| 2 | |
| 3 | === Author === |
| 4 | |
| 5 | * Benjamin Fuks, LPTHE / Sorbonne U. [ fuks @ lpthe.jussieu.fr ] |
| 6 | |
| 7 | === Description of the model & references === |
| 8 | |
| 9 | In contrast to the [https://feynrules.irmp.ucl.ac.be/wiki/MSSM leading order MSSM implementation in FeynRules], the NLO MSSM implementation does not allow for inter-generational sfermion mixing and CP-violation beyond the one included in the CKM matrix. The implementation relies on the superspace capabilities of !FeynRules (see [https://arxiv.org/abs/1102.4191 arXiv:1102.4191]) and follows the [https://arxiv.org/abs/hep-ph/0311123 SUSY Les Houches accord] (version 1). As there is some freedom in the way the model renormalisation in the on-shell scheme can be implemented, the user is free to implement his/her own by making use of a !FeynRules plugin called MoGRe. A few examples of usage can be found below and in [https://arxiv.org/abs/1907.XXXXX arXiv:1907.XXXXX]. |
| 10 | |
| 11 | === Model files === |
| 12 | |
| 13 | * [/attachment/wiki/MSSMatNLO/mssm-nlo.fr mssm-nlo.fr]: The model file. The current (and first public) version is v1.5. A restriction file with 5 flavours can be downloaded [/attachment/wiki/MSSMatNLO/Massless.rst here]. |
| 14 | * [/attachment/wiki/MSSMatNLO/MoGRe.m MoGRe.m]: The MoGRe plugin to !FeynRules. |
| 15 | * [/attachment/wiki/MSSMatNLO/use-MoGRe.nb use-MoGRe.nb]: An example of Mathematica® notebook loading the model and the parameters and using MoGRe for the renormalisation. |