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Table 1.

Summary of models with an aligned field.

Model ( † ) βmax a Final Ṁin,H ⟨ϕBH⟩t ⟨ M ˙ out , 10 r g ⟩ t $ \langle\dot M_{{\mathrm{out},10r_{g}}}\rangle_t $ ⟨ M ˙ out , 10 r g ⟩ t $ \langle\dot M_{{\mathrm{out},10r_{g}}}\rangle_t $
(code units) (code units) (M⊙ yr−1)
b1.a0.2D 1.0 0 4.91 43.08 3.00 × 10−5 1.060 × 10−7
b1.a60.2D 1.0 0.60 0.49 41.95 3.07 × 10−5 1.084 × 10−7
b1.a90.2D 1.0 0.90 0.62 35.06 4.82 × 10−5 1.703 × 10−7
b1.a99.2D 1.0 0.99 1.54 28.72 8.11 × 10−5 2.864 × 10−7
b05.a0.2D 0.5 0 2.70 45.73 2.36 × 10−5 8.325 × 10−8
b05.a60.2D 0.5 0.60 0.71 43.44 2.45 × 10−5 8.666 × 10−8
b05.a90.2D 0.5 0.90 1.08 35.57 3.99 × 10−5 1.410 × 10−7
b05.a99.2D 0.5 0.99 2.92 28.88 6.87 × 10−5 2.429 × 10−7
b01.a0.2D 0.1 0 2.77 46.78 2.16 × 10−5 7.645 × 10−8
b01.a60.2D 0.1 0.60 2.98 44.67 2.81 × 10−5 9.941 × 10−8
b01.a90.2D 0.1 0.90 4.61 35.68 4.29 × 10−5 1.515 × 10−7
b01.a99.2D 0.1 0.99 12.25 29.04 9.18 × 10−5 3.243 × 10−7
b01.a90.3D 0.1 0.90 3.18 43.36 8.50 × 10−5 3.003 × 10−7
b01.a99.3D 0.1 0.99 8.05 32.41 12.65 × 10−5 4.468 × 10−7

Notes. The models are parameterized by the initial maximum plasma β and the dimensionless Kerr parameter a. The time-averaged magnetic flux on the horizon and the equatorial mass outflow rate at 10rg were computed after the magnetic field was turned on. The outflow rate given in the last column is the estimated value in physical units considering our mass ejection model with the mass of the central engine of M87. The final accretion rate was taken at 2000tg after the magnetic field was turned on. ( † )The notation of the first column indicates the simulation run, the assumed spin value (0 ≤ a < 1), and the adopted 2D or 3D computation.

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