User Tools

Site Tools


2019:groups:bsm:bdm

Differences

This shows you the differences between two versions of the page.

Link to this comparison view

Both sides previous revision Previous revision
Next revision
Previous revision
2019:groups:bsm:bdm [2019/07/23 15:22]
jose.zurita
2019:groups:bsm:bdm [2019/07/23 16:00] (current)
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+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 
 + 
 +(from Jan: "MG gives me an error on hypercharge violation, should be checked"​). 
 +(from Benj: "The error is because mass and gague eigenstates are involved, and no hypercharge can be defined. Just ignore it").
  
 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.1563888169.txt.gz · Last modified: 2019/07/23 15:22 by jose.zurita