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Page 1: Jet Physics at CDF

Jet Physics at CDF

Sally SeidelUniversity of New Mexico

APS’99

24 March 1999

Page 2: Jet Physics at CDF

1. Jets at CDF

2. The Inclusive Jet Cross Section

3. The Dijet Mass Cross Section

4. The Differential Dijet Cross Section

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CDF: A multi-purpose detector for studying hadronic collisions

at the Fermilab Tevatron:

TeV 8.1at spp

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The motivation:

Jet distributions at colliders can:

• signal new particles

• test QCD predictions

• check parton distribution functions

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The data:

CDF reconstructs jets using an iterative cone algorithm with cone radius

7.0)()( 22 R

Jet energies are corrected for

• calorimeter non-linearity

• uninstrumented regions

• contributions from spectator partons

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The iterative cone algorithm:

•Examine all calorimeter towers with ET > 1 GeV.

•Form preclusters from continuous groups of towers with monotonically decreasing ET.

•If a tower is outside a window of 7 x 7 towers from the seed of its cluster, start a new precluster with it.

•For each precluster, find the ET-weighted centroid with R = 0.7.

•Define the centroid to be the new cluster axis.

•Save all towers with ET > 100 MeV within R = 0.7 about the new axis.

•Iterate until the tower list is stable.

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The Inclusive Jet Cross Section

• For jet transverse energies in the range 40 < ET < 440 GeV: this probes distances down to 10-17 cm.

• The analysis:– For luminosity (88.8 ± 4.1) pb-1 – Trigger on jet-like events: accept 4

triggers with uncorrected ET thresholds at 20, 50, 70, and 100 GeV; correct for pre-scaling

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– Apply data quality requirements:zvertex< 60 cm to maintain projective

geometry of calorimeter towers

• 0.1 < |detector| < 0.7 for full containment of energy in central barrel

• Etotal < 1800 GeV to reject accelerator loss events

• Define ET = Esin and = missing ET. Require

to reject cosmic rays

– Correct (“unsmear”) observed ET for energy degradation and calorimeter resolution

6

all

T

T

E

ETE

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• Calculate the cross section:

TT E

N

LddE

dd

111

where

N = number of events

L = luminosity

range is 1.2

and ET bins have width 5 - 80 GeV

• Compare to EKS (Ellis, Kunszt, Soper) NLO calculation with CTEQ4M pdf and renormalization/factorization scale = ET

jet/2

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Systematic uncertainties (all uncorrelated)

on the inclusive jet cross section:

i. Calorimeter response to high-pT charged hadrons

ii. Calorimeter response to low-pT charged hadrons

iii. Energy scale stability (1%)

iv. Jet fragmentation model used in the simulation

v. Energy of the underlying event in the jet cone (30%)

vi. Calorimeter response to electrons + photons

vii. Modelling of the jet energy resolution function

viii. Luminosity (4.1%)

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The Dijet Mass Cross Section

•Many classes of new particles have a larger branching fraction to just 2 partons than to modes containing a lepton or a W/Z…so this can be a powerful way to search for new particles.

•The analysis:

•For luminosity (85.9 ± 4.1) pb-1

•Trigger on jet-like events

•Select events with 2 jets, both with |event| < 2.

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•Define * (1-2)/2, then require e2|*| < 5. This is the same as |cos*| = |tanh *| < 2/3 where * is the Rutherford scattering angle:

•Apply the data quality cuts.

•Correct for trigger efficiency, |zvertex| cut

efficiency, resolution, and calorimeter effects.

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•Define the dijet mass:

•Calculate the cross section:

where:

N = number of events, corrected for prescaling

L = luminosity

Mjj = 10% mass bins (consistent with detector resolution)

•Compare to JETRAD (Giele, Glover, Kosower) NLO calculation with CTEQ4M + = ET

max/2. Two partons are merged if they are within Rsep = 1.3 R.

jjjj M

N

LdM

d

1

)]cos()[cosh(2

)()(

21

221

221

TT

jj

EE

ppEEM

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The dijet mass cross section compared to JETRAD with

CTEQ4M:

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Compare results to data + JETRAD with other pdf’s:

Changing from 0.5 ETmax to 0.25 ET

max changes the normalization by 25%.

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Compare CDF and D0 results for CTEQ4M

(D0 examines || < 1 with no requirement on cos*)

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Systematic uncertainties on the dijet mass cross section (17-34%, asymmetric + ET-dependent):

• Absolute energy scale (14-31%):

•Calorimeter calibration: 1.3-1.8% over the ET range

• Jet fragmentation model: 1.2-1.7% over the ET range

•Calorimeter stability: 1% of E

•Energy of the underlying event: 1 GeV

• Unsmearing:

•Parameterization of the resolution function: 1-9% depending on Mjj

•Variation between analytic and MC procedure: ±4%

•Detector simulator energy scale: 2-8%

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•Relative jet energy scale (5-9% depending on Mjj and considering all instrumented regions):

•Other uncertainties:

•luminosity: 4.1%

•prescale factors: 1.7-3.5% depending on trigger used.

•|zvertex| cut efficiency: 1%

•trigger efficiency: < 1% depending on the statistics of the turn-on region of the trigger.

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The Dijet Differential Cross Section

•The rapidity dependence of the cross section probes the parton momentum fractions.

•The analysis:

•For luminosity (86.0 ± 4.1) pb-1

•Trigger on jet-like events; select events with 2 jets

•Apply data quality cuts

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•Order the jets by ET. Define:

•The “leading jet”: with highest ET. Require that it has 0.1 < |1| < 0.7 and ET1 > 40 GeV.

•The “probe jet”: with second highest ET. Require that it has ET2 > 10 GeV.

•Correct jet energies for calorimeter effects; require ET1 > 35 GeV.

•Classify events according to probe jet , 2:

0.1 < |2| < 0.7

0.7 < |2| < 1.4

1.4 < |2| < 2.1

2.1 < |2| < 3.0

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•Correct (“unsmear”) measured

•Correct for trigger efficiency, prescale, and vertex-finding efficiency

•For events in each of the 4 2 classes, calculate the cross section:

N = number of events, corrected for prescale

L = luminosity

ET1 bins are consistent with detector resolution

•Compare to JETRAD for 3 pdf’s + = ET

max/2

1

1

TT E

N

LdE

d

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Sources of systematic errors on the dijet differential cross section:

Same as for inclusive cross section + resolution

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Probing the high-x, high-Q2 regime:

Notice that for a two-body process,

and

so these data examine a range in (x,Q2)

including that where an excess was observed at HERA:

)( 21 ees

Ex T

)tanh1(cosh2

)cos1(2

ˆ

ˆ

**22

*

2

TE

s

tQ

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