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Advances in perturbative QCD for LHC physics Frank Petriello APS April meeting April 2007
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Advances in perturbative QCDfor LHC physics

Frank Petriello

APS April meetingApril 2007

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Outline

MotivationImportance of perturbative QCD at collidersTesting tools with HERA, Tevatron data

Merging LO with parton showersStatus of NLO calculations

LHC phenomenology at NLODifficulties at NLO: processesNew techniques for NLO calculations

Status of NNLO calculationsDGLAP evolution at NNLONNLO cross sections with spin correlations and Tevatron data

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Physics at the LHC

LHC turns on in year!Excellent discovery reach at TeV:

SUSY: squark/gluino reach of 2.5-3 TeV, graviton reach of 5-6 TeV

Enormous event rates at /year:: events: events

: eventsHiggs ( GeV): events

Both an opportunity (precision, low systematics) and achallenge (backgrounds)

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Physics at the LHC

Not all discovery channels producedramatic signatures!

Need theoretical control of distribution shapes,backgrounds, uncertainties, . . .

Measurements of new physics parametersneeds theory

Incorrect theory leads to:

Tevatron high jetsTevatron -meson productionNuTeVBrookhaven of the muon

signal

background

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Bottom production at the Tevatron

Long-standing discrepancy for -hadron productionTevatron Run I: factor of higher than QCD prediction!Motivated light sbottom/gluino interpretation of data (Berger et al.)

Missing theory components: inconsistent fragmentation functions,updated PDF extractions, resummation, underestimated uncertainties,(Cacciari et al.)Detailed theory analysis needed to understand data

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SUSY searches and PYTHIA

: standard SUSY discriminator

Current tools (PYTHIA) underestimate background by factor of 10! (Mangano et al.)PYTHIA: extra jets generated via parton shower wrong hard emissions

Need exact matrix elements from QCD

Incorrect simulation in ATLAS TDR

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Moral

Moral: need systematic, controlled QCD expansionpQCD expansion in augmented with necessary resummationCross-check and improve simulation tools

Issues to consider:Are the kinematics described correctly?What is the correct normalization, and what is its uncertainty?Where do new qualitative effects like the gluon pdf (large at the LHC) appear in thecalculation?Have kinematic boundaries where resummation may be required been considered?

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QCD at hadron colliders

Observables in hadronic collisions

Requireluminosity measurementparton distribution functionsscattering cross sections

All of these require precise QCD cross sections!

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Cross sections in QCD

, ,

Strong coupling constant not small:Contains scales

Get scales from UV and IR renormalizationScales are arbitrary:

but truncation of expansion at induces a scale dependence ofResidual scale dependences provide estimate of neglected higher order effects

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Parton shower simulations

Usual first attempt at hadron collider predictionBegin with: PS generates shower for each line:

In the soft+collinear limit, extra emissions simplifyCan sum to all orders, incorporates large swath of QCD correctionsDoesn’t get extra hard jet, need exact matrix elementsthis was the SUSY study problem shown beforeAlso misses correlations between extra jetsCan the resummation and the hard emissions be combined?

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Merging LO with parton showers

CKKW (Catani, Krauss, Kuhn, Webber): prescription to cover entire phase-space correctly

Define ; generate hard jets from MEs; feed this intoshowering algorithm and veto hard jets from shower

n jets)≥Multiplicity (0 1 2 3 4

)* γ(Z

n je

ts) /

+

* γ(Z

-410

-310

-210

-110

1-1DØ, 0.4 fb

DataMCFMME-PSPYTHIA

(GeV)TpJet 0 50 100 150 200 250 300

Even

ts/5

GeV

-110

1

10

210

310

-1DØ, 0.4 fb

+ DataME-PS

ME/PS matching describes Run II data well (hep-ex/0608052)

Codes: SHERPA includes ME generator, HERWIG, PYTHIA use external tree-levelgenerator (MADGRAPH) and apply CKKW (Mrenna, Richardson)

Kinematics seemingly well described by this procedure

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The need for NLO

Still not good enough for LHC physicsPredictions at LO suffer from debilitating theory errors

Example: jets, GeV, ,

N

3 6.47 pb 13.52 pb4 0.90 pb 2.48 pb

Uncertainty from variation must vanish at higher orders large NLO correctionsTypical NLO size: 30-100% not just naive expansion!

New channels open up at higher orders gluon pdf large at smallNew kinematics regions allowed generate , other effectsLarge coefficients in perturbative corrections ( for -channel processes)

NLO calculations needed for LHC physics!

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Status of NLO calculations

Parton-level results available for all and someprocesses:

AYLEN/EMILIA (de Florian et al.):DIPHOX (Aurenche et al.): ,HQQB (Dawson et al.):MCFM (Campbell, Ellis):NLOJET++ (Nagy): , ,VBFNLO (Figy et al.):

Recent:, (Cordero, Reina, Wackeroth hep-ph/0606102)(Campbell, Ellis, Zanderighi hep-ph/0608194)(Dittmaier, Uwer, Weinzierl, hep-ph/0703120)(Lazopoulos, Melnikov, FP, hep-ph/0703273)

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NLO wishlist

Campbell, KnutesonWant flexibile, automated approach many backgrounds, possible new states

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Calculation of an NLO component

7

Example of difficulty

Evaluate this integral via Passarino-Veltmanreduction. Result is …

Consider a tensor integral:

Bern

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The result...

8

Result of performing the integration

Numerical stability is a key issue.Clearly, there should be a better way

Bern

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Improved techniques for NLO

Sticking point: loops for external legsMuch recent activity on new methods:

Twistor-inspired: (Witten; Cachazo et al.; Bern, Dixon et al.; )

(b)(a)

++

++

+_

_ __

++

++

+

String theory in twistor-space QCD amplitudesUse “MHV” amplitudes rather than Feynman diagramsDrastically simplified analytic structure

Semi-numerical techniques: (Ellis, Giele, Zanderighi, et al.; Soper; Lazopoulos,Melnikov, FP; )

Can we avoid reducing the loop integrals, or store coefficients as numbers?Need to numerically handle IR singularities, internal thresholds,

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H+2 jets at NLO

QCD corrections to recently completed(Campbell, Ellis, Zanderighi hep-ph/0608194)

First output from semi-numerical methods for NLO computationsNLO needed for extraction of coupling in WBF

Residual scale dependence reduced; corrections are kinematic-independent

Maybe this kinematic independence is generic?

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+jet at NLO

QCD corrections to recently completed(Dittmaier, Uwer, Weinzierl hep-ph/0703120)

Background to Higgs in WBF, channels; measurement of properties

LO (CTEQ6L1)NLO (CTEQ6M)

pT,jet > 20GeV

√s = 14TeV

pp → tt̄+jet+X

µ/mt

σ[pb]

1010.1

1500

1000

500

0LO (CTEQ6L1)NLO (CTEQ6M)

pT,jet > 20GeV

!s = 1.96TeV

pp̄ " tt̄+jet+X

µ/mt

AtFB

1010.1

0.04

0.02

0

!0.02

!0.04

!0.06

!0.08

!0.1

!0.12

Residual scale dependence reducedNLO corrections wipe out forward-backward charge asymmetry!

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at NLO

QCD corrections to using numerical approach(Lazopoulos, Melnikov, FP hep-ph/0703273)

Background to various SUSY tri-lepton signatures, gauge boson coupling measurmentsCompletely numerical approach for loop calculations

Large, 50% corrections not seen by LO scale variation! 15% shift from pdfs,35% shift from termsInclusive -factor approximation works, however

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NLO summary

Corrections large, no obvious kinematic dependence pattern

for now, must have complete result for each process

New approaches that promise to simplifyand automate these calculations

Stay tuned for progress!

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Status of NNLO calculations

When is NNLO needed?When corrections are large ( production, fixed target energies for pdfs)For benchmark measurements, where expected errors are small ( production)Jet production at colliders:

What is known?Several inclusive processes ( production)(van Neerven, Harlander, Kilgore, Anastasiou, Melnikov, Ravindran, Smith)A few "semi-inclusive" distributions ( rapidity distributions)(Anastasiou, Dixon, Melnikov, FP)Fully differential result ( )(Anastasiou, Melnikov, FP)DGLAP splitting kernels (Moch, Vermaseran, Vogt)Generalization to processes ( ) very difficult

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DGLAP evolution

Full calculation of NNLO kernels recently completed(Moch,Vermaseren,Vogt)

Controls evolution of parton distribution functionsenters every hadron collider prediction!

-0.4

-0.3

-0.2

-0.1

0

0.1

0.2

0.3

0.4

10 -5 10 -4 10 -3 10 -2 10 -1 1x

d ln qS / d ln µf 2

LO

NLO

NNLO

µr = µf

x

NLO/LO

NNLO/NLO

αS = 0.2, nf = 40.8

1

1.2

1.4

1.6

1.8

2

10 -5 10 -4 10 -3 10 -2 10 -1 1

Corrections for

New color stucture at NNLO!

variation forfor

likely important for small

LHC probes low

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W,Z at NNLO

NNLO QCD result for production (Melnikov, FP)Needed for , pdfs, luminosity, calibration,Contains spin correlations, finite-width effects, interference, all kinematics

Residual scale dependences for standard cutsComparison with recent CDF result for forward production;take ratio of over

; ;potential stringent constraint on pdfs with more data

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Conclusions

Need more work on QCD tools for LHC physics!Need higher order QCD+resummation, fixed-order+MC matching,Must accurately quantify, reduce uncertainties; test at HERA, Tevatron

Highlights:Test of ME+PS merging on Tevatron +jetsNo obvious pattern in NLO corrections, except largeTheory progress on automated NLO coming! First results:large corrections badly missed by LO scale variationDGLAP kernels at NNLO precicion pdf extractionsDifferential result at NNLO with spin correlations for acceptancestested on Tevatron data, potential pdf implications


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