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Efficiency of Magnetized Thin Accretion Disks in the Kerr Metric

Published 1999 July 23 © 1999. The American Astronomical Society. All rights reserved. Printed in U.S.A.
, , Citation Charles F. Gammie 1999 ApJ 522 L57 DOI 10.1086/312207

1538-4357/522/1/L57

Abstract

The efficiency of thin disk accretion onto black holes depends on the inner boundary condition, specifically the torque applied to the disk at the last stable orbit. This is usually assumed to vanish. I estimate the torque on a magnetized disk using a steady magnetohydrodynamic inflow model originally developed by Takahashi et al. I find that the efficiency epsilon can depart significantly from the classical thin disk value. In some cases epsilon > 1, i.e., energy is extracted from the black hole.

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10.1086/312207