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Table 3
Constraints on magnetic fields in the hadronic model.
| Minimum magnetic field, B0,min [μG] : | ||||
| αB | α | |||
| 2.1 | 2.2 | 2.3 | 2.5 | |
|
|
||||
| 0.3 | 5.86 | 4.09 | 3.15 | 2.06 |
| 0.5 | 8.62 | 6.02 | 4.63 | 3.05 |
| 0.7 | 13.1 | 9.16 | 7.08 | 4.68 |
|
|
||||
| Corresponding XCR (100 kpc) [%] : | ||||
| 0.3 | 1.7 | 2.5 | 4.9 | 26.7 |
| 0.5 | 1.7 | 2.5 | 4.8 | 26.1 |
| 0.7 | 1.6 | 2.3 | 4.5 | 23.6 |
Notes. Constraints on magnetic fields in the hadronic model of the Perseus radio mini-halo and the corresponding CR-to-thermal pressure ratio (at the largest emission radius of 100 kpc) such that the model reproduces the observed radio surface brightness profile.
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