Table 3.
Injection parameters used in this work and selected work in the literature on nonthermal emission by CRs in the large-scale structure of the Universe.
| Reference | η(ℳs) | η(θB) | Kep |
 |
|---|---|---|---|---|
| This Work | Ryu et al. (2019) | Pais et al. (2018) | 0.01 | 1 |
| Hoeft et al. (2008) | Hoeft & Brüggen (2007) | – | 0.05 | Eq. (19) |
| Pinzke et al. (2013) | Pinzke et al. (2013) | – | Eq. (21) | Eq. (20) |
| Hong et al. (2014) | Kang & Ryu (2013) | – | – | 0.01 |
| Vazza et al. (2015b) | Kang & Ryu (2013) | 0.3 | 0.01 | Eq. (18) |
| Donnert et al. (2016) | Kang & Ryu (2013) | – | 0.01 | 0.1 |
| Wittor et al. (2017) | Kang & Ryu (2013) | Θ(θ − θcrit) | 0.05 | Eq. (19) |
| Ha et al. (2023) | Ha et al. (2023) | – | Eq. (21) | Eq. (20) |
Notes. From left to right, we list the indicated work, Mach number-dependent acceleration efficiency, magnetic field angle-dependent efficiency, injection ratio between electrons and protons, and injection momentum.
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