2019:groups:bsm:bdm
Differences
This shows you the differences between two versions of the page.
| Both sides previous revision Previous revision Next revision | Previous revision Last revision Both sides next revision | ||
|
2019:groups:bsm:bdm [2019/07/23 15:24] jose.zurita |
2019:groups:bsm:bdm [2019/07/23 15:58] jose.zurita |
||
|---|---|---|---|
| Line 17: | Line 17: | ||
| 2) Decide on a concrete model and delineate the cosmologically interesting parameter space (from conversion-driven freeze-out, freeze-in etc). Candidate model exists, with a sbottom-like parent decaying into a neutralino-like dark matter + a bottom quark. | 2) Decide on a concrete model and delineate the cosmologically interesting parameter space (from conversion-driven freeze-out, freeze-in etc). Candidate model exists, with a sbottom-like parent decaying into a neutralino-like dark matter + a bottom quark. | ||
| - | 3) Generate the signal [UFO model is here] | + | 3) Generate the signal [UFO model is here + FR file in] |
| https://phystev.cnrs.fr/wiki/_media/2019:groups:bsm:bdm:sbottom_ufo_model_fr.zip | https://phystev.cnrs.fr/wiki/_media/2019:groups:bsm:bdm:sbottom_ufo_model_fr.zip | ||
| + | |||
| + | (from Jan: "MG gives me an error on hypercharge violation, should be checked"). | ||
| 4) Investigate how to improve S/B (e.g. Br(B->l v)=10%, a third lepton veto, B is displaced in signal but not in background etc). | 4) Investigate how to improve S/B (e.g. Br(B->l v)=10%, a third lepton veto, B is displaced in signal but not in background etc). | ||
2019/groups/bsm/bdm.txt ยท Last modified: 2019/07/23 16:00 by jose.zurita
Page Tools
Except where otherwise noted, content on this wiki is licensed under the following license: Public Domain
