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Top physics during ATLAS commissioning. Ivo van Vulpen Wouter Verkerke. Structure of the talk: Reminder you of the goals of the study and main results presented in Rome Overview new results since Rome. - PowerPoint PPT Presentation
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Top physics during ATLAS commissioning
Ivo van VulpenWouter Verkerke
Structure of the talk:
Reminder you of the goals of the study and main results presented in Rome Overview new results since Rome
Ivo van Vulpen (NIKHEF) ATLAS physics week (October 2005) Slide 3
Goals for top physics during comissioning:
1) Can we see the top peak in the LHC commissioning run ? With 300 pb-1 Without b-tagging
2) Can we help commission the ATLAS detector using these events ? Calibrate light jet energy scale Calibrate missing ET
Obtain enriched b-jet sample Cross section
1 lepton PT > 20 GeV
Missing ET > 20 GeV
4 jets(R=0.4) PT > 40 GeV
Selection efficiency = ~5 %
TOP quark CANDIDATE
W bosonCANDIDATE
Simple (standard) top quark selection:
Ivo van Vulpen (NIKHEF) ATLAS physics week (October 2005) Slide 4
Main results shown in Rome:
3-jet mass distributions m(jjj), with and without cut on Mw
Hadronic 3-jet mass
m(Whad)L=300 pb-1
(~1 week of running)
Cut on Mw
Hadronic 3-jet mass
Mjjj (GeV) Mjjj (GeV)
Ivo van Vulpen (NIKHEF) ATLAS physics week (October 2005) Slide 5
What’s new since Rome
Ivo van Vulpen (NIKHEF) ATLAS physics week (October 2005) Slide 6
What’s new since Rome: focus on concerns
1) Trigger Effect of electron trigger: 2e15i+e25i+e60
2) New background estimate from W+jets Addressing concern about phase space coverage A7 sample (W+jets) used for Rome analysis New estimate using Alpgen+MLM matching
3) 100 pb-1
More realistic estimate for integrated luminosity during LHC commissioning run
Ivo van Vulpen (NIKHEF) ATLAS physics week (October 2005) Slide 7
Trigger Performance
“How much ‘good’ electron events do we lose by including the trigger ?”
Ivo van Vulpen (NIKHEF) ATLAS physics week (October 2005) Slide 8
Impact various selection criteria on ttbar selection efficiency
Electron trigger important for event selection and cross section measurementNeed to understand differences between ttbar and clean Ze+e- or Weν events
• Jets: 4 reconstructed jets with Pt > 40 GeV 13.4% Losses mainly due to hard analysis cut on jet kinematics • Electrons At least 1 reconstructed electron wth Pt> 20 GeV 62.0% Losses mainly due to reconstruction
• Missing Et > 20 GeV 91.8 %
Fraction of events passing cuts
Ivo van Vulpen (NIKHEF) ATLAS physics week (October 2005) Slide 9
Scope of trigger plots
Data Reconstruction AnalysisTrigger
step 1: Require reconstructed good e- (with/without Pt cut)
step 2: Require e- to point back to MC truth e- from W decay
step 3: Look at trigger decision
Investigate trigger performance:
“How much ‘good’ electron events do we lose by including the trigger ?”
Ivo van Vulpen (NIKHEF) ATLAS physics week (October 2005) Slide 10
Trigger efficiency versus Pt (no pt-cut)
83.9 %
MC truth electron Pt (GeV)
Remaining questions: What object triggered the events with low-Pt e-‘s ? Why do we lose electrons Pt = 100 GeV in barrel ?
e- (Rec+match)e- (Rec+match + Trigger)
Note: Events with a reconstructed electron (no Pt-cut) that matches the electron from the W decay (Monte-Carlo truth)
Same as white, but have ‘yes’ trigger decision
MC truth electron Pt (GeV)
Ivo van Vulpen (NIKHEF) ATLAS physics week (October 2005) Slide 11
Trigger efficiency versus Eta (Pt > 20 GeV)
MC truth electron Eta
e- (Rec+match) e- (Rec+match + Trigger)
MC truth electron Eta
Note: Events with a reconstructed electron (Pt>20 GeV) that matches the electron from the W decay (Monte-Carlo truth)
Same as white, but have ‘yes’ trigger decision
Ivo van Vulpen (NIKHEF) ATLAS physics week (October 2005) Slide 12
Background estimate from W+jets
“Do you cover the full phase space contributing to 4 reconstructed jets?”
Ivo van Vulpen (NIKHEF) ATLAS physics week (October 2005) Slide 13
Cross section presented on wiki was wrong by factor ~2 Background goes down!
• ‘Good’ news: A7 cross section wrong on wiki:
What did we have in Rome: the A7 sample
• What is the A7 sample
W l
A7 = ‘Alpgen+ 4 jets’:
= W+4-partons L.O. Matrix Element + (Herwig) parton shower
Do we cover the full phase space that contributes to 4 reconstructed jets. Probably not. What about W+1/2/3-partons + hard gluon(s) from PS ?
• Possible concern about the A7 sample
Wlν
Ivo van Vulpen (NIKHEF) ATLAS physics week (October 2005) Slide 14
Towards modeling the full phase space
• ‘Traditional’ approach : W+0jets Matrix Elements(ME) + Parton Shower (PS):
– Would covers full phase space, but …
– Extremely inefficient for high-Pt jet sample
– Parton shower does not correctly describe hard gluon emission• remember: we require 4 jets with Pt > 40 GeV
• Idea for improvement:– Use parton shower for low-Pt radiation
– Use matrix element for high-Pt radiation
• Practical translation: – Generate separate samples of W + 0,1,2,3,4,5 ME partons
– add arton shower to each sample
– Cannot simply add samples because of double counting from hard parton showers
– Solution: Alpgen + MLM matching (M. Mangano)In a nutshell: kill events with too high PT-gluons in PS
– After matching can add W + n ME partons samples
Matrix ElementParton shower
0 PT-cut 40 100 GeV
40
Ivo van Vulpen (NIKHEF) ATLAS physics week (October 2005) Slide 15
Does MLM matching work ?
• Look at PT distribution of W-boson at Tevatron
– Region of high W-boson transverse momentum described by matrix element computation
– Sum of MLM-matched W + n ME parton samples describes CDF data well
W+1jetsW+0jets
W+2/3/4jets
(Plot taken from presentation by M. Mangano)
W
PT W-boson = net PT radiation
Ivo van Vulpen (NIKHEF) ATLAS physics week (October 2005) Slide 16
Applying MLM to estimate W + 4 reco jet background
• Generate samples of W + n ME partons + PS sample (n=0,1,2,3,4,5)
• Look at contribution of each sample to W + 4 reco jets final state
Sample (# of ME partons)
#R
eco jets
Sample (# of ME partons)
#Even
ts
• # Alpgen ME partons versus # reconstructed jets
• Constribution of ME parton samples in selected events (4 reconstr. jets)
Ivo van Vulpen (NIKHEF) ATLAS physics week (October 2005) Slide 17
Applying MLM to estimate W + 4 reco jet background
• Generate samples of W + n ME partons + PS sample (n=0,1,2,3,4,5)
• Look at contribution of each sample to W + 4 reco jets final state
Sample (# of ME partons)
#R
eco jets
Sample (# of ME partons)
#Even
ts
• # Alpgen ME partons versus # reconstructed jets
• Constribution of parton samples in ttbar sample (4 reconstr. jets)
Background dominated by W + 4 ME parton sample
But other samples also contribute due to small differences in jet definition in MLM matching and reconstruction, effects of
detector simulation etc…
Does not affect validity of procedure but strong mismatch will increase number of significantly contributing samples
Ivo van Vulpen (NIKHEF) ATLAS physics week (October 2005) Slide 18
Result: W + 4 reco jet background from MLM matching
• Bottom line for W + 4 jets background in 3-jet invariant mass m(jjj)Add all W + n ME partons samples and normalize sum to 127 pb-1
(luminosity of A7 sample)
• Including full phase space adds ~10% background w.r.t A7 samples
A7 estimate (127 pb-1) MLM estimate (127 pb-1) A7 & MLM (unit norm)
Amount of background increases by ~10% Shape consistent
W + 0 ME part.W + 1 ME part. W + 2 ME part. W + 3 ME part. W + 4 ME part. W ≥ 5 ME part.
Ivo van Vulpen (NIKHEF) ATLAS physics week (October 2005) Slide 19
More plots on W+ n ME MLM shape vs A7
MLM: PT of W-boson
PT of leading jet
A7 estimate (127 pb-1) MLM estimate (127 pb-1) A7 & MLM (unit norm)
pT, distributions of all jets and the electron consistent between A7 and MLM
W + 0 ME part.W + 1 ME part. W + 2 ME part. W + 3 ME part. W + 4 ME part. W ≥ 5 ME part.
Ivo van Vulpen (NIKHEF) ATLAS physics week (October 2005) Slide 20
Summary on W+jets background
• Evaluated background on full phase space by including W + 0,1,2,3,4,5 ME partons + PS using MLM technique
- Background level increases by ~10% w.r.t. A7 sample
- M(jjj), pT(jet), η(jet), pT(e-), η(e-) shapes all consistent between A7 and MLM sample
• To do: study effect of varying MLM matching parameters
– Can e.g. vary PT threshold between PS and ME
– Check that result is not strongly dependent on choice of matching parameters
• Include Wν decays in study (need to be generated)
Ivo van Vulpen (NIKHEF) ATLAS physics week (October 2005) Slide 21
Results for 100 pb-1
“What are the results of the study when using a more conservative estimate for the luminosity collected during the commissioning run ?“
Ivo van Vulpen (NIKHEF) ATLAS physics week (October 2005) Slide 22
Results for 100 pb-1 (no cut on reconstructed W mass)
Note 1: Background ~factor 2 lower due to initial mistake in A7 lumi
Note 2: Error bars now reflect statistical error of 100 pb-1 instead of statistical error of MC sample as was done for Rome plots.
Mjjj mass (GeV) Mjjj mass (GeV)
100 pb-1200 pb-1
Hadronic 3-jet mass
Mjjj (GeV) Mjjj (GeV)
electron-only
L =100 pb-1
electron+muon estimate for L=100 pb-1
L=200 pb-1
Hadronic 3-jet mass
Even
ts /
4.1
5 G
eV
Even
ts /
4.1
5 G
eV
Ivo van Vulpen (NIKHEF) ATLAS physics week (October 2005) Slide 23
Results for 100 pb-1 (with cut on reconstructed W mass)
Distribution of 3-jet invariant mass after a cut on the mass of the reconstructed W-boson: 70 < Mjj < 90 GeV
Mjjj (GeV) Mjjj (GeV)
electron-only
L =100 pb-1
electron+muon estimate for L=100 pb-1
L=200 pb-1
Hadronic 3-jet mass
Even
ts /
4.1
5 G
eV
Even
ts /
4.1
5 G
eV Hadronic 3-jet mass
Ivo van Vulpen (NIKHEF) ATLAS physics week (October 2005) Slide 24
Relax cut on minimum PT requirement for jets
“Top peak close to rising edge of background distribution when using a minimum jet PT-cut at Pt = 40 GeV. “
Ivo van Vulpen (NIKHEF) ATLAS physics week (October 2005) Slide 25
Relaxed cut on minimum PT requirement for jets
• Top peak on rising edge background distribution: Try relaxing cut on minimum jet-PT
In Note: investigate stability and effects from changed selection criteria
Mjjj (GeV) Mjjj (GeV)
electron-only
L =100 pb-1
electron-only
L=100 pb-1
Hadronic 3-jet mass
Even
ts /
4.1
5 G
eV
Even
ts /
4.1
5 G
eV Hadronic 3-jet mass
Minimum Jet PT = 40 GeV Minimum Jet PT = 30 GeV
Ivo van Vulpen (NIKHEF) ATLAS physics week (October 2005) Slide 26
Summary
• Focused on concerns after Rome– New estimate for W+jets background
• Lower estimate due to mistake in A7 lumi
• New procedure Alpgen+MLM matching 10% higher than corrected A7 result
– First results on impact electron trigger
– Preliminary results now quoted for 100 pb-1
• Plan– Finalize Alpgen+MLM matching study
– Evaluate some outstanding issues (b-tag, calibrations, etc.)
– Write note
Ivo van Vulpen (NIKHEF) ATLAS physics week (October 2005) Slide 27
Backup slidesBackup slides
Ivo van Vulpen (NIKHEF) ATLAS physics week (October 2005) Slide 28
Impact various selection criteria on ttbar selection efficiency
ttbar events passing all cuts
100 %
Pt of 4th jet (GeV)
Pt electron (GeV)
Jet Pt-cut
Electron Pt-cut
Main loss due to kinem. cuts (also # jets)
Main loss dueto reconstruc.
Nu
mb
er
of
even
ts
Selection criterium
Electron (62.0%)
Et-miss (91.8%)
Jets (13.4%)
Electron trigger important for event selection and cross section measurementNeed to understand differences between ttbar
and clean Ze+e- or Weν events
Nu
mb
er
of
jets
Nu
mb
er
of
even
ts