Magnetised relativistic accretion disc around a spinning charged accelerating black hole

This paper studied the relativistic accretion thick disc model in the background of a spinning charged accelerating black hole described by the C-metric family. We generalise the construction of the thick disc model to the spinning charged C-metric. This work aims to study the effects of this background on the thick magnetised disc model via studying the properties of these equilibrium sequences of magnetised, non-self-gravitating discs. In particular, we analyse the influence of the strength of the magnetic field in this space-time. We show the properties of this relativistic accretion disc model and its dependence on the initial parameters. In principle, this space-time could be distinguished from a Kerr space-time by observing the features of accretion disc in its vicinity. Besides, this theoretical model can serve as the initial data for numerical simulations.