Upload
quynh
View
27
Download
0
Tags:
Embed Size (px)
DESCRIPTION
Photon(s) + MET Analyses. Bruce Schumm UC Santa Cruz / SCIPP 16 April 2013 ATLAS SUSY Workshop Amsterdam, NE. Motivation: GMSB and the Bino NLSP. GMSB breaks SUSY via intermediate-scale messenger interactions Naturally protects SM flavor symmetry LSP is gravitino. “Minimal” GMSB. - PowerPoint PPT Presentation
Citation preview
Photon(s) + MET Analyses
Bruce Schumm
UC Santa Cruz / SCIPP
16 April 2013
ATLAS SUSY Workshop
Amsterdam, NE
Motivation: GMSB and the Bino NLSP
• GMSB breaks SUSY via intermediate-scale messenger interactions
• Naturally protects SM flavor symmetry
• LSP is gravitino
• Over much of parameter space NLSP is short-lived Bino
• B(bino G) cos2W 78%
Diphoton + ETmiss signature
Photon + Njets + ETmiss signature
bino cos2W
“Minimal” GMSB
Prior Analysis: Diphoton + MET
A: Strong production, heavy binoB: Strong production, light binoC: Electroweak production
Strong production
EW production
For strong production, high total-energy cut gives~background-free analysis
8 TeV Analysis: Diphoton + MET
“SPS8” Trajectory
For 2012 (8 TeV) Data:
Replace “constrained” SPS8 grid with wino/bino grid
Bino = 10
Wino = degenerate triplet 1 and 2
0
Production through 1 2
0 and 1+ 1
-
Signal region optimization points
Low-mass, high-mass bino for Strong and EW production
Resulting signal regions
“Model-independent” selection MET cut for which QCD, EW background are about the same.
Issue for Photon(s) + MET Analyses: What MET?
• Significant changes for p1328 relative to p1181• Use gamma-gamma MC as proxy for signal (can look at high MET)
• EG10NoTauPhotonLoose designed for photon analyses; performs worse in p1328
• “Vanilla” MetRefFinal does well
Control samples for MetRefFinal
“g” is control photon (loose but not tight); can be isolated or not
“t” is isolated tight photon
“QCDtg” is nominal diphoton control sample
Good agreement w/ signal MET, especially QCDtg
Challenges: “Irreducible” W Background
• Sizeable for EW production and “model independent” selections• Constrain with data looking at (e,) events
Expected signal(MC)
50 < MET < 125
125 < MET < 250
125 < MET < 250
Expect: ~1.5
Observe: 0
Constrains K-factor (currently assumed to be 33)
CMS diphoton+MET with 4 fb-1 at 8 TeV
CMS diphoton analysis:
• Employs no “overall energy scale” observable (HT, Meff)
• Single analysis similar to ATLAS “MIS” signal region
• Look at strong production only
Single Photon + MET Analysis
Motivation: Diphoton analysis may not be sensitive if
• Neutralino is not NLSP (no photons; not for this session!)• Neutralino is the NLSP but is not purely bino
GMSB Neutralino NLSP Phenomenology
• Bino-like diphoton final state• Wino-like admixture photon + lepton• Higgsino-like admixture, <0 photon + bjets• Higgsino-like admixture, >0 photon + jets
Single Photon + MET analysis covers this final, missing signature
CMS single- analysis
• Photon ET > 80 GeV
• 2 jets with pT > 30 GeV
• HT > 450 GeV
• MET in bins, but sensitivity arises for MET > 250
• Set limit of mgluino > 1125 GeV for bino-like neutralino (4 fb-1 at 8 TeV)
Single-Photon + MET Signal Regions
• Minimize model dependence by minimizing Njet requirement
• RT2 is fraction of total visible energy in two leading jets
Photon + MET Challenges / Next Steps
Devising grid was significant development (tune gluino, neutralino BFs and lifetimes) but is now being submitted for generation.
Next steps: understand backgrounds challenges, e.g.
Conclusions and Outlook
For 8 TeV data, significant new model space has been introduced
• Weak production (decoupled strong partners) limits with diphoton analysis (bino-like neutralino)
• GMSB scenario with photon + jet signature
Plan is summary paper with all four photon(s) + MET analysis, covering full range of neutralino NLSP possibilities, plus electroweak production for bino- and wino-like NLSP
Distinction between pointing, non-pointing signatures is somewhat arbitrary and artificial Combine into unified analysis for 2015 data?