Table 3.
Summary of two representative models with the magnetic field inclined with respect to the rotation axis of the black hole.
| Model | Angle of | βmin | a | Final | ⟨ϕBH⟩t |
 |
 |
|---|---|---|---|---|---|---|---|
| inclination | Ṁin,H | (code units) | (M⊙ yr−1) | ||||
| incl45.bmin0003.a90 | 45° | 0.0003 | 0.90 | 1.53 | 36.09 | 2.18 × 10−4 | 7.69 × 10−7 |
| incl45.bmin0003.a99 | 45° | 0.0003 | 0.99 | 2.68 | 29.12 | 3.21 × 10−5 | 1.13 × 10−7 |
Notes. The models are parameterized by the initial minimum plasma β in the domain and the dimensionless Kerr parameter a. The time-averaged magnetic flux on the horizon and the mass outflow rate were computed from time 1500tg to 2000tg after the magnetic field was turned on. The final mass accretion rate is given at 2000tg after the magnetic field was turned on. The outflow rate in physical units was estimated by considering the central engine mass of M87, as for the earlier models.
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