Fermionic and Bosonic Greybody Factors as well as Quasinormal Modes for Charged Taub NUT Black Holes

TL;DR

This paper investigates the greybody factors and quasinormal modes of charged Taub NUT black holes for both fermionic and bosonic fields, revealing how the NUT parameter influences these phenomena.

Contribution

It provides a detailed analysis of fermionic and bosonic wave equations, deriving effective potentials and studying the impact of the NUT parameter on greybody factors and quasinormal modes.

Findings

Fermionic QNMs and GFs increase with NUT parameter.

Bosonic GFs increase more rapidly than bosonic QNMs as NUT parameter increases.

The NUT parameter significantly affects the effective potentials for both fermions and bosons.

Abstract

The paper studies the spinorial wave equations, namely the Dirac and the Klein Gordon equations, as well as the greybody radiations and quasinormal modes (QNMs) of the charged Taub NUT black hole (CTNBH). To obtain fermionic greybody factors (GFs) and QNMs, we study the charged fermions by employing the Dirac equation. To this end, we use a null tetrad in the Newman-Penrose formalism. Then, we separate the Dirac equation into radial and angular sets. Using the obtained radial equations, we convert them into the typical one dimensional Schr\"{o}dinger like wave equations with the aid of tortoise coordinate and derive the effective potentials. For bosonic GFs and QNMs, we study the Klein Gordon equation in the CTNBH geometry and obtain the radial equation. We then derive the effective potential and investigate the effect of NUT parameter on it. We show that while the fermionic QNMs and GFs individually increase with the increasing NUT parameter, the increase of bosonic GFs with increasing NUT parameter is overwhelmingly greater than that of the bosonic QNMs.