Table 3
Maximum allowed neutrino flux from nearby clusters at 250 TeV.
| Cluster | αp = 2 | αp = 2.2 | αp = 2.4 | |
|
|
||||
| Virgo | ≤ | 3.2 × 10-19 | 4.0 × 10-20 | 3.4 × 10-21 |
| Centaurus | ≤ | 7.3 × 10-21 | 9.1 × 10-22 | 7.7 × 10-23 |
| Perseus | ≤ | 1.8 × 10-20 | 2.3 × 10-21 | 1.9 × 10-22 |
| Coma | ≤ | 2.8 × 10-20 | 3.5 × 10-21 | 2.9 × 10-22 |
| Ophiuchus | ≤ | 4.5 × 10-20 | 5.6 × 10-21 | 4.7 × 10-22 |
|
|
||||
| Sum | ≤ | 4.2 × 10-19 | 5.2 × 10-20 | 4.4 × 10-21 |
Notes. Maximum allowed neutrino flux at 250 TeV in units of cm-2 s-1 GeV-1. Numbers were obtained assuming the phenomenological luminosity-mass relations of Sect. 3. All cases refer to B = 1μG; αp = 2 refers to 30% loud clusters, our most optimistic while still realistic case; and the cases of αp = 2.2 and 2.4 refer to 100% loud clusters (see Table 1).
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.