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Fig. 1.

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Mass accretion rate at the black hole horizon for the initial part of the simulation before the magnetic field was introduced (β = ∞). The accretion rate initially grows and saturates to a quasi-steady value as time proceeds. It is given in geometric units, which can be scaled to physical units with the black hole mass M. The plot is given for only one spin value, but it is the same for all other values.

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