Torn accretion disks around Kerr black holes erode the inner shadow and produce bifurcated, crescent, and multi-order ring morphologies hard to obtain with standard equatorial disks.
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2 Pith papers cite this work. Polarity classification is still indexing.
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AGN disk capture and merger rates scale as (H/R)^{-8} and drop by 10-20 orders of magnitude in thick magnetically supported disks compared to thin thermal disks.
citing papers explorer
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Reshaping the inner shadow of a Kerr black hole by a torn accretion disk
Torn accretion disks around Kerr black holes erode the inner shadow and produce bifurcated, crescent, and multi-order ring morphologies hard to obtain with standard equatorial disks.
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Thick Disks, Thin Hopes: Suppressed Capture and Merger Rates in AGN
AGN disk capture and merger rates scale as (H/R)^{-8} and drop by 10-20 orders of magnitude in thick magnetically supported disks compared to thin thermal disks.