Free Access
Table 2
Rescaling mass (Eqs. (12) and (13)) for the simulated MG theories listed in Table 1.
| Model | μ200 [h-1 M⊙] | |
|
|
||
| f(R) | Weak | 1.0 × 1013 |
| Medium | 1.0 × 1014 | |
| Strong | 3.0 × 1016 | |
|
|
||
| Symmetron | Weaker coupling | 4.5 × 1011 |
| Stronger coupling | 4.5 × 1011 | |
| Early SSB | 2.8 × 1012 | |
| Super-early SSB | 2.0 × 1013 | |
Notes. Halos with mass M200 ≫ μ200 are expected to be fully screened, while those with M200 ≃ μ200 will be partially screened.
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.