Advection Dominated Accretion Flows Around Kerr Black Holes
M. A. Abramowicz, X. -M. Chen, M. Granath, J. -P. Lasota
Abstract
We derive all relevant equations needed for constructing a global general relativistic model of advectively cooled, very hot, optically thin accretion disks around black holes and present solutions which describe advection dominated flows in the gravitational field of a Kerr black hole.
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