introduction / motivation photon identification results inclusive prompt photons

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Prompt Photon Production at HERA Prompt Photon Production at HERA and LEP and LEP ICHEP 2004, Beijing Thomas Kluge, DESY on behalf of the H1, OPAL and ZEUS Collaborations Introduction / Introduction / Motivation Motivation Photon Identification Photon Identification Results Results Inclusive Prompt Photons Inclusive Prompt Photons Prompt Photons together Prompt Photons together with a Jet with a Jet Conclusion / Summary Conclusion / Summary “Test QCD by measuring photons” prompt photon

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Prompt Photon Production at HERA and LEP ICHEP 2004, Beijing Thomas Kluge, DESY on behalf of the H1, OPAL and ZEUS Collaborations. Introduction / Motivation Photon Identification Results Inclusive Prompt Photons Prompt Photons together with a Jet Conclusion / Summary. prompt photon. - PowerPoint PPT Presentation

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Page 1: Introduction / Motivation  Photon Identification  Results   Inclusive Prompt Photons

Prompt Photon Production at HERA and LEPPrompt Photon Production at HERA and LEPICHEP 2004, Beijing

Thomas Kluge, DESYon behalf of the H1, OPAL and ZEUS Collaborations

Prompt Photon Production at HERA and LEPPrompt Photon Production at HERA and LEPICHEP 2004, Beijing

Thomas Kluge, DESYon behalf of the H1, OPAL and ZEUS Collaborations

• Introduction / MotivationIntroduction / Motivation• Photon IdentificationPhoton Identification• Results Results

– Inclusive Prompt PhotonsInclusive Prompt Photons– Prompt Photons together with a JetPrompt Photons together with a Jet

• Conclusion / SummaryConclusion / Summary

• Introduction / MotivationIntroduction / Motivation• Photon IdentificationPhoton Identification• Results Results

– Inclusive Prompt PhotonsInclusive Prompt Photons– Prompt Photons together with a JetPrompt Photons together with a Jet

• Conclusion / SummaryConclusion / Summary

“Test QCD by measuring photons”“Test QCD by measuring photons”

prompt photonprompt photon

Page 2: Introduction / Motivation  Photon Identification  Results   Inclusive Prompt Photons

ICHEP04 Th.Kluge: Prompt Photon Production at HERA 2

Prompt Photons and QCDPrompt Photons and QCD

soft QCD

parametrised in p.d.f.

hard QCD

matrix elements up to NLO in s

soft QCD

hadronisation models

An example (HERA)

e

p

q

prompt photonprompt photon

Prompt photon: small hadronisation uncertainty, good energy measurement!

Two signatures are investigated1) isolated photon (inclusive)2) isolated photon + at least one jet (ET > 3-5 GeV)

Prompt photon: small hadronisation uncertainty, good energy measurement!

Two signatures are investigated1) isolated photon (inclusive)2) isolated photon + at least one jet (ET > 3-5 GeV)

Page 3: Introduction / Motivation  Photon Identification  Results   Inclusive Prompt Photons

ICHEP04 Th.Kluge: Prompt Photon Production at HERA 3

Production of Prompt PhotonsProduction of Prompt Photons

marks a remnant, made of low pT particles

direct/single resolved (resolved/double resolved) both present in data …there are more (higher order) diagrams

marks a remnant, made of low pT particles

direct/single resolved (resolved/double resolved) both present in data …there are more (higher order) diagrams

e

e

q

e

e

q

photon photon collisions at LEPphoton photon collisions at LEPelectron proton collisions at HERAelectron proton collisions at HERA

e

p

q

e

p

q

resolved photoproduction

direct photoproduction & deep inelastic scattering single resolved process

double resolved process

Page 4: Introduction / Motivation  Photon Identification  Results   Inclusive Prompt Photons

ICHEP04 Th.Kluge: Prompt Photon Production at HERA 4

Some details on photon identification….Some details on photon identification….

1.1. Basic Basic selection: electromagnetic cluster, with selection: electromagnetic cluster, with no associated trackno associated trackProblem: large background of Problem: large background of 00->-> and and --

>>

2.2. Require isolation cone: veto energy nearby the Require isolation cone: veto energy nearby the photon candidate photon candidate Problem: sensitive to energy deposits from Problem: sensitive to energy deposits from

multiple interactions (m.i.)multiple interactions (m.i.)

3.3. Perform a shower shape analysis: single Perform a shower shape analysis: single photons are more compactphotons are more compact-> Fit signal/background ratio for any result bin -> Fit signal/background ratio for any result bin

(independent of MC background rate!)(independent of MC background rate!)

1.1. Basic Basic selection: electromagnetic cluster, with selection: electromagnetic cluster, with no associated trackno associated trackProblem: large background of Problem: large background of 00->-> and and --

>>

2.2. Require isolation cone: veto energy nearby the Require isolation cone: veto energy nearby the photon candidate photon candidate Problem: sensitive to energy deposits from Problem: sensitive to energy deposits from

multiple interactions (m.i.)multiple interactions (m.i.)

3.3. Perform a shower shape analysis: single Perform a shower shape analysis: single photons are more compactphotons are more compact-> Fit signal/background ratio for any result bin -> Fit signal/background ratio for any result bin

(independent of MC background rate!)(independent of MC background rate!)

Page 5: Introduction / Motivation  Photon Identification  Results   Inclusive Prompt Photons

ICHEP04 Th.Kluge: Prompt Photon Production at HERA 5

Inclusive Prompt Photons in ep Photoproduction (HERA)Inclusive Prompt Photons in ep Photoproduction (HERA)

H1 and ZEUS data consistent within errors MC: shape OK but normalisation low by ~40-50%

: direct exchanged makes up less than ½ of the cross section Multiple interactions spoil isolation cut -> reduced cross section

H1 and ZEUS data consistent within errors MC: shape OK but normalisation low by ~40-50%

: direct exchanged makes up less than ½ of the cross section Multiple interactions spoil isolation cut -> reduced cross section

Comparison with PYTHIA and HERWIG event generators

Comparison with PYTHIA and HERWIG event generators

142 < W < 266 GeV

Q2 < 1GeV2

ℒint = 105 pb-1

142 < W < 266 GeV

Q2 < 1GeV2

ℒint = 105 pb-1

Page 6: Introduction / Motivation  Photon Identification  Results   Inclusive Prompt Photons

ICHEP04 Th.Kluge: Prompt Photon Production at HERA 6

Inclusive Prompt Photons in ep Photoproduction (HERA)Inclusive Prompt Photons in ep Photoproduction (HERA)

Reasonable description by NLO calculations on parton level After corrections for hadronisation and multiple interactions:

normalisation 30-40% below the data

Reasonable description by NLO calculations on parton level After corrections for hadronisation and multiple interactions:

normalisation 30-40% below the data

Comparison with NLO pQCD:

Fontanaz, Guillet, Heinrich (FGH)

Krawczyk, Zembruski(K&Z)

Comparison with NLO pQCD:

Fontanaz, Guillet, Heinrich (FGH)

Krawczyk, Zembruski(K&Z)

142 < W < 266 GeV

Q2 < 1GeV2

ℒint = 105 pb-1

142 < W < 266 GeV

Q2 < 1GeV2

ℒint = 105 pb-1

Page 7: Introduction / Motivation  Photon Identification  Results   Inclusive Prompt Photons

ICHEP04 Th.Kluge: Prompt Photon Production at HERA 7

Inclusive Prompt Photons in Photon-Photon Collisions (LEP)Inclusive Prompt Photons in Photon-Photon Collisions (LEP)

PYTHIA: shape OK but normalisation low by ~50% NLO calculation on parton level gives good description of the data

Variation from photon p.d.f. small compared to experimental uncertainty

PYTHIA: shape OK but normalisation low by ~50% NLO calculation on parton level gives good description of the data

Variation from photon p.d.f. small compared to experimental uncertainty

Comparison with PYTHIA and NLO pQCD (Fontannaz et al)

Comparison with PYTHIA and NLO pQCD (Fontannaz et al)

<see>2 = (197 GeV)2

Q2 < 10 GeV2

ℒint = 649 pb-1

<see>2 = (197 GeV)2

Q2 < 10 GeV2

ℒint = 649 pb-1

Page 8: Introduction / Motivation  Photon Identification  Results   Inclusive Prompt Photons

ICHEP04 Th.Kluge: Prompt Photon Production at HERA 8

Inclusive Prompt Photons in ep Deep Inelastic Scattering (HERA)Inclusive Prompt Photons in ep Deep Inelastic Scattering (HERA)

MC lower than data by factors 2 (PYTHIA) and 8 (HERWIG) Shape of Et well described, PYTHIA gives a poor description of

pseudorapidity

The MCs do not include wide-angle QED bremsstrahlung

MC lower than data by factors 2 (PYTHIA) and 8 (HERWIG) Shape of Et well described, PYTHIA gives a poor description of

pseudorapidity

The MCs do not include wide-angle QED bremsstrahlung

Comparison with PYTHIA and HERWIG event generators

Comparison with PYTHIA and HERWIG event generators

Q2>35GeV2

ℒint=121pb-1

Q2>35GeV2

ℒint=121pb-1

(x2.3)

(x7.9)

(x2.3)

(x7.9)

Page 9: Introduction / Motivation  Photon Identification  Results   Inclusive Prompt Photons

ICHEP04 Th.Kluge: Prompt Photon Production at HERA 9

Jet + Prompt Photon: a handle to direct and resolved reactionsJet + Prompt Photon: a handle to direct and resolved reactions

x: Fractional part of the incoming photon energy, taking part in interaction Definitions are infrared safe for x -> 1 Jet Et does not enter the definition (but hadronic final state does via y )

x: Fractional part of the incoming photon energy, taking part in interaction Definitions are infrared safe for x -> 1 Jet Et does not enter the definition (but hadronic final state does via y )

pp

jetjet

prompt photonprompt photon

electronelectron

protonproton

p

e

q

eyEx 2

eyE2

eE

HERA

Page 10: Introduction / Motivation  Photon Identification  Results   Inclusive Prompt Photons

ICHEP04 Th.Kluge: Prompt Photon Production at HERA 10

Jet + Prompt Photon in ep Deep Inelastic Scattering (HERA)Jet + Prompt Photon in ep Deep Inelastic Scattering (HERA)

NLO calculation on parton level: normalisation reasonable poor description at low Et and in the more forward (proton beam) direction

PYTHIA and HERWIG still by factors 2-4 too low (not shown)

NLO calculation on parton level: normalisation reasonable poor description at low Et and in the more forward (proton beam) direction

PYTHIA and HERWIG still by factors 2-4 too low (not shown)

Comparison with calculation to O(3s

1) (Kramer, Spiesberger)

Comparison with calculation to O(3s

1) (Kramer, Spiesberger)

Q2 > 35 GeV2

ℒint = 121 pb-1

Q2 > 35 GeV2

ℒint = 121 pb-1

Page 11: Introduction / Motivation  Photon Identification  Results   Inclusive Prompt Photons

ICHEP04 Th.Kluge: Prompt Photon Production at HERA 11

Jet + Prompt Photon in ep Photoproduction (HERA)Jet + Prompt Photon in ep Photoproduction (HERA)

Reasonable description of the data by both NLO calculation on parton level

If a jet is required: slightly better description, NLO/LO correction more moderate

Corrections for hadronisation and multiple interactions, taken from PYTHIA, do not improve the description

Reasonable description of the data by both NLO calculation on parton level

If a jet is required: slightly better description, NLO/LO correction more moderate

Corrections for hadronisation and multiple interactions, taken from PYTHIA, do not improve the description

Comparison with NLO pQCD:

Fonatanaz, Guillet, Heinrich (FGH)

Krawczyk, Zembruski (K&Z)

Comparison with NLO pQCD:

Fonatanaz, Guillet, Heinrich (FGH)

Krawczyk, Zembruski (K&Z)

Q2 < 1GeV2

ℒint = 105 pb-1

Q2 < 1GeV2

ℒint = 105 pb-1

Page 12: Introduction / Motivation  Photon Identification  Results   Inclusive Prompt Photons

ICHEP04 Th.Kluge: Prompt Photon Production at HERA 12

Jet + Prompt Photon in ep Photoproduction and Photon-Photon Collisions Jet + Prompt Photon in ep Photoproduction and Photon-Photon Collisions

Shape of the distributions different for HERA and LEP Both: NLO consistent with the data multiple interactions more important at low x (resolved photon)

Shape of the distributions different for HERA and LEP Both: NLO consistent with the data multiple interactions more important at low x (resolved photon)

Photon structure enters at lower x≲0.85 (resolved contribution)

Photon structure enters at lower x≲0.85 (resolved contribution)

Page 13: Introduction / Motivation  Photon Identification  Results   Inclusive Prompt Photons

ICHEP04 Th.Kluge: Prompt Photon Production at HERA 13

Prompt photons: study pQCD and p.d.f. of proton and photon

Alternative to jets: no hadronisation of the photon, good energy measurement small cross section, elaborate photon identification

Consistent findings for p,DIS (HERA) and (LEP)

– MC generators PYTHIA, HERWIG: always undershoot the data, shape in general OK

– NLO QCD calculations on parton level are in reasonable agreement with the data

– If multiple interactions and hadronisation are taken into account, the NLO calculations somewhat undershoot the data (H1)

Why are the predictions low? Higher orders? Non-perturbative effects?

Possible improvements of data analyses: extend phasespace, use more data (HERA II), refine 0 supression/subtraction

Prompt photons: study pQCD and p.d.f. of proton and photon

Alternative to jets: no hadronisation of the photon, good energy measurement small cross section, elaborate photon identification

Consistent findings for p,DIS (HERA) and (LEP)

– MC generators PYTHIA, HERWIG: always undershoot the data, shape in general OK

– NLO QCD calculations on parton level are in reasonable agreement with the data

– If multiple interactions and hadronisation are taken into account, the NLO calculations somewhat undershoot the data (H1)

Why are the predictions low? Higher orders? Non-perturbative effects?

Possible improvements of data analyses: extend phasespace, use more data (HERA II), refine 0 supression/subtraction

SummarySummary