Supercritical accretion disks with winds in General Relativity
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Abstract
We propose a new model to describe a super-Eddington accretion disk with outflows around black holes in general relativity. We focus on the vertical structure of the disk and analyze the conditions under which the fluid becomes transonic in the $z$-direction.
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Copyright owned by the author(s) under the term of the Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License.
Copyright owned by the author(s) under the term of the Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License.