This shows you the differences between two versions of the page.
Both sides previous revision Previous revision | Last revision Both sides next revision | ||
2017:groups:higgs:fxsnp [2017/06/26 19:06] sabine.kraml |
2017:groups:higgs:fxsnp [2017/06/26 19:16] sabine.kraml |
||
---|---|---|---|
Line 9: | Line 9: | ||
If new operators and/or new Higgs production modes are present, this can change the kinematic distributions and thus the signal acceptance. This can be tested with fiducial cross sections, [[https://phystev.cnrs.fr/wiki/2017:groups:higgs:stxs | STXS]], differential distributions. However, appropriate tools and explicit studies using the available measurements are still missing. | If new operators and/or new Higgs production modes are present, this can change the kinematic distributions and thus the signal acceptance. This can be tested with fiducial cross sections, [[https://phystev.cnrs.fr/wiki/2017:groups:higgs:stxs | STXS]], differential distributions. However, appropriate tools and explicit studies using the available measurements are still missing. | ||
- | Rivet routines are available for the ATLAS diphoton (and 4l ?) measurements at 8 TeV. These could be used to constrain additional Higgs production from e.g. | + | Rivet routines are available for the ATLAS diphoton and 4l measurements at 8 TeV. These could be used to constrain additional Higgs production from e.g. |
* A -> Zh | * A -> Zh | ||
* VLQ decays to Higgs | * VLQ decays to Higgs |