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Rapid Black Hole Spin-down by Thick Magnetically Arrested Disks

  • Authors: Beverly Lowell, Jonatan Jacquemin-Ide, Alexander Tchekhovskoy, Alex Duncan

Beverly Lowell et al 2024 The Astrophysical Journal 960 .

  • Provider: AAS Journals

Caption: Figure 6.

We plot k = ΩFH and its dependence on spin, which is crucial for converting jet power into angular momentum in our semi-analytic model. The red-dashed line shows the fit that we used to construct our semi-analytic model for a > 0. We did not find a strong dependence on spin for a < 0 and so used a constant value, k = 0.23, in our semi-analytic model for a < 0.

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