Table 2
Upper limits on ⟨ σv ⟩ eff/ ⟨ σv ⟩ 0 from the EGB.
| WIMP model | Upper limit on ⟨ σv ⟩ eff/ ⟨ σv ⟩ 0 | ||||
| Channel | mχ [GeV] | FHM | SHM | FHM | SHM |
|
|
|||||
|
500 | 1650 | 530 | 1875 | 605 |
| W+ W− | 500 | 2096 | 673 | 2381 | 769 |
| τ+ τ− | 500 | 3490 | 1121 | 3964 | 1279 |
| τ+ τ− | 150 | 378 | 121 | 429 | 139 |
|
|
|||||
| Mmin | 10-10 M⊙ | 10-6 M⊙ | |||
Notes. We assumed a subhalo mass fraction of fsh = 15% for a cut-off mass Mmin = 10-6 M⊙. Upper limits are listed for the cut-off masses bordering a 500 GeV neutralino scenario (see Bringmann 2009) and with respect to ψ = 180° and E = 40 GeV. See text and Appendix C for details.
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.