Table 1.
Summary of simulations, including key results.
| Run | LAGN | min Min(< 0.5 kpc) | ΔMSMBH(1 Myr) |
|---|---|---|---|
| (erg s−1) | (M⊙) | (M⊙) | |
| Control | 0 | 1.5 × 108* | 1.2 × 108 |
| L0.1 | 1.26 × 1045 | 1.5 × 108* | 1.2 × 108 |
| L0.3 | 3.78 × 1045 | 1.4 × 108 | 4.0 × 107 |
| L0.5 | 6.30 × 1045 | 9.2 × 107 | 5.1 × 106 |
| L0.7 | 8.82 × 1045 | 2.8 × 107 | 1.6 × 106 |
| L1.0 | 1.26 × 1046 | 7.8 × 106 | 6.2 × 104 |
| L1.3 | 1.64 × 1046 | 4.1 × 106 | 5.9 × 103 |
| L1.5 | 1.89 × 1046 | 2.3 × 106 | 4.4 × 103 |
| L1.7 | 2.14 × 1046 | 1.3 × 106 | 6.1 × 103 |
| L1.9 | 2.39 × 1046 | 6.0 × 105 | 3.9 × 103 |
| L2.0 | 2.52 × 1046 | 3.1 × 105 | 4.8 × 103 |
| L2.2 | 2.77 × 1046 | 2.3 × 105 | 2.8 × 103 |
| L2.5 | 3.15 × 1046 | 8.1 × 104 | 5.7 × 103 |
Notes. The first column shows the simulation name in the form L#, where the number refers to AGN luminosity in terms of the Eddington luminosity LEdd = 1.26 × 1046 erg s−1. The second column shows the AGN luminosity. The subsequent columns show the main quantitative results: minimum value of cold rapidly infalling gas mass within the central 0.5 kpc and the SMBH particle mass change over 1 Myr. Each line corresponds to four simulations with stochastically different initial conditions, which we used to investigate the level of variance due to small-scale inhomogeneities. * marks models where the minimum is at the beginning of the simulation run (see the main text for details).
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