direct-photon production in phenix oliver zaudtke for the collaboration winter workshop on nuclear...

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Direct-Photon Production in PHENIX Oliver Zaudtke for the Collaboration Winter Workshop on Nuclear Dynamics 2006

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Direct-Photon Production in PHENIX

Oliver Zaudtke

for the CollaborationWinter Workshop on Nuclear Dynamics 2006

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direct photons

What are Direct Photons?

decay photonsinclusive photons = +

Definition:

Photons that emerge directly from a particle collision

challenge: large background from hadronic decays

measured direct-photons in various reaction systems

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PHENIX Data

Data presented in this talk:

Direct Photons in p+pat √s = 200 GeV

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p+ptest of pQCDbaseline for direct photons in A+Aconstrain gluon distribution in proton (gluon contributes at LO)

Why Direct Photons in p+p?

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produced in hard scatterings:rates can be calculated in pQCD

quark-gluon Compton scatteringquark-antiquark annihilationBremsstrahlung

Direct-Photon Production in p+p

fragmentation component

prompt/pQCD photons

q

q

q

q

g

g

g

γγ

direct component

q

qg

γ

q

q g

γ

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Cocktail Methodstart with inclusive photons

subtract photons from hadronic decays

main contribution from0 decays (0 → )spectrum of decay photons can be simulated

signal/background ratio very small

Analysis Techniques (I)

0 → (80 %)

→ → 0

’ → X

sum

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Results in p+p (I)GeV 200s at pp

PbGlPbScNLO pQCD CTEQ6M PDF µ=pT/2, pT, 2pT

(by W. Vogelsang)

two independent analyses

different detectors

measured spectra agree with each other

good agreement with NLO pQCD

important baseline for Au+Au measuement

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What fraction of direct photons is isolated?

Analysis Techniques (II)

Isolation Method q

qg

γ

q

q g

γ

isolatedphotons

Compton

Annihilation

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What fraction of direct photons is isolated?

isolation cut should remove Bremsstrahlung

difficult to estimate efficiency of isolation cut:

underlying event (soft physics)limited acceptance

Analysis Techniques (II)

Isolation Method

Jet

q

q

q

q

g

g

g

γγBremsstrahlung

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Results in p+p (II)isolation of direct photons:

direct photon sample with cocktail method

effect on 0 decay photons

data is better described by pQCD + underlying event

isolation cutno cut

PHENIX Preliminary

includes underlyingevent

NLO pQCD calculationby W. Vogelsang

Direct Photons in d+Au at √s = 200 GeV

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d+Austudy cold nuclear matter effects

kT broadening (Cronin)

nuclear shadowing

p+ptest of pQCDbaseline for direct photons in A+Aconstrain gluon distribution in proton (gluon contributes at LO)

Why Direct Photons in d+Au?

done

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Results in d+Au

no indication of cold nuclearmatter effects (RdA ≈ 1)

in good agreement with binary scaled pQCD

Direct Photons in Au+Au at √s = 200 GeV

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d+Austudy cold nuclear matter effects

kT broadening (Cronin)

nuclear shadowing

Au+Auphotons do not interact strongly with mediumhard photons

test of binary scaling(Ncoll scaling)

understand high-pT hadron suppression

thermal photonsconstrain temperature of the collision systemQGP signature

Why Direct Photons in Au+Au?

done

p+ptest of pQCDbaseline for direct photons in A+Aconstrain gluon distribution in proton (gluon contributes at LO)

done

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Hard-Scattering in Au+Audirect photons produced in early hard scatterings at high-pT

signal should scale with number of binary collisions

PRL 94, 232301 (2005)

binary scaling holds for all centralities

0 suppression caused by parton energy loss in the medium

PRLnuclear modification factor

(Run 2)

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Contribution of Bremsstrahlung

maybe it is not that simple:is Bremsstrahlung production modified by medium?

calculation by W. Vogelsang

direct

Bremsstrahlung

large contributionfrom Bremsstrahlung

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dir

ect

photo

n R

AA

Jeon, Jalilian-Marian, Sarcevic,Nucl. Phys. A 715, 795 (2003)Zakharov, hep-ph/0405101

Modification of Bremsstrahlung?

is Bremsstrahlung suppressed by parton energy loss in the medium (induced gluon radiation)?

enhancement of direct-photon production via medium induced Bremsstrahlung?

possible net effect: RAA ≈ 1

issue not solved yet!

Thermal Photons in Au+Au

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Decay photons

Photon Spectrum in Au+Au

hot and dense medium inthermal equilibrium

nT

1

phard:

/ E Tethermal:

schematic view

Compton

Annihilation

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Realistic Calculation

thermal photons from QGP dominant source in pT range ≈1-3 GeV/c

potential signature for QGP

Turbide, Rapp, Gale, Phys. Rev. C 69 (014902), 2004

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Thermal Signal?published spectrum

new data set (Run4)

no significant excess at low pT with conventional methods

PRL 94, 232301 (2005)(Run 2)

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Internal Conversion (I)

direct photons via internal conversion

any source of real photons can emit virtual photons with very low mass (e.g. 0 Dalitz)virtual photons can subsequently decay into e+e- pairs

same is true for direct-photon production

A New Approach:

0

e+

e-

q

g q

e+

e-

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Internal Conversion (II)

mass distribution of Dalitz pairs is given by Kroll-Wada Formula

QED phasespace

formfactor

at very low mass (mee ≈ 0) mass distribution process independent (only governed by QED part)

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Internal Conversion (III)

direct photons:hadronic form factor becomes unityno phase space limitation for photons in chosen mass range

90-300 MeV

0-3

0

0 Dalitz pairs highly suppressedin this mass range

S/B ≈ 1

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The Method

Measure ratio:

Calculate:

0-3

0 90-300 MeV

÷

from Kroll-Wada formula

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The Method

Measure ratio:

Calculate:

0-3

0 90-300 MeV

÷measured with EMCal

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Comparison to Conventional Result

significant signal belowpT = 3 GeV/c

systematic errors:~20% measured /0

~10% inclusive photons~5% acceptance

~25 % total systematic error

(+1)

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The Direct-Photon Spectrum

NLO pQCD

Thermal Model2+1 hydroT0

ave=360 MeV(T0max=570

MeV)0=0.15 fm/c

The data are consistent with thermal + pQCD(only one possible interpretation!)

Phys. Rev. D48, 3136 (1993)L.E. Gordon, W. Vogelsang

nucl-th/0503054

D. d’Enterria, D. Perresounko

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Signal of thermal origin?analysis of p+p and d+Au using the same technique is needed

if excess in Au+Au is of thermal origin the reference will show a much smaller effect

The Direct-Photon Spectrum

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p+pdirect photons show good agreement with NLO pQCDisolated signal better described by pQCD + underlying event

d+Augood agreement with scaled NLO pQCDno indication of cold nuclear matter effects

Au+Auhard scattering contribution (pT>4 GeV/c) follows binary scaling for all centralitiessignificant signal obtained at low pT (<4 GeV/c) using internal conversion

spectrum agrees with NLO pQCD + thermal model

Summary

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Backup

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The PHENIX Experiment I

photon measurement:EMCal (PbGl, PbSc)

electron measurement:Tracking, RICH, EMCal

~5 m

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Tagging Method

increase signal/background ratio by tagging 0 photonsstart with sample of direct photon candidates

tagging efficiency determind in Monte-Carlo

Analysis Techniques (II)

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more peripheral

Centrality dependence

indication for centrality dependence