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STScI Preprint #1286
We critically assess the role of the Blandford-Znajek mechanism in the powering of outflows from accretion disk-fed black holes. We argue that there is no reason to suppose that the magnetic field threading the central spinning black hole differs significantly in strength from that threading the central regions of the disk. In this case, we show that the electromagnetic output from the inner disk regions is expected in general to dominate over that from the hole. Thus the spin (or not) of the hole is probably irrelevant to the expected electromagnetic power output from the system. We also point out that the strength of the poloidal field in the centre of a standard accretion disk has been generally overestimated, and discuss scenarios which might give rise to more significant central poloidal fields.
1) Space Telescope Science Institute, 3700 San Martin Drive
Baltimore, MD 21218
2) Institute of Astronomy, Madingley Road, Cambridge CB3 0HA, UK