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Ratio of Three over Two Jet Cross Sections: Update 36 pb-1
P.Kokkas, I.Papadopoulos, C.FountasUniversity of Ioannina, Greece
QCD High pT Meeting 17 Dec 2010
2
MotivationD
0 PRL 86, p1955 (2001)
• Motivation: Measure the ratio R32
and compare with pQCD predictions with goals:• Extend the phase space of the measurement in a regime
that goes above the Tevatron.
• Measure S: Comparisons of the measured ratio at hadron level with the predictions of pQCD (parton level), after accounting for hadronisation corrections uncertainty, will measure the QCD coupling constant S at a scale never measured before.
jetTpTH vs
2n X; jetsn ppσ
3n X; jetsn ppσ
2σ3σ
32R
• First CMS result with 76nb-1 consistent with the predictions of PYTHIA 6 and MadGraph (PAS QCD-10-012)
• The measured ratio rises, due to phase space, with HT . Above HT≈0.7 TeV it reaches a plateau which is most sensitive to αs.
• Two sources of systematic uncertainties were considered:• Uncertainties due to absolute (10%) and eta-
dependent (2%xη) Jet Energy Scale lead to R32 uncertainties of 5%.
• Systematic uncertainty due to difference in shape between data and MC is 5%.
3
Data - Triggers
Eras Runs Lumi Data & JSON file & Relevant HLT_Jet TriggersEra_1 136035-141881 284.7nb-1 /JetMETTau/Run2010A-Nov4ReReco_v1/RECO
Cert_136033-149442_7TeV_Nov4ReReco_Collisions10_JSON.txtHLT_Jet30U, HLT_Jet50U
Era_2 141956-144114 2.9pb-1 /JetMET/Run2010A-Nov4ReReco_v1/RECOCert_136033-149442_7TeV_Nov4ReReco_Collisions10_JSON.txtHLT_Jet30U, HLT_Jet50U
Era_3 146428-147116 5.6pb-1 /Jet/Run2010B-Nov4ReReco_v1/RECOCert_136033-149442_7TeV_Nov4ReReco_Collisions10_JSON.txtHLT_Jet30U, HLT_Jet50U, HLT_Jet70U
Era_4 147196-148058 9.5pb-1 /Jet/Run2010B-Nov4ReReco_v1/RECOCert_136033-149442_7TeV_Nov4ReReco_Collisions10_JSON.txtHLT_Jet30U, HLT_Jet50U, HLT_Jet70U_v2, HLT_Jet100U_v2
Era_5 148822-149294 18.3pb-1 /Jet/Run2010B-Nov4ReReco_v1/RECOCert_136033-149442_7TeV_Nov4ReReco_Collisions10_JSON.txtHLT_Jet30U_v3, HLT_Jet50U_v3, HLT_Jet70U_v3, HLT_Jet100U_v3, HLT_Jet140U_v3
• Data were spitted to 5 eras according to different luminosities and trigger conditions.
• Below in the Table we present for each era:• The run range• The total Integrated Luminosity• The latest Nov4ReReco and JSON file used• The triggers involved in the analysis (prescaled in
red, unprescaled in green).
P.Kokkas, Univ. of Ioannina 4
Hadron Level Various MC
• The following MC Samples (available up to now) were also used:• Pythia6 TuneZ2 Fall10: QCD_Pt-xxtoxx_TuneZ2_7TeV-pythia6/Fall10-START38_V12-v1/GEN-SIM-RECO• Pythia8 Tune1 Fall10: QCD_Pt_xxtoxx_Tune1_7TeV_pythia8/Fall10-START38_V12-v1/GEN-SIM-RECO• Madgraph TuneD6T Fall10 : QCD_TuneD6T_HT-xxx_7TeV_madgraph/Fall10-START38_V12-v1/GEN-SIM-RECO• Alpgen TuneZ2 Fall10: QCDXJets_Pt-xxtoxx_TuneZ2_7TeV_alpgen/Fall10-START38_V12-v1/GEN-SIM-RECO• Pythia6 D6T Spring10: QCDDiJet_Ptxxtoxx/Spring10-START3X_V26_S09-v1/GEN-SIM-RECO
• On the right we see the predictions of above MCs at hadron level.
• The new MCs :• Herwig++ Tune23 Fall10 (Flat)• Pythia6 D6T Fall10 (Flat or slices)
will also be added in the next weeks (Not available for analysis at some QCD T2).
P.Kokkas, Univ. of Ioannina 5
Analysis JEC-Selection
• Analysis with CMSSW_3_8_6
• Jets were reconstructed using the antikt (R=0.5) clustering algorithm.
• PF + Calo jets were corrected for energy loss and effects due to non-linear response of calorimeter• Relative (corrects for η dependence) (Data & MC)
[Spring10_L2Relative_AK5PPF , Spring10_L2Relative_AK5Calo ]• Absolute (corrects for the pT dependence) (Data & MC)
[Spring10_L3Absolute_AK5PF , Spring10_L3Absolute_AK5Calo]• Residual corrections for η>1.5 only to Data
[Spring10DataV1_L2L3Residual_AK5PF , Spring10DataV1_L2L3Residual_AK5Calo]
• On line Selection:• Technical bit 0, and halo bits (None of Technical bits 36,37,38,39) NOT USED!• Select events with HLT single Jet triggers: HLT Jet30U , HLT Jet50U etc
• Off line Selection:• Primary Vertex: |PVz| < 24 cm, nDof > 4• Jet selection: pT ≥ 50 GeV and |y|≤2.5• “Loose” Jet ID for PF and Calo jets .
6
Trigger Efficiencies
HLT Jet70U
HLT Jet50U
HLT Jet30U
HLT Jet140U_v3
HLT Jet100U
• Trigger Efficiencies were studied in detail for all data eras.
• Below the efficiencies of main triggers versus HT in the case of nJets ≥2 and nJets ≥3.
P.Kokkas, Univ. of Ioannina 7
Combining Triggers
HLT Jet Trigger HT nJets≥2 (GeV)
HT nJets≥3 (GeV)
HLT Jet30U 130 180
HLT Jet50U 260 280
HLT Jet70U 360 380
HLT Jet100U 520 540
HLT Jet140U 700 750
HLT Jet Trigger HT (GeV) Lumi HLT Jet30U 200-310 352nb-1
HLT Jet50U 310-400 3.5 pb-1
HLT Jet70U 400-560 9.2 pb-1
HLT Jet100U 560-800 19.8 pb-1
HLT Jet140U 800- 36 pb-1
• The table on the right shows the HT values where every trigger becomes fully efficient.
• The table below-left shows for every trigger used : the HT range and the corresponding Integrated Luminosity.
• The figure below-right shows how we combine the triggers to extract our measurement.
8
Data stability : Era1 (PF Jets)
nJets≥2 (HLT_Jet50U)
nJets≥3 (HLT_Jet50U)
(nJets≥3)/(nJets≥2) (HLT_Jet50U)
• To control the Data Stability over the whole period we produced for each era the following plots:• Number of events per nb-1 for of nJets ≥2 and nJets ≥3 (Luminosity dependent).• Ratio events (nJets ≥3)/(nJets ≥2) (Luminosity independent) .
P.Kokkas, Univ. of Ioannina 9
Data stability : Era2 (PF Jets)
nJets≥2 (HLT_Jet50U)
nJets≥3 (HLT_Jet50U)
(nJets≥3)/(nJets≥2) (HLT_Jet50U)
P.Kokkas, Univ. of Ioannina 10
Data stability : Era3 (PF Jets)
nJets≥2 (HLT_Jet70U) nJets≥3 (HLT_Jet70U)
(nJets≥3)/(nJets≥2) (HLT_Jet70U)
P.Kokkas, Univ. of Ioannina 11
Data stability : Era4 (PF Jets)
nJets≥2 (HLT_Jet100U) nJets≥3 (HLT_Jet100U)
(nJets≥3)/(nJets≥2) (HLT_Jet100U)
P.Kokkas, Univ. of Ioannina 12
Data stability : Era5 (PF Jets)
nJets≥2 (HLT_Jet140U) nJets≥3 (HLT_Jet140U)
(nJets≥3)/(nJets≥2) (HLT_Jet140U)
• No bad runs were spotted for any era.• No slope was observed for any era.
13
Data over MC : HLT_Jet30U (PF Jets : HT > 200 GeV)
nJets ≥2
nJets ≥3
PYTHIA6 TuneZ2 Fall10 MC normalized to the total number of inclusive DiJet events for HT>200GeV.
14
Data over MC : HLT_Jet50U (PF Jets : HT > 310 GeV)
nJets ≥2
nJets ≥3
PYTHIA6 TuneZ2 Fall10 MC normalized to the total number of inclusive DiJet events for HT>310GeV.
15
Data over MC : HLT_Jet70U (PF Jets : HT > 400 GeV)
nJets ≥2
nJets ≥3
PYTHIA6 TuneZ2 Fall10 MC normalized to the total number of inclusive DiJet events for HT>400GeV.
16
Data over MC : HLT_Jet100U (PF Jets : HT > 560 GeV)
nJets ≥2
nJets ≥3
PYTHIA6 TuneZ2 Fall10 MC normalized to the total number of inclusive DiJet events for HT>560GeV.
17
Data over MC : HLT_Jet140U (PF Jets : HT > 800 GeV)
nJets ≥2
nJets ≥3
PYTHIA6 TuneZ2 Fall10 MC normalized to the total number of inclusive DiJet events for HT>800GeV.
P.Kokkas, Univ. of Ioannina 18
Data over MC – R32
• pT , y and phi Data distributions have been compared with PYTHIA6 TuneZ2 Fall10 MC.• No major discrepancies have been observed. However there are discrepancies in all kinematic
distributions which must be addressed and a systematic error must be assigned to it.• Shown bellow is the measured ratio with PF Jets.
• Multiplicative Correction factor to go to hadron level.
R32 with PF Jets
Multiplicative Correction factor ≈1-2%
19
Ratio at Hadron level
• The measured ratio rises, due to phase space, with HT . Above HT≈0.8 TeV it reaches a plateau which is most sensitive to αs.
• Errors are only statistical.• PYTHIA6 and MadGraph show better agreement with data however the full systematic error is not yet known .• It appears that PYTHIA8 and Alpgen do not agree with the measurement.
P.Kokkas, Univ. of Ioannina 20
Ratio at Hadron level
• Measured ratio seems to be closer to Madgraph (systematics pending).
21
Ratio at Hadron Level
• Analysis with Calo Jets gives very similar result.
P.Kokkas, Univ. of Ioannina 22
New result & ICHEP
• The new measurement with 36 pb-1 is in agreement with the previous CMS public result (ICHEP result.)
23
Summary
P.Kokkas, Univ. of Ioannina
• Summary:• The ratio of the inclusive three-jet over two-jet cross sections as a function of the
total jet transverse energy, HT, has been measured with the CMS detector at the LHC for proton-proton center-of-mass energy 7 TeV using an integrated luminosity of 36 pb-1.
• Measurements have been performed for jets with pT ≥50 GeV in the rapidity range |y| ≤2.5.
• The measured ratio rises, due to phase space, with HT . Above HT≈0.8 TeV it reaches a plateau which is most sensitive to αs.
• Study of Systematic uncertainties is on the way:• Uncertainties due Jet Energy Scale (PAS JME 10-010) are expected to be ≈1%. • Systematic uncertainties due to difference in shape between data and MC and pileup
are under investigation. • PYTHIA6 and MadGraph show better agreement with data however the full
systematic error is not yet known .• It appears that PYTHIA8 and Alpgen do not agree with the measurement.
P.Kokkas, Univ. of Ioannina 24
Spare
P.Kokkas, Univ. of Ioannina 25
Data over MC
Data over MC ratiosPF Jets
26
Dat
a - M
C : H
LT_J
et30
U (P
F Je
ts :
HT >
200
GeV
)
27
Dat
a - M
C : H
LT_J
et50
U (P
F Je
ts :
HT >
310
GeV
)
P.Kokkas, Univ. of Ioannina 28
Dat
a - M
C : H
LT_J
et70
U (P
F Je
ts :
HT >
400
GeV
)
P.Kokkas, Univ. of Ioannina 29
Dat
a - M
C : H
LT_J
et10
0U (P
F Je
ts :
HT >
560
GeV
)
P.Kokkas, Univ. of Ioannina 30
Dat
a - M
C : H
LT_J
et14
0U (P
F Je
ts :
HT >
800
GeV
)
P.Kokkas, Univ. of Ioannina 31
Method of extracting R32
T
CaloSmear
T ΔH
jetsN
ε
C
dH
dσ
L
Inclusive jetcross section
sizebin H the: ΔH
bin ain counted events ofnumber : jetsN
ibin in eventsGen ofNumber
ibin at eventsGen from events Calo tedreconstruc ofNumber ε
cuts survived eventsfor efficiency the: ε
luminocity integrated the:
ibin in events Calo tedreconstruc ofNumber
ibin at eventsGen from events Calo tedreconstruc ofNumber C
correction smearing : C
TT
Calo
Smear
Smear
L
Smear2
2
3
Smear3
T
CaloT
Calo
T
Calo
2
Smear2
T
Calo
3
Smear3
T
2
T
3
C
ε
ε
C
ΔH
2Jetsn N
ΔH
3Jetsn N
ΔH
2Jetsn N
ε
C
ΔH
3Jetsn N
ε
C
dH
dσdH
dσ
32R
L
LRatio R32
A Bmeasurement
• The factor AxB has been used to correct the Calo Level ratio to stable particle level (Hadron Level).
P.Kokkas, Univ. of Ioannina 32
Method of extracting R32
3 jetsn N
3 jetsn N
3 jetsn N
3 jetsn NA
Calo
CaloPass
CaloPass
Gen
2 jetsn N
2 jetsn N
2 jetsn N
2 jetsn NB
Gen
CaloPass
CaloPass
Calo
H of ibin in eventsGen ofNumber : 2,3 jetsn N TGen
TCalo H of ibin in events Calo tedreconstruc ofNumber : 2,3 jetsn N
bin any appear to and cuts survived events
Calo tedreconstruc allH of ibin of eventsGen For : 2,3 jetsn N TCaloPass
1/ε3 (1/efficiency)nJets≥3
CSmear3
Smearing correctionnJets≥3
ε2 (efficiency)nJets≥2
1/CSmear2
Smearing correctionnJets≥2
With
• This MC driven method of extracting R32 from the data does not depend upon the absolute predictions of the MC programs .
• It does depend on how well the MC distributions describe the shape of the data distributions.
• As we have seen in the previous slides PYTHIA6 describes well the shapes of the data distributions, hence we are entitle to use them to derive the AxB correction factor to the data.
P.Kokkas, Univ. of Ioannina 33
Ratio PF-Calo Level
P.Kokkas, Univ. of Ioannina 34
Ratio for HT<1TeV
• For HT<1TeV the measured ratio is closer to Madgraph (systematics pending).