Les Houches
2023 Session
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- Use of wiki pages and slack. Wifi access/set-up.
- Important info about bus, lodging, facilities.
- Bulletins.
Wikis of Previous sessions
Les Houches Themes
(Lyrics and Music)
(Lyrics and Music)
People: Priscilla Pani, Giacomo Polesello, Amit Chakraborty, Björn Herrmann, Benjamin Fuks, Mihoko Nojiri, Abishek Iyer, Ramona Gröber
Email: priscilla.pani@cern.ch, giacomo.polesello@cern.ch, herrmann@lapth.cnrs.fr, amit@post.kek.jp, fuks@lpthe.jussieu.fr, nojiri@post.kek.jp, abhishek@theory.tifr.res.in, ramona.groeber@durham.ac.uk
pp → t j ETmiss
We start by investigating a simplified model setup as follows. We complement the SM by a right-handed scharm (scR) and stop (stR).
In the gauge eigenbasis, the two-squark system is parametrized with the three parameters:
After diagonalisation, in the mass eigenbasis, the three physical parameters are:
such that sq1 = ct*scR + st*St (and the corresponding relation for the second squark state sq2).
In addition, we add to the model a gluino (go), with the appropriate SUSY mixings (so that it will contribute to the various production process) and a bino (chi) that will allow both squarks to decay. The corresponding mass parameters are
The FeynRules model file is available here, and the corresponding UFO there. Do not forget, in madgraph, to load the model as
import model stop-scharm_UFO -modelname
and that the neutralino is called chi (and not n1).
1. Compute diagonal production cross-sections (at LO): function of mSq1 and mSq2, but independent of thSq.
2. Compute non-diagonal production cross-sections (at LO): function of mSq1, mSq2, and thSq. Evaluate, e.g., for thSq=(0, pi/4, pi/2) and mGl=3 TeV, and check importance w.r.t. diagonal production.
3. Compute branching ratios of Sq1 and Sq2 into t+N1 and into c+N1: function of mSq1, mSq2, thSq, mN1.
4. From the above, deduce cross-sections pp → t t ETmiss
, pp → c c ETmiss
, pp → t c ETmiss
: functions of mSq1, mSq2, thSq, mN1. Make sure to seperate contributions from different subchannels, since this information is necessary to determine the experimental acceptance!
5. Compute the above signal cross-sections in the full model (i.e. with 4×4 mixing) and use the obtained acceptances to deduce the limits. For this, we will use analytical formulas tu compute the BR. NLO+NLL cross sections for the signal.
6. At the end, try a different bino mass (50 GeV as default, and let's increase it). Try also to include BR of the squarks into something else (that is not populating the signal regions). Finally, maybe get the gluino mass dependence.
This set of macro was created to automatically rescale the scharm and stop analyses in the reference (8TeV 20ifb results) for any assumptions of mixing and U-masses. Download the full directory: nmfvstop.tgz
Execution Command (to be run in the working directory - run python rescaleExclusion.py –help for parameters explanation )
python rescaleExclusion.py –u1max 1000 –u1min 400 –step 100 –lumi 20 –alphalist 4,8 –Mchi 50
(NOTE before each parameter you need two dashes, I cannot make it appear in the twiki )