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SIGNATURES OF BLACK HOLE SPIN IN GALAXY EVOLUTION

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D. Garofalo

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We explore the connection between black hole spin and active galactic nucleus (AGN) power by addressing the consequences underlying the assumption in the recent literature that the gap region between accretion disks and black holes is fundamental in producing strong, spin-dependent, horizon-threading magnetic fields. Under the additional assumption that jets and outflows in AGNs are produced by the Blandford-Znajek and Blandford-Payne mechanisms, we show that maximum jet/outflow power is achieved for accretion onto black holes having highly retrograde spin parameters, an energetically excited yet unstable gravitomagnetic configuration.


Keywords

black hole physics; galaxies: evolution


PACS

98.62.Js Galactic nuclei (including black holes), circumnuclear matter, and bulges

98.62.En Electric and magnetic fields

98.54.Cm Active and peculiar galaxies and related systems (including BL Lacertae objects, blazars, Seyfert galaxies, Markarian galaxies, and active galactic nuclei)

98.62.Nx Jets and bursts; galactic winds and fountains

98.62.Ai Origin, formation, evolution, age, and star formation

98.62.Mw Infall, accretion, and accretion disks

Subjects

Astrophysics and astroparticles

Dates

Issue 1 (2009 July 1)

Received 2009 May 4, accepted for publication 2009 May 28

Published 2009 June 15



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