Table 1.
Properties of the different TDE photon fields considered in this work for a cosmic-ray acceleration efficiency ηacc = 1.
| Lbol[Lpk] (erg s−1) | â | B′(G) | E′p,max(eV) |
|---|---|---|---|
| 3.5 × 1048 [1048] | 0.25 | 5.1 × 103 | 1.8 × 1018 |
| 6.8 × 1048 [1048] | 0.07 | 7.0 × 103 | 2.4 × 1018 |
| 1.0 × 1049 [1048] | 0.03 | 8.7 × 103 | 2.2 × 1018 |
| 6.8 × 1046 [1046] | 0.07 | 7.0 × 102 | 6.3 × 1018 |
| 6.8 × 1047 [1047] | 0.07 | 2.2 × 103 | 4.3 × 1018 |
| 6.8 × 1048 [1048] | 0.07 | 7.0 × 103 | 2.4 × 1018 |
Notes. All the photon fields are modeled by a log-parabola (Eq. (1)), with bolometric luminosity Lbol, peak luminosity Lpk, peak energy ɛpk, and width â.
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