Fig. 11

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Summary of properties related to the most massive BH in the DFROGIN run, as they evolve across time. From top to bottom: z-component of the BH spin direction jBH,z (black, solid line) and direction of the angular momentum of the gas in the BH kernel jg,z (orange, dashed line); cosine of the angle between the accretion disc and the BH spin at the beginning of each accretion episode cos θBH–d (i.e. left-hand side of Eq. (6), black solid line) and − Jd/(2JBH) (i.e. right-hand side of Eq. (6), orange dashed line); ratio of the magnitudes of the disc and BH angular momenta Jd/JBH; BH dimensionless spin parameter α; radiative efficiency of the accretion disc єr; Eddington ratio fEdd; BH mass MBH.
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