Fig. 10
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Breakdown of the different contributions to the DF correction term in Eq. (12) for simulations LR_B1e4_DF_ϵ∗, B1e5_DF_ϵ∗, B1e6_DF_ϵ∗, and B1e7_DF_ϵ∗. From top to bottom: BH distance to the halo centre, ratio of DF acceleration to gravitational acceleration, ratio of stellar to DM contributions to DF, total number of particles within ϵBH, Coulomb logarithm term, and inverse velocity term of Eq. (34).
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