| 6 | | * K. Mawatari |
| 7 | | * C. Zhang |
| | 11 | === Description of the model === |
| | 12 | |
| | 13 | This is simplified dark matter models. |
| | 14 | Our effective lagrangian consists of different types of DM: |
| | 15 | |
| | 16 | * Xr (real scalar DM) |
| | 17 | * Xc (complex scalar DM) |
| | 18 | * Xd (Dirac spinor DM) |
| | 19 | * Xm (Majorana spinor DM) (to be done.) |
| | 20 | * ... |
| | 21 | |
| | 22 | and different types of mediators: |
| | 23 | |
| | 24 | * s-channel |
| | 25 | * Y0 (spin-0) |
| | 26 | * Y1 (spin-1) |
| | 27 | * Y2 (spin-2) (to be done.) |
| | 28 | * ... |
| | 29 | |
| | 30 | * t-channel (to be done.) |
| | 31 | |
| | 32 | |
| | 33 | === Model files === |
| | 34 | |
| | 35 | * : the s-channel model files in UFO format |
| | 36 | |
| | 37 | |
| | 38 | === Version updates === |
| | 39 | |
| | 40 | *2015.06.11 - v0.1_alpha: alpha version. |