$\ddot{o}$schl-Teller potential and have presented exact quasi normal frequencies.