Magnetised accretion discs in Kerr spacetimes

TL;DR

This study investigates how external magnetic fields influence the thermal spectra and iron line profiles of accretion discs around Kerr black holes and naked singularities, providing tools to probe magnetic environments and the cosmic censorship conjecture.

Contribution

We developed a numerical scheme to compute magnetised accretion disc spectra and iron line profiles around Kerr objects, incorporating different magnetic field configurations and assessing observable effects.

Findings

Magnetic fields cause observable modifications in spectra and line profiles.

Naked singularities produce harder, brighter spectra than black holes.

Magnetic field effects vary with black hole spin and magnetic field configuration.

Abstract

We study the effect caused by external magnetic fields on the observed thermal spectra and iron line profiles of thin accretion discs formed around Kerr black holes and naked singularities. We aim to provide a tool that can be used to estimate the presence of magnetic fields in the neighbourhood of a compact object and to probe the cosmic censorship conjecture in these particular astrophysical environments. We developed a numerical scheme able to calculate thermal spectra of magnetised Page-Thorne accretion discs formed around rotating black holes and naked singularities as seen by an arbitrary distant observer. We incorporated two different magnetic field configurations: uniform and dipolar, using a perturbative scheme in the coupling constant between matter and magnetic field strength. Under the same assumptions, we obtained observed synthetic line profiles of the 6.4 keV fluorescent iron line. We show that an external magnetic field produces potentially observable modifications on the thermal energy spectrum and the fluorescent iron line profile. Thermal energy spectra of naked singularities are harder and brighter than those from black holes, and in addition, peak and cut-off energies are affected by the external magnetic field. Moreover, iron line profiles of slowly rotating black holes suffer more changes by a uniform magnetic field, while nearly extremal black holes and naked singularities are more altered in the dipolar case. Based on our calculations, we discard the possibility of modelling the archetypal black-hole candidate in Cygnus X-1 as a naked singularity. Comparison of our models with observational data can be used to probe the cosmic censorship conjecture and to estimate the existence and global geometry of magnetic fields around compact objects by fitting the thermal energy spectra and iron line profiles of X-ray binaries.