On the accreting tori sequences in Ringed Accretion Disks models. Polytropic equations of state and toroidal magnetic fields

Abstract

We consider ringed accretion disks (RADs), representing models of aggregates of corotating and counterrotating toroids orbiting a central Kerr super-massive black hole (SMBH). We comment on system of two-tori governed by the polytropic equation of state and including a toroidal magnetic field. We found the RADs leading function describing the RAD inner structure and governing the distribution of orbiting toroidal structures and the emergence of the (hydro-mechanical) instabilities in the disk. We perform this analysis first in pure hydrodynamical models by considering one-specie perfect fluid toroids and then by considering the contribution of toroidal magnetic field.

11 pages, 3 figures, RAGtime 20, 2018, Opava, Czech Republic

References in corpus (3)

• Papaloizou-Pringle instability suppression by the magnetorotational instability in relativistic accretion discs
• Relativistic thick accretion disks: morphology and evolutionary parameters
• Oblique magnetic fields and the role of frame dragging near rotating black hole