direct-photon production in s nn = 200 gev au+au collisions

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Direct-Photon Production in s NN = 200 GeV Au+Au Collisions CIPANP 2006 June 2, 2006 Klaus Reygers University of Münster for the PHENIX collaboration

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Direct-Photon Production in  s NN = 200 GeV Au+Au Collisions. CIPANP 2006 June 2, 2006 Klaus Reygers University of Münster for the PHENIX collaboration. Direct Photons in A+A collisions – Why?. High p T (> 6 GeV/ c ):. Low p T :. - PowerPoint PPT Presentation

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Page 1: Direct-Photon Production in   s NN  = 200 GeV Au+Au Collisions

Direct-Photon Production in sNN = 200 GeV Au+Au Collisions

CIPANP 2006June 2, 2006

Klaus ReygersUniversity of Münster

for the PHENIX collaboration

Page 2: Direct-Photon Production in   s NN  = 200 GeV Au+Au Collisions

2 CIPANP 2006, Klaus Reygers

Direct Photons in A+A collisions – Why?

High-pT direct photons produced in initial hard parton-parton scatterings

Photons leave the subsequently produced medium (quark-gluon plasma !?) unaltered

Test hard scattering predictions

Measure rate of hard processes

Low pT thermal direct photons expected to reflect the initial temperature of the fireball

Temperatures above Tc indicate quark-gluon plasma phase

High pT (> 6 GeV/c): Low pT:

Page 3: Direct-Photon Production in   s NN  = 200 GeV Au+Au Collisions

3 CIPANP 2006, Klaus Reygers

Known and Presumed Photon Sources in A+A

Photons in A+A

Direct Photons Decay Photons

hard

direct fragmentation

These mechanisms are also present in p+p collisions and are calculable within pQCD

Page 4: Direct-Photon Production in   s NN  = 200 GeV Au+Au Collisions

4 CIPANP 2006, Klaus Reygers

Known and Presumed Photon Sources in A+A

Photons in A+A

Direct Photons Decay Photons

hard

direct fragmentation

Compton Annihilation

Hard direct photons:direct component

q + g + q q + q + g

Page 5: Direct-Photon Production in   s NN  = 200 GeV Au+Au Collisions

5 CIPANP 2006, Klaus Reygers

Known and Presumed Photon Sources in A+A

Photons in A+A

Direct Photons Decay Photons

hard

direct fragmentation

Hard direct photons:bremsstrahlung / fragmentation component

Page 6: Direct-Photon Production in   s NN  = 200 GeV Au+Au Collisions

6 CIPANP 2006, Klaus Reygers

Known and Presumed Photon Sources in A+A

Photons in A+A

Direct Photons Decay Photons

hard thermal hard+thermal

QGP Hadron gasdirect fragmentation

Preequilibriumphotons

jet--conv.

Medium induced bremsstr.

Page 7: Direct-Photon Production in   s NN  = 200 GeV Au+Au Collisions

7 CIPANP 2006, Klaus Reygers

Known and Presumed Photon Sources in A+A

Photons in A+A

Direct Photons Decay Photons

hard thermal hard+thermal

QGP Hadron gasdirect fragmentation

Preequilibriumphotons

jet--conv.

Medium induced bremsstr.

Preequillibrium photons Produced through rescattering of the primarily produced partons prior to

thermalization

Difficult to treat theoretically

Page 8: Direct-Photon Production in   s NN  = 200 GeV Au+Au Collisions

8 CIPANP 2006, Klaus Reygers

Known and Presumed Photon Sources in A+A

Photons in A+A

Direct Photons Decay Photons

hard thermal hard+thermal

QGP Hadron gasdirect fragmentation

Preequilibriumphotons

jet--conv.

Medium induced bremsstr.

Thermal photons Reflect temperature of the system, produced over entire evolution

Significant direct photon source only at low pT

Page 9: Direct-Photon Production in   s NN  = 200 GeV Au+Au Collisions

9 CIPANP 2006, Klaus Reygers

Known and Presumed Photon Sources in A+A

Photons in A+A

Direct Photons Decay Photons

hard thermal hard+thermal

QGP Hadron gasdirect fragmentation

Preequilibriumphotons

jet--conv.

Medium induced bremsstr.

Hard+thermal:Jet-Photon-Conversion

hard QGPq + q + g

hard QGPq + g + q Interaction of parton from hard scattering with soft parton

( )3jet- -conv jetp pg gs d -

Page 10: Direct-Photon Production in   s NN  = 200 GeV Au+Au Collisions

10 CIPANP 2006, Klaus Reygers

Known and Presumed Photon Sources in A+A

Photons in A+A

Direct Photons Decay Photons

hard thermal hard+thermal

QGP Hadron gasdirect fragmentation

Preequilibriumphotons

jet--conv.

Medium induced bremsstr.

Medium induced photon bremsstrahlung Due to multiple scattering of quarks in the medium

Different theoretical predictions, likely rather small contribution

Page 11: Direct-Photon Production in   s NN  = 200 GeV Au+Au Collisions

11 CIPANP 2006, Klaus Reygers

Schematic Photon Spectrum in A+A

Hard photons dominant direct photon source for pT > ~ 6 GeV/c

Thermal photons expected to be significant contribution below pT ~ 3 GeV/c

Jet-photon conversion might be significant contribution below pT ~ 6 GeV/c

T

1np

hard:

/ E Tethermal:

Decay photons(0→, →, …)

Page 12: Direct-Photon Production in   s NN  = 200 GeV Au+Au Collisions

12 CIPANP 2006, Klaus Reygers

PHENIX: Photon and Electron Detectors

PbSc: Highly segmented lead

scintillator sampling calorimeter

Module size: 5.5 cm x 5.5 cm x 37 cm

PbGl: Highly segmented lead glass

Cherenkov calorimeter Module size:

4.0 cm x 4.0 cm x 40 cm

Ring Imaging Cherenkov Detector (RICH): Electron identification Insensitive to pions with p < 4.6 GeV/c

Pseudorapidity coverage : || < 0.35

~5 m

Page 13: Direct-Photon Production in   s NN  = 200 GeV Au+Au Collisions

13 CIPANP 2006, Klaus Reygers

Direct-Photon Spectra in Au+Au

TAB p+p pQCD

Phys.Rev.Lett.94:232301,2005

Au+Au at sNN = 200 GeV (RHIC run 2)

High-pT direct photons scale with TAB

Nuclear overlap function TAB

Measures increase of parton luminosity relative to p+p

Calculated with a simple geometrical Glauber model

p+pAB coll inel/T N s=

Page 14: Direct-Photon Production in   s NN  = 200 GeV Au+Au Collisions

14 CIPANP 2006, Klaus Reygers

Hadron Suppression: A Final State Effect!

A+B

AB T p+p

d / d

d / dT

AB

N pR

T ps=

´

Factor 5 suppression

energy lossfor q and g

No energyloss for ‘s

Hadrons are suppressed whereas direct photons are not:Evidence for parton energy loss (as expected in the QGP)

Page 15: Direct-Photon Production in   s NN  = 200 GeV Au+Au Collisions

15 CIPANP 2006, Klaus Reygers

Bremsstrahlung Component

Bremsstrahlung contribution large

Modification of Bremsstrahlung contribution expected in A+A

direct

Bremsstrahlung

calculation by W. Vogelsang

Page 16: Direct-Photon Production in   s NN  = 200 GeV Au+Au Collisions

16 CIPANP 2006, Klaus Reygers

Effect of Parton Energy Loss

20-30% reduction of direct photon RAA expected due to parton energy loss

Consistent with PHENIX data

F. Arleo, hep-ph/0601075

Page 17: Direct-Photon Production in   s NN  = 200 GeV Au+Au Collisions

17 CIPANP 2006, Klaus Reygers

New High-Statistics Data (Run 4)

Run 4: factor ~10 increase in statistics compared to run 2

Direct-photon signal up to pT ~ 13 GeV/c, reduced statistical uncertainties

Consistent with Ncoll-scaled pQCD calculation

p+pcoll pQCD

Au+Aubackground

1N g

g

´+

Calculated basedon measured 0 and spectra

Page 18: Direct-Photon Production in   s NN  = 200 GeV Au+Au Collisions

18 CIPANP 2006, Klaus Reygers

Centrality Dependence

No significant deviation from Ncoll-scaled pQCD for all centralities

Page 19: Direct-Photon Production in   s NN  = 200 GeV Au+Au Collisions

19 CIPANP 2006, Klaus Reygers

Direct Photons from Jet-Medium Interactions?

Model parameters (QGP evolution, parton energy loss) adjusted so as to describe the pion suppression

Bremsstrahlung component reduced due to parton energy loss

Direct photons:Better agreement with data if jet-photon conversion is added

hard QGPq + q + g hard QGPq + g + q

Jet-photon conversion:

Page 20: Direct-Photon Production in   s NN  = 200 GeV Au+Au Collisions

20 CIPANP 2006, Klaus Reygers

Direct Photons via Internal Conversion

Any source of real photons emits virtual photons with small invariant mass

The distribution of the virtual photon mass depends on the emitting source

Phase space at higher inv. masses limited for virtual photons from hadron decays

Signal/background for virtual direct photons significantly improves with increasing mass

Different invariant mass

distribution

Page 21: Direct-Photon Production in   s NN  = 200 GeV Au+Au Collisions

21 CIPANP 2006, Klaus Reygers

Internal Conversion: Kroll-Wada Formula

Virtual photonmass

distributionQED

phase space

form factor

Kroll-Wada formula:

Direct photon internal conversion:→ Described by QED part alone

(as long as pT >> mee)

0 and Dalitz decay:→ QED part dominates

for mee/M → 0→ meson mass limits mee

mee (GeV)

dN

ee/dm

ee (

arb

. u

nit

s)

0

direct

Page 22: Direct-Photon Production in   s NN  = 200 GeV Au+Au Collisions

22 CIPANP 2006, Klaus Reygers

Internal Conversion: Analysis Method

mee (GeV)

dN

ee/dm

ee (

arb

. u

nit

s)

B Adata ee ee/R N N=Measured quantity:

Without direct photons:Kroll-Wada

data hadronR R=

input: /0 ratio

translates into

fraction of virtual direct photons:* Kroll-Wadadirect data hadron

* Kroll-Wada Kroll-Wadaall direct hadron

R R

R Rg

gg

-=

-

Kroll-Wadadata hadronR R>

Direct photon spectrum viainclusive photon spectrumfrom EMCal:

*direct

direct all*all

gg g

g= ×

fromEMCal

signal~ 1

background

Page 23: Direct-Photon Production in   s NN  = 200 GeV Au+Au Collisions

23 CIPANP 2006, Klaus Reygers

Direct Photon Spectrum in Central Au+Au

Direct photon spectrum for 1 < pT < 4.5 GeV via internal conversion

Systematic errors

Small! (~25 %)

Dominated by uncertainty of /0 ratio

A breakthrough!

Agreement with conventional method

Page 24: Direct-Photon Production in   s NN  = 200 GeV Au+Au Collisions

24 CIPANP 2006, Klaus Reygers

Comparison with Scaled pQCD

Contribution of hard processes estimated with scaled pQCD

pQCD uncertainties

Arbitrary scales

Parton distribution function

Parton-to-photon frag. function

Scale uncertainties dominate

Cold nuclear matter effects (“kT broadening”) likely to be negligible

Differentparton-to-photonfrag. function (BFG)

NLO pQCD byWerner Vogelsang

Excess above pQCD possibly due to thermal photons

Page 25: Direct-Photon Production in   s NN  = 200 GeV Au+Au Collisions

25 CIPANP 2006, Klaus Reygers

Comparison with Hydro-Models

Hydro models:QGP and HG photon rates convolved with fireball evolution

Data can be described with pQCD + hydro

Ti,max (MeV) i (fm/c)

Alam et al. 400 0.2

Chaudhuri 400 0.6

d’Enterria, Perresounko

570 0.15

2+1 hydro,d’Enterria, Perresounko

Temperatures above critical temperature Tc for QGP transition

Page 26: Direct-Photon Production in   s NN  = 200 GeV Au+Au Collisions

26 CIPANP 2006, Klaus Reygers

Conclusions

Unlike pions high-pT direct photons are not suppressed (i.e. they follow TAB scaling)

Thus, pion suppression is a final state effect, consistent with parton energy loss in a quark-gluon plasma

Direct Photon measurement via internal conversion

Excess above pQCD possibly due to thermal radiation

Data only described with initial tempartures above Tc

Direct Photons in sNN = 200 GeV Au+Au

High pT (> 6 GeV/c): Low pT:

Page 27: Direct-Photon Production in   s NN  = 200 GeV Au+Au Collisions

27 CIPANP 2006, Klaus Reygers

Backup

Page 28: Direct-Photon Production in   s NN  = 200 GeV Au+Au Collisions

28 CIPANP 2006, Klaus Reygers

Turbide, Gale, Jeon, Moore,Phys. Rev. C 72, 014906 (2005)

Page 29: Direct-Photon Production in   s NN  = 200 GeV Au+Au Collisions

29 CIPANP 2006, Klaus Reygers

Page 30: Direct-Photon Production in   s NN  = 200 GeV Au+Au Collisions

30 CIPANP 2006, Klaus Reygers

Referenz: p+p Daten

Referenz: pQCD

Page 31: Direct-Photon Production in   s NN  = 200 GeV Au+Au Collisions

31 CIPANP 2006, Klaus Reygers

0

0AA T

AA

AA NN Tf

d / d

d / d

N pR

T p

Page 32: Direct-Photon Production in   s NN  = 200 GeV Au+Au Collisions

32 CIPANP 2006, Klaus Reygers

Page 33: Direct-Photon Production in   s NN  = 200 GeV Au+Au Collisions

33 CIPANP 2006, Klaus Reygers

Page 34: Direct-Photon Production in   s NN  = 200 GeV Au+Au Collisions

34 CIPANP 2006, Klaus Reygers

Lines: 1 + Ncoll x Nγ,pQCD/Nγ,bg

(dashed lines: µ=2pT, µ=0.5pT; grey band includes error in Ncoll)

Page 35: Direct-Photon Production in   s NN  = 200 GeV Au+Au Collisions

35 CIPANP 2006, Klaus Reygers

GeV 200s at pp

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

(by W. Vogelsang)

Page 36: Direct-Photon Production in   s NN  = 200 GeV Au+Au Collisions

36 CIPANP 2006, Klaus Reygers

isolation cutno cut

PHENIX Preliminary

includes underlyingevent

NLO pQCD calculationby W. Vogelsang

Page 37: Direct-Photon Production in   s NN  = 200 GeV Au+Au Collisions

37 CIPANP 2006, Klaus Reygers