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The long-term evolution of a black hole accretion torus: a comparison between GRMHD simulations and relativistic thin disk theory
In this paper we analyse the long-term evolution of a black hole accretion torus using novel GRMHD simulations which, for the first time, have been run out to extremely large evolutionary times $t_{\rm max} = 10^7 GM_\bullet/c^3$. This allows for detailed comparisons between the gross evolution of t
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