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Jet Physics at the Tevatron Sally Seidel University of New Mexico XXXVII Rencontres de Moriond For the CDF and D0 Collaborations

Jet Physics at the Tevatron

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Jet Physics at the Tevatron. Sally Seidel University of New Mexico XXXVII Rencontres de Moriond For the CDF and D0 Collaborations. An overview of selected jet studies by CDF and D0 in 2001-2. 1. Jets at CDF and D0 2. Inclusive Jet Production (CDF) - PowerPoint PPT Presentation

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Page 1: Jet Physics at the Tevatron

Jet Physics at the Tevatron

Sally SeidelUniversity of New Mexico

XXXVII Rencontres de Moriond

For the CDF and D0

Collaborations

Page 2: Jet Physics at the Tevatron

An overview of selected jet studies by CDF and D0 in 2001-2.

1. Jets at CDF and D0

2. Inclusive Jet Production (CDF)

3. Inclusive Jet and ET Dependence (D0)

4. s from Inclusive Jet Production (CDF)

5. Inclusive Jet Cross Section using the kT Algorithm (D0)

6. Ratios of Multijet Cross Sections (D0)

7. Subjet Multiplicity of g and q Jets using the kT Algorithm (D0)

8. Charged Jet Evolution and the Underlying Event (CDF)

Page 3: Jet Physics at the Tevatron

Jet distributions at colliders can:

• signal new particles + interactions

• test QCD predictions

• improve parton distribution functions

Page 4: Jet Physics at the Tevatron

CDF (D0) data quality and reconstruction requirements:• |zvertex | < 60 (50) cm to maintain projective

geometry of calorimeter towers.

• 0.1 (0.0) |detector| 0.7 (0.5) for full containment of energy in central barrel.

• To reject cosmic rays + misvertexed events, define = missing ET. Require

(CDF)

< (30 GeV or 0.3ETleading jet,

whichever is larger). (D0)• Reconstruct jets using a cone algorithm with

cone radius • Apply EM/HA + jet shape cuts to reject noise

fakes.

6

all

T

T

E

E

TE

TE

7.022 R

Page 5: Jet Physics at the Tevatron

Next correct for

•Pre-scaling of triggers.

•Detection efficiencies (typically 94 –100%).

•underlying event + multiple interactions.

•“smearing” of the data: the effects of detector response and resolution.

•If > 1 primary vertex:

•choose vertex with 2 highest ET jets. (CDF).

•choose 2 vertices with max track multiplicity, then choose the one with minimum . (D0)

No correction is made for jet energy deposited outside the cone by the fragmentation process, as this is included in the NLO calculations to which the data are compared.

jetE

Page 6: Jet Physics at the Tevatron

The Inclusive Jet Cross Section, E·d3/dp3 CDF

• For jet transverse energies achievable at the Tevatron, this probes distances down to 10-17 cm.

This is what’s measured.

ddE

d

Edp

dE

TT

2

3

3

2

1

LE

N

T

Page 7: Jet Physics at the Tevatron

(88.8 pb-1)(20.0 pb-1)

GeV 1800s

The CDF result for unsmeared data:

Page 8: Jet Physics at the Tevatron

New in this analysis: compare raw data to smeared theory. This uncouples the systematic shift in the cross section associated with smearing from the statistical uncertainty on the data.

•Consider only uncorrelated uncertainties first.

•Develop a 2 fitting technique that includes experimental uncertainties, to quantify the degree to which each theory reproduces the data.

Page 9: Jet Physics at the Tevatron

Define

where:

nd = observed # jets in bin i

nt = predicted # jets in bin i

t = uncertainty on prediction

sk,t= shift in kth systematic for tth theoretical prediction

Term 1: uncorrelated scatter of points about a smooth curve

Term 2: 2 penalty from systematic uncertainties

8

1

2,

12

22 ))()((

ktk

nbin

i t

tdt s

inin

Page 10: Jet Physics at the Tevatron

Begin with nt0: nominal prediction by

theory t. Smear prediction separately for each systematic uncertainty k to get smeared prediction nt

k. The systematic

uncertainty in bin i is then

)()()( 0 ininif tkt

kt

Predicted # jets in bin i is

)()(8

1,

0 ifsnin kt

ktktt

Use this nt(i) to calculate (uncorrelated) statistical uncertainty. The sk are chosen to minimize total 2 using MINUIT.

Page 11: Jet Physics at the Tevatron

Example resulting 2 values:

CTEQ4M: 63.4

CTEQ4HJ: 46.8

MRST: 49.5

This suggests that CTEQ4HJ best describes the data. But combinations of the 8 systematics can cancel. To study this, redo the fit separately for every combination of systematics. For:

NO systematics: 2 = 94.2

4 systematics: best 2 = 47.6

8 systematics: best 2 = 46.8

The normalization systematic can be cancelled by shape systematics.

Page 12: Jet Physics at the Tevatron

To extract confidence levels:

•Generate fake raw data (“pseudo-experiments”) using CTEQ4HJ. Predict nominal # entries for each of the 33 bins. Vary each prediction with 33 (statistical) + 8 (systematic) random numbers. Assume systematics are gaussian but ET dependent. Repeat for other PDF’s.

•Fit each pseudo-experiment to the nominal PDF prediction using 2.

Page 13: Jet Physics at the Tevatron

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Calculate 2 between data and smeared theory. Integral of the distribution above this 2 is the CL.

Page 14: Jet Physics at the Tevatron

Results, for 33 dof:

CTEQ4HJ: 10% CL

MRST: 7% CL (relatively high value because normalization systematic is cancelled by shape systematics).

All other PDF’s: < 5% CL

CTEQ4M: 1.4% CL, change in agreement with data above 250 GeV cannot be accounted for.

Page 15: Jet Physics at the Tevatron

CDF conclusion on inclusive jet cross section measurement:

•predictions using CTEQ4HJ have best agreement with data in both shape and normalization before considering systematics.

•when systematics are included, some combinations cancel out to produce only small changes in the spectrum shape. CTEQ4HJ provides the best prediction, followed by MRST.

•CDF Run Ib data are consistent with Run Ia and with NLO QCD given the flexibility allowed by current knowledge of PDF’s. CDF is also consistent with D0.

Page 16: Jet Physics at the Tevatron

The Inclusive Jet Cross Section versus

Pseudorapidity and ET

D0Extends the kinematic range

beyond previous measurements:Title:fig0.dviCreator:dvipsk 5.66a Copyright 1986-97 Radical Eye Software (www.radicaleye.com)Preview:This EPS picture was not savedwith a preview included in it.Comment:This EPS picture will print to aPostScript printer, but not toother types of printers.

Page 17: Jet Physics at the Tevatron

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D0 result, with cone algorithm, for 95 pb-1 at 1800 GeV:

Page 18: Jet Physics at the Tevatron

2 Comparison of D0 data and theory:

i.) Define

ii.) Construct the Cij by analyzing the correlation of uncertainties between each pair of bins. (Bin-to-bin correlations for representative bins are ~ 40% + positive.)

iii.) There are 90 -ET bins.

matrix covariancey uncertaint

theoryby the predicted jets ofnumber

data in the observed jets ofnumber

#bin

where, 1

,

2

C

T

D

i

TDCTD jjijji

ii

Page 19: Jet Physics at the Tevatron

Conclusions:

PDF 2/dof Probability

CTEQ4HJ 0.66 0.99

MRSTg 0.95 0.63

CTEQ4M 1.03 0.41

MRST 1.26 0.05

Page 20: Jet Physics at the Tevatron

Measurement of s from Inclusive Jet Production

CDF

),,()(1

),(ˆ

1

)0(2

TFRRs

TFsT

Ek

EXdE

d

The cross section and s are related at NLO by:

In the Tevatron ET regime, non-perturbative contributions are negligible.1

1S.D. Ellis et al., PRL 69, 3615 (1992).

Page 21: Jet Physics at the Tevatron

Procedure:

•The and k1 are calculated with JETRAD1 for given2 matrix elements, in the scheme. Clustering and cuts are applied directly to the partons.

•The 33 ET bins provide independent measurements at 33 values of R = F.

•Evolve the measured s values:

1W. Giele et al., PRL 73, 2019 (1994) and Nucl. Phys. B403, 633 (1993)2R.K. Ellis and J. Sexton, Nucl. Phys. B 269, 445 (1986).

)0(X̂

SM

21

0

10

24

38306

,6

233

)/ln())()((1)(

f

f

ZRRsRs

sZa

nb

nb

MbbM

Page 22: Jet Physics at the Tevatron

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•Result, for 87 pb-1, with CTEQ4M :•Average of results is s =

s evolution verified for 40 < ET < 250 GeV :

27 values of s(MZ) are ET-independent.

syst.). (exp. (stat) 1000.01178.0 0.00810095.0

ET (GeV)

Page 23: Jet Physics at the Tevatron

Theoretical uncertainties due to:

ET/2 < < 2ET:

PDF: 5% (extracted s values are consistent with those in PDF’s.)

1.3 < Rsep < 2.0: 2-3%

%6%4

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Page 24: Jet Physics at the Tevatron

The Inclusive Jet Cross Section using the kT

Algorithm D0

The kT algorithm differs from the cone algorithm because

•Particles with overlapping calorimeter clusters are assigned to jets unambiguously.

•Same jet definitions at parton and detector levels: no Rsep parameter needed.

•NNLO predictions remain infrared safe.

Page 25: Jet Physics at the Tevatron

The kT algorithm successively merges pairs of nearby objects (partons, particles, towers) in order of increasing relative pT.

Parameter D controls the end of merging, characterizes jet size.

Every object is uniquely assigned to one jet.

Infrared + collinear safe to all orders.

Page 26: Jet Physics at the Tevatron

D0 kT Algorithm1:

1) For each object i with pTi, define dii = (pTi)2

2) For each object pair i, j, define

•(Rij)2 = (ij)2 + (ij)2

•dij = min[(pTi)2,(pTj)2]·(Rij)2/D2

3) If the min of all dii and dij is a dij, i and j are combined; otherwise i is defined as a jet.

4) Continue until all objects are combined into jets.

5) Choose D = 1.0 to obtain NLO prediction identical to that for R = 0.7 cone.1Based on S.D. Ellis and D. Soper, PRD 48. 3160 (1993).

Page 27: Jet Physics at the Tevatron

kT jets do not have to include all objects in a cone of radius D, and may include objects outside cone.

D0 result for 87 pb-1, unsmeared data, ||<0.5, statistical errors only:

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Page 28: Jet Physics at the Tevatron

Title:este.epsCreator:HIGZ Version 1.23/07Preview:This EPS picture was not savedwith a preview included in it.Comment:This EPS picture will print to aPostScript printer, but not toother types of printers.

Theory below data by 50% at low pT, by (10 - 20)% for pT > 200 GeV/c.

NLO predictions with kT and cone are within 1%.

Cross section measured with kT is 37% higher than with cone.

Page 29: Jet Physics at the Tevatron

Effect of final state hadronization studied with HERWIG:

For 24 d.o.f., 2 calculated with covariance technique:

PDF 2/dof Prob.

MRST + hadr. 1.00 0.46 CTEQ4HJ + hadr. 1.01 0.44 MRST 1.12 0.31 MRSTg 1.17 0.25 CTEQ4M 1.30 0.15 MRSTg 1.38 0.10

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Page 30: Jet Physics at the Tevatron

Ratios of Multijet Cross Sections

D0

This study measures

as a function of . Compare to JETRAD with CTEQ4M for several choices of renormalization scale using a 2 covariance technique.

)2 X; jets (

)3 X; jets (32

mmpp

nnppR

jetTT EH

Page 31: Jet Physics at the Tevatron

Recall F controls infrared divergences; R controls ultraviolet. Assume R= F.

Test four options:

R = for leading 2 jets and

(a) R = also for third jet.

(b) R = ET for third jet.

(c) R = 2ET for third jet.

R = 0.6 ETmax for all 3 jets.

jetTE

jetTE

Page 32: Jet Physics at the Tevatron

Result, for 10 pb-1:Title:/home/gallas/mult/eps/r32_ht_203040_nt.epsCreator:HIGZ Version 1.23/09Preview:This EPS picture was not savedwith a preview included in it.Comment:This EPS picture will print to aPostScript printer, but not toother types of printers.

Page 33: Jet Physics at the Tevatron

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•No prediction accurately describes the data throughout the full kinematic region.

•A single R assumption is adequate: introduction of additional scales does not improve agreement with data.

• R = 0.3 is consistent with the data.

jetTE

Page 34: Jet Physics at the Tevatron

Subjet Multiplicity of Gluon and Quark Jets Reconstructed with the kT Algorithm

D0This study examines

•pT and direction of kT jets

•event-by-event comparison of kT and cone

•multiplicity structure of quark and gluon jets

Page 35: Jet Physics at the Tevatron

Calibration of jet momentum:

responsedetector

where

),(

),,(

R

ppp

pR

pLppp

environunderlyingoffset

jetjet

jetT

jetoffset

measjettrue

jet

To find penviron (from U noise, multiple interactions, pile-up) : overlay HERWIG events with zero-bias (random crossing) events at various luminosities.

Observation: penviron for (D = 1.0) kT is 50-75% higher (i.e., 1 GeV/jet) than for (R = 0.7) cone.

Page 36: Jet Physics at the Tevatron

To find punderlying:

(1) overlay HERWIG events with minimum-bias (coincidence in hodoscopes) data at low luminosity (negligible environment)

(2) overlay HERWIG events with zero-bias events at low luminosity

(3) subtract: (1) - (2).

Observation: punderlying for (D = 1.0) kT is 30% higher than for (R = 0.7) cone.

Page 37: Jet Physics at the Tevatron

To find R:

(1) calibrate EM energy scale with Z, J, 0 decays

(2) require pT conservation in -jet events:

R consistent for kT and cone jets.

T

TTrcalorimete p

nER

ˆ1

Page 38: Jet Physics at the Tevatron

Comparison of kT and cone jet reconstruction for 2 leading jets in 69k Run 1b events:

99.94% of jets reconstructed within R < 0.5.

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Page 39: Jet Physics at the Tevatron

systematically higher than by 3-6%:

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jetkT

Tp jetconeTE

Page 40: Jet Physics at the Tevatron

Subjets

Reapply kT algorithm to each jet, using its preclusters, until all remaining objects have

)(),min( 22

22

,2

, jetpyD

Rppd tcut

ijjTiTij

These are subjets, defined by fractional pT and separation in space. Multiplicity M depends on:

•color factor (gluon > quark)

•ycut: ycut = 0 M = # preclusters

ycut = 1 M = 1

Choose ycut = 10-3.

s

Page 41: Jet Physics at the Tevatron

Select gluon-enriched and quark-enriched data samples:

PDF data show that fraction of gluon jets decreases with x pT/ .

•Select jets with same pT at = 630 GeV and = 1800 GeV for 2-jet events.

s

s s

Page 42: Jet Physics at the Tevatron

•Use HERWIG with CTEQ4M to predict gluon jet fraction f. LO calculation is algorithm-independent.

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•Identify reconstructed jets with type of nearest parton. Gluon jet fractions for 55 < pT < 100 GeV/c:

f1800: 0.59

f630: 0.33

Page 43: Jet Physics at the Tevatron

Multiplicity M measured in the data is related to gluon jet multiplicity Mg and quark jet multiplicity Mq by:

qg MffMM )1(

For Mg, Mq independent of , s

6301800

18006306301800

6301800

63018001800630

and

)1()1(

ff

MfMfM

ff

MfMfM

q

g

•Correct result for shower detection effects in calorimeter.

Page 44: Jet Physics at the Tevatron

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Mean subjet multiplicities:

•gluon jets: 2.21 0.03

•quark jets: 1.69 0.04

after unsmearing,

22.018.015.084.1

1

1

q

g

M

Mr

Page 45: Jet Physics at the Tevatron

Charged Jet Evolution and the Underlying Event

CDF

A two-part analysis: Data are compared to HERWIG, ISAJET, and PYTHIA for

• observables associated with the leading charged jet: the hard scatter.

•global observables used to study the behavior of the underlying event.

Page 46: Jet Physics at the Tevatron

The data:

•minimum bias (one interaction each with forward + backward beam-beam counters) and charged jets with ||<1, 50 GeV/c > pT > 0.5 GeV/c.

•measured in the central tracker: pT/pT

2 0.002 (GeV/c)-1

•impact parameter cut, vertex cut, to ensure 1 primary vertex.

•no correction for track finding efficiency (92% correction applied to models).

Page 47: Jet Physics at the Tevatron

The models:

•pthard > 3 GeV/c, to guarantee

22 ‹ total inelastic

•All assume superposition of

•the hard scatter

•the underlying event: beam-beam remnants, initial state radiation, and multiple parton scattering

•but different models for underlying event...

Page 48: Jet Physics at the Tevatron

•HERWIG: soft collision between 2 beam “clusters.”

•ISAJET: “cut Pomeron” similar to soft min bias. Independent fragmentation allows tracing of particles to origin: beam-beam, initial state rad, hard scatter + final state rad.

•PYTHIA: non-radiating beam remnants + multiple parton interactions with different effective minimum pT options: 0, 1.4, and 1.9 GeV/c. No independent fragmentation: cannot distinguish initial from final state radiation but can distinguish beam-beam.

Page 49: Jet Physics at the Tevatron

The standard CDF jet algorithm based on calorimeter towers is not directly applicable to charged particles. A naive jet algorithm is used because it can be applied at low pT:

•define jet as a circular region with radius

•Order all charged particles by pT.

•Start with particle with pTmax , include in

the jet all particles within R = 0.7. Recalculate centroid after each addition.

•Go to next highest pT particle and construct new jet around its R = 0.7.

•Continue until all particles are in a jet.

•Jet can extend beyond || < 1.

7.022 R

Page 50: Jet Physics at the Tevatron

Results on the leading jet:

The QCD hard scattering models describe these observables for the leading (highest ) charged jet well:

•multiplicity of charged particles

•size

•radial distribution of charged particles and pT around jet direction

•momentum distribution of charged particles

Charged particle clusters evident in the minimum bias data above pT 2 GeV/c

a continuation of the high pT jets in the jet trigger samples.

Tp

Page 51: Jet Physics at the Tevatron

To study the underlying event, global observables

<charged multiplicity> and

< >

are correlated with angle relative to axis of leading jet. Region transverse to leading jet (normal to the plane of the 22 parton hard scatter) is most sensitive to beam-beam fragments and initial state radiation.

Tp

Page 52: Jet Physics at the Tevatron

Observation: <charged multiplicity> and < > grow rapidly with pT

leading, then plateau at pT

leading > 5 GeV/c. Tp

Plateau height in transverse direction is half height in direction of leading jet.

Page 53: Jet Physics at the Tevatron

PYTHIA 6.115 best model for <charged multiplicity> in tranverse region but over-estimates in direction of leading jet. ISAJET shows right activity but wrong pT dependence:

Page 54: Jet Physics at the Tevatron

ISAJET uses independent fragmentation (too many soft hadrons when partons overlap) and leading log picture without color coherence (no angle ordering within the shower):

Page 55: Jet Physics at the Tevatron

HERWIG + PYTHIA model hard scatter (esp. initial state radiation) component of underlying event best:

Page 56: Jet Physics at the Tevatron

HERWIG lacks adequate : Tp

Page 57: Jet Physics at the Tevatron

Summary:

Many interesting and significant results from D0 and CDF in

•Inclusive jets

s

•kT algorithm

•Multijet production

•Particle evolution

•Underlying event

On to Run II!