status of nlojet++ for dijet angular distributions

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Status of NLOjet++ for dijet angular distributions Lee Pondrom University of Wisconsin 20 May 2010

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Status of NLOjet++ for dijet angular distributions. Lee Pondrom University of Wisconsin 20 May 2010. Ingredients. 1.1 fb -1 jet100 triggered data 1E10 nlojet++ events with CTEQ6 2E6 Pythia events with full CDFSim and CTEQ5 - PowerPoint PPT Presentation

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Page 1: Status of NLOjet++ for dijet angular distributions

Status of NLOjet++ for dijet angular distributions

Lee Pondrom

University of Wisconsin

20 May 2010

Page 2: Status of NLOjet++ for dijet angular distributions

Ingredients

• 1.1 fb-1 jet100 triggered data

• 1E10 nlojet++ events with CTEQ6

• 2E6 Pythia events with full CDFSim and CTEQ5

• 1E6 ‘standalone’ Pythia events with CTEQ6 and ISR, FSR turned off.

Page 3: Status of NLOjet++ for dijet angular distributions

Pythia first

• We have to use Pythia to correct the data to the hadron level.

• We use a calculation of the subprocess cross sections to understand Pythia.

• We learn that to reproduce the Pythia angular distributions, the 2->2 subprocesses with nonidentical final state partons must be u<->t symmetrized.

Page 4: Status of NLOjet++ for dijet angular distributions

2->2 symmetirzed jet_chi cross sections 600 GeV mass bin

Page 5: Status of NLOjet++ for dijet angular distributions

Key to previous slide

• q1q2->q1q2 t channel gluon exchange• q1q2bar->q1q2bar t channel gluon*• q1q1->q1q1 t channel gluon• q1q1bar->q2q2bar s channel annihilation• q1q1bar->q1q1bar s and t channels*• q1q1bar->glueglue s channel annihilation• glueglue->q1q1bar/glueglue* s and t • q1glue->q1glue compton* *=large

Page 6: Status of NLOjet++ for dijet angular distributions

2->2 subprocesses

• The peaks at =1 come from the u<->t symmetrization

• The t channel gluon exchange cross sections dominate, which is the motivation for the choice of scale Q2=pT

2.

• Now that we understand Pythia born, let us look at nlojet++ born

Page 7: Status of NLOjet++ for dijet angular distributions

2->2 Pythia compared to Nlojet born and jet_chi

Page 8: Status of NLOjet++ for dijet angular distributions

2->2 Pythia compared to Nlojet born and jet_chi

Page 9: Status of NLOjet++ for dijet angular distributions

Normalization

• Each set of four mass plots has one overall normalization.

• All programs agree on the 1/mass4 dependence of the cross section.

• Nlojet++ born agrees better with Pythia as the mass increases.

Page 10: Status of NLOjet++ for dijet angular distributions

conclusion

• We understand Pythia. It agrees well with the data, and strengthens the Pythia based quark substructure analysis.

• To compare nlojet++ to the data, we need to correct the data to the hadron level using Pythia

Page 11: Status of NLOjet++ for dijet angular distributions

Nlojet++ has no CDF trigger

• After jet energy corrections the 100 GeV trigger moves to about 125 GeV

• ET= M/(1+)=(Msin(*))/2 which has to be removed, in addition to other instrumental effects.

Page 12: Status of NLOjet++ for dijet angular distributions

125 GeV trigger threshold cut in the angular distribution

Page 13: Status of NLOjet++ for dijet angular distributions

Correct the data to the hadron level using Pythia MC

Page 14: Status of NLOjet++ for dijet angular distributions

Correct the data to the hadron level using Pythia MC

Page 15: Status of NLOjet++ for dijet angular distributions

Corrected data agree well with hadron level Pythia Q2=pT

2

Page 16: Status of NLOjet++ for dijet angular distributions

Corrected data agree well with hadron level Pythia Q2=pT

2

Page 17: Status of NLOjet++ for dijet angular distributions

2 for hadron level data compared to Q2=pT

2 Pythia noqsub

• 20 bins one parameter fits

• M (GeV) events (data) 2

• 600 150343 32

• 700 42106 38

• 800 11392 17

• 900 3134 17

Page 18: Status of NLOjet++ for dijet angular distributions

Jet-jet angular distribution and quark substructure

• Quark substructure effective contact color singlet Lagrangian of Eichten, et al is:

• L = ±(g²/2Λ²(LLLL

• Looks just like muon decay. Affects only the u and d quarks. Color singlet means that some diagrams have no interference term.

• g²/4 = 1; strength of the interaction ~(ŝ/²)²• This measurement is not sensitive to the interference

term.

_ _ _

Page 19: Status of NLOjet++ for dijet angular distributions

Dependence of the angular distributions

Page 20: Status of NLOjet++ for dijet angular distributions

Dependence of the angular distributions

Page 21: Status of NLOjet++ for dijet angular distributions

Plot the ratio R=(1<<7)/(7<<13) vs (mass)4 for each

Page 22: Status of NLOjet++ for dijet angular distributions

Fitted slopes vs (1/4) give sensitivity to quark substructure

Page 23: Status of NLOjet++ for dijet angular distributions

Run nlojet++ 1010 events 0=ETavge

Page 24: Status of NLOjet++ for dijet angular distributions

Vary 0 in NLOjet++

Page 25: Status of NLOjet++ for dijet angular distributions

Fit nlojet++ to hadron level data

Page 26: Status of NLOjet++ for dijet angular distributions

2 for one parameter fits to first 12 bins of data with nlojet++

• Mass GeV 0=Etav 0.7Etav 1.4Etav• 600 75 110 78• 700 75 48 65• 800 36 48 35• 900 37 35 37

• No fit is particularly good, compared to Pythia

Page 27: Status of NLOjet++ for dijet angular distributions

Compare lo and nlo 0=ETaveK factor 1.1

Page 28: Status of NLOjet++ for dijet angular distributions

Cuts in nlojet++

• For 2 partons with highest ET

• ET>10 GeV

• ||<2

• Cone size D=0.7 in (,) space

• Rsep = 1.3. D and Rsep govern when the third parton is included with one of the other two to form a ‘jet’. Should have no effect on a born calculation.

Page 29: Status of NLOjet++ for dijet angular distributions

Systematics

• Calculate R(Nlojet++) for 0=ETave, 0.7 ETave, and 1.4ETave.

• Calculate R(data) for level7JetE corrections, and 1 on JetE corrections

• Average the results <R(data)> and <R(Nlojet)>

Page 30: Status of NLOjet++ for dijet angular distributions

Table

• M(GeV) R(data) R(nlojet) ratio

• 600 .815.017 .818.009 1.0.02

• 700 .87.02 .81.01 1.07 .02

• 800 .85.05 .82.02 1.04.06

• 900 .92.09 .83.02 1.1.1

• Fitted slope s=0.160.07, intersept=1.0, 2=2.3

Page 31: Status of NLOjet++ for dijet angular distributions

R(data)/R(Nlojet++) vs (mass)4

Page 32: Status of NLOjet++ for dijet angular distributions

Conclusions

• The original Pythia based analysis has been repeated, with the following changes.

• Only Pythia with Q2=pT2 used.

• Data corrected to hadron level with Pythia

• Sensitivity to quark substructure uses Pythia integrated over smaller regions in to accommodate Nlojet++.

Page 33: Status of NLOjet++ for dijet angular distributions

Conclusions continued

• Systematics are included in the comparison of data to nlojet++ by varying the jet energy corrections in data and the hard scale 0 in nlojet++.

limit from the fitted slope: >2.1 TeV 95% confidence.

• Expected limit for zero slope is >2.6 TeV 95% confidence.