Fig. 8

Numerically obtained accretion rates of rest mass , energy
and angular momentum
averaged over the evolution time intervals [0, 1000 M] and [2000 M, 3000 M] as a functionof the initial MRI growth rate estimate Im(ωmax). We note that a lower negative value of
corresponds to a higher loss rate of the quantity from the torus and thus a higher accretion rate. The displayed values correspond to the parameter κ in the interval [−1, 1.31].
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