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LoopFest VII May, 2008, Buffalo. NLO Q C D corrections to WW + 1-jet production at hadron colliders. Peter Uwer *). Universität Karlsruhe. Work in collaboration with S.Dittmaier, S. Kallweit. - PowerPoint PPT Presentation
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Peter Uwer *) Universität Karlsruhe Financed through Heisenberg fellowship and SFB-TR09 LoopFest VII May, 2008, Buffalo NLO QCD corrections to WW + 1-jet production at hadron colliders Work in collaboration with S.Dittmaier, S. Kallweit Comparable results by [Campbell, Ellis, Zanderighi] and [Binoth, Guillet, Karg, Kauer, Sanguinetti]
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Page 1: Peter Uwer *)

Peter Uwer*)

Universität Karlsruhe

*) Financed through Heisenberg fellowship and SFB-TR09

LoopFest VII May, 2008, Buffalo

NLO QCD corrections to WW + 1-jet production at hadron colliders

Work in collaboration with S.Dittmaier, S. Kallweit

Comparable results by [Campbell, Ellis, Zanderighi] and [Binoth, Guillet, Karg, Kauer, Sanguinetti]

Page 2: Peter Uwer *)

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Contents

1. Introduction

2. Methods

3. Results

4. Conclusion / Outlook

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WW + 1-Jet ― Motivation

Why is WW + 1 Jet important ?

Precise understanding important for tests of the SM at high scale, i.e. electro-weak gauge-boson

coupling analysis

● Benchmark process for loop calculations ?

● Important background process

● Large fraction of WW with additional jet activity

No, not enough colored particles to be really difficult…(# diagrams, # divergencies, #exceptional regions,…)

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WW + 1-Jet ― Motivation

● For 155 GeV < mh < 185 GeV, H WW is important channel

● For 130 GeV < mh < 190 GeV, Vector Boson Fusion (VBF) dominates over ggH as far as signal significance is concerned

Higgs search:

[Atlas ‘03]

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WW + 1-Jet ― Motivation

NLO corrections for Higgs production via VBF known:

[Figy, Oleari, Zeppenfeld ‘03, Berger,Campbell ‘04]

Experimental Signature:

Background reactions:

WW + 2 Jets, WW + 1 Jet

If only leptonic decay of W´s and 1 Jet is demanded(improved signal significance)

Two forward tagging jets + “Higgs”

NLO corrections unknown

Top of the Les Houches list ‘07

[Han, Valencia, Willenbrock '92; Spira '98; Djouadi, Spira '00]- Total cross section- Differential distributions

[Mellado, Quayle, Wu, ’05,’07]

QCD uncertainty ~ 4%

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Leading-order results

Basic process:

3 x 4 = 12 different partonic channels

Different quark flavours + crossing

Diagrams for uu:

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Leading-order results

Some features:

● Jet algorithm required to render cross section finite Ellis-Soper-Algorithm, no recombination at LO

● Dependence on 2x2-“CKM” matrix cancels (unitarity)● Significance of individual channels due to PDF’s● “Large” residual scale dependance LHC: 12(30)% for change 2(5)

Tevatron: 25(75)% for change 2(5)

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Methods

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Next-to leading order corrections

Every piece is individually divergent,only in the combination a finite result is obtained

Standard procedure:

Dipole subtraction method

[Frixione,Kunszt,Signer ´95, Catani,Seymour ´96, Nason,Oleari 98, Phaf, Weinzierl, Catani,Dittmaier,Seymour, Trocsanyi ´02]

in all single-unresolved regionsWith:

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Real corrections

Generic amplitudes:

Crossing + non-diagonal 2x2 flavour structure:

136 different channels

Some book keeping required

Sample diagrams:

Two independent computer codes, based on:● Short analytic expressions, using spinor helicity methods● Madgraph [Stelzer, Long ‘94]

Page 11: Peter Uwer *)

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Dipole subtraction method

Universal structure:

Generic form:Leading-order amplitudes

Vector in color space

Color charge operators,induce color correlation

Spin dependent part,induces spin correlation

universal

Example: 10 dipoles required

! !

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Dipole subtraction method — implementation

LO – amplitude, with colour information,

i.e. correlations

List of dipoles we want to calculate

0

1234

5

reduced kinematics,“tilde momenta” + Vij,k

Dipole di

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Dipole subtraction method — implementation

LO – amplitude, with colour information,

i.e. correlations

List of dipoles we want to calculate

0

1234

5

reduced kinematics,“tilde momenta” + Vij,k

Dipole di

Page 14: Peter Uwer *)

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Virtual corrections

Sample diagrams

Again many different channels!

Further decomposition possible:

“bosonic corrections” “fermionic corrections”

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Virtual corrections

Issues:

● Scalar integrals

● How to derive the decomposition

Traditional approach: Passarino-Veltman reduction

Scalar integrals

Large expressions numerical implementation

Numerical stability and speed are important

?

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Reduction of tensor integrals — what we did…

Reduction à la Passarino-Veltman,with special reduction formulae in singular regions,

Five-point tensor integrals:

Four and lower-point tensor integrals:

● Apply 4-dimensional reduction scheme, 5-point tensor

integrals are reduced to 4-point tensor integrals

Based on the fact that in 4 dimension 5-point integrals can be reduced to 4 point integrals

No dangerous Gram determinants!

[Melrose ´65, v. Neerven, Vermaseren ‘84]

[Denner, Dittmaier ‘02]

Two independent computer codes based on:

- Feynarts 1.0 + Mathematica library + Fortran library- Feynarts 3.2 [Hahn ‘00] + FormCalc/LoopTools [Hahn, Perez-Victoria ’98]

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Checks of the NLO calculation

● Leading-order amplitudes checked with Madgraph

● Subtractions checked in singular regions

● Structure of UV singularities checked

● Structure of IR singularities checked

Most important:

● Two complete independent programs for all parts of the calculation, inparticular:

complete numerics done twice !

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Tuned comparison with other groups

Campbell, Ellis, Zanderighi (CEZ), JHEP 0712:056,2007

Binoth, Guillet, Karg, Kauer, Sanguinetti (in progress) (BGKKS)

Stefan Kallweit LL2008

impressive agreement !

Page 19: Peter Uwer *)

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Results

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Results WW+1-Jet –– Tevatron[Dittmaier, Kallweit, Uwer ‘07]

Phys.Rev.Lett.100:062003,2008

…as it should be…

Note: shown results independent from the decay of the W´s

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Results WW + 1-Jet –– LHC[Dittmaier, Kallweit, Uwer ‘07]

Note: shown results independent from the decay of the W´s

Phys.Rev.Lett.100:062003,2008

scale dependence only improved after jet-veto !

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Distributions including decay (LHC)[Campbell, Ellis, Zanderighi, JHEP 0712:056,2007]

LO rescaled by appropriate K-factor

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Conclusions

[Gudrun Heinrich ]

● Our group: Two complete independent calculations

● In addition: perfect agreement with two other groups

● Scale dependence is improved (LHC jet-veto)

● Corrections are important

● NLO has only mild effect on the shape of distributions [CEZ]

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Outlook

● Further improvements possible (and underway…)

(remove redundancy, further tuning, except. momenta,…)

● Distributions

● Include leptonic decay of the W´s

● Apply tools to other processes

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The End


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