English (United Kingdom)

https://curated-unify.zendy.io/wp-json/zendy-region/v1/featured_content/oa?rat=en

https://curated-unify.zendy.io/wp-json/zendy-region/v1/highlighted_journal/

Global: Zendy Plus annual

Presents the access of premium content as premium feature

Premium Content

Presents the keyphrase highlighting as premium feature

Keyphrase Highlighting

Presents the summarisation as premium feature

Summarisation

Insights

Presents the pdf analysis as premium feature

PDF Analysis

Presents the zaia usage as premium feature

ZAIA

Global: Zendy Tools annual

Global: Zendy Free Plan

Global: Zendy Tools monthly

Global: Zendy Plus monthly

This paper examines the general relativistic model of a geometrically thickconfiguration of an accretion disc around an electrically charged black hole inan accelerated motion, as described by the C-metric family. We aim to study theeffects of the spacetime background on the magnetised version of the thick discmodel via the sequences of figures of equilibrium. While maintaining theassumption of non-selfgravitating (test) fluid, we newly explore the influenceof the strength of the large-scale magnetic field with field lines organisedover the length-scale of the black hole horizon. We systematically analyze thedependence on a very broad parameter space of the adopted scenario. Wedemonstrate that the C-metric can, in principle, be distinguished from Kerrblack hole metric by resolving specific (albeit rather fine) features of thetorus, such as the location of its centre, inner and outer rims, and theoverall shape. The analytical setup can serve as a testbed for numericalsimulations.

Magnetised relativistic accretion disc around a spinning, electrically charged, accelerating black hole: case of C-metric