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Trapping of magnetic flux by the plunge region of a black hole accretion disk

Christopher S. Reynolds·David Garofalo·Mitchell C. Begelman
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Abstract

The existence of the radius of marginal stability means that accretion flows around black holes invariably undergo a transition from a MHD turbulent disk-like flow to an inward plunging flow. We argue that the plunging inflow can greatly enhance the trapping of large scale magnetic field on the black hole, and therefore may increase the importance of the Blandford-Znajek (BZ) effect relative to previous estimates that ignore the plunge region. We support this hypothesis by constructing and analyzing a toy-model of the dragging and trapping of a large scale field by a black hole disk, revealing a strong dependence of this effect on the effective magnetic Prandtl number of the MHD turbulent disk. Furthermore, we show that the enhancement of the BZ effect depends on the geometric thickness of the accretion disk. This may be, at least in part, the physical underpinnings of the empirical relation between the inferred geometric thickness of a black hole disk and the presence of a radio jet.

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Christopher S. Reynolds, David Garofalo, Mitchell C. Begelman. 2006-07-17. Trapping of magnetic flux by the plunge region of a black hole accretion disk. https://doi.org/10.1086/507691

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