Table 1.
Summary of the simulations.
| Lx | 2h | np | Ep | Jp/e | B(RA) | Np sim | γ | Lν |
|---|---|---|---|---|---|---|---|---|
| erg s−1 | cm | cm−3 | TeV | s−1 | G | GeV/s | ||
| 5 × 1036 | 6.3 × 106 | 2.4 × 1019 | 0.11 | 3.0 × 1033 | 1.8 × 103 | 106 | −7.8 ± 0.3 | (4.2 ± 0.2)×1031 |
| 1037 | 5.6 × 106 | 5.1 × 1019 | 0.22 | 4.4 × 1033 | 3.3 × 103 | 105 | −5.3 ± 0.1 | (1.6 ± 0.04)×1033 |
| 5 × 1037 | 3.0 × 106 | 4.0 × 1020 | 1.12 | 1.1 × 1034 | 1.3 × 104 | 104 | −3.41 ± 0.05 | (8.0 ± 0.2)×1034 |
| 1038 | 2.8 × 106 | 7.3 × 1020 | 2.24 | 1.6 × 1034 | 2.3 × 104 | 104 | −3.13 ± 0.04 | (1.96 ± 0.04)×1035 |
| 1039 | 4.5 × 106 | 5 × 1021 | 22.4 | 6.1 × 1034 | 1.6 × 105 | 104 | −2.94 ± 0.08 | (1.51 ± 0.08)×1036 |
| 5 × 1039 | 2.1 × 107 | 5 × 1021 | 100.0 | 1.5 × 1035 | 6.7 × 105 | 104 | −2.88 ± 0.04 | (1.15 ± 0.04)×1037 |
Notes. Input parameters: X-ray luminosity (Lx ), accretion disc thickness (2h), proton density in the disc (np), energy of the protons of the beam (Ep), flux of protons of the beam (Jp/e), magnetic field at RA (B(RA)) assuming B0 = 5 × 1012 G, number of protons of the beam simulated (Np sim). Output parameters: Value of the slope of the power-law from the best fit of the simulated spectra (γ, where the power-law function is N = KEγ), neutrino luminosity above 50 GeV from the simulated spectra (Lν).
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