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Direct Photons in PHENIX

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Stefan Bathe (UCR) for the PHENIX collaboration. ICPAQGP-2005, Kolkata, India ... Stefan Bathe. 16. GAA in central Au Au at RHIC ... – PowerPoint PPT presentation

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Title: Direct Photons in PHENIX


1
Direct Photons in PHENIX
  • Stefan Bathe (UCR)
  • for the PHENIX collaboration

ICPAQGP-2005, Kolkata, India February 8-12, 2005
2
Why Direct Photons? (I)
  • Direct Photons
  • Pragmatic DefinitionPhotons not coming from
    hadron decays
  • Difficult measurementLarge background from
  • pp
  • Test of QCD
  • Reduce uncertainty on pQCD photons in AA
  • Future
  • Constraining gluon distribution functions
  • In polarized pp also gluon spin structure
    function

3
Why Direct Photons? (II)
  • AA collisions
  • Photons dont strongly interact with fireball
  • Carry information about early stage of collision
  • QGP potentially detectable via thermal photon
    radiation
  • Thermal photons dominantly from early, hot QGP
    phase? initial temperature
  • Direct Photons at high pT
  • Allow test of Ncoll scaling for hard processes
  • Important for interpretation of high-pT hadron
    suppression at RHIC

4
Photon Sources in AA
Photons in AA
Direct Photons
Decay Photons
5
Schematic Photon Spectrum in AA
  • Advantage in central AA at RHICDecay photon
    background strongly reduced due to p0 suppression

6
Realistic Calculation
Turbide, Rapp, Gale, Phys. Rev. C 69 (014903),
2004
  • Window for thermal photons from QGP in this
    calculationpT 1 - 3 GeV/c

7
PHENIX Experimental Setup
  • Central spectrometer arms h lt 0.35
  • g, p0 via p0 ? gg
  • Electromagnetic calorimeter (EMCal)
  • Lead scintillator calorimeter (PbSc)
  • Lead glass calorimeter (PbGl)

8
Measurement of Direct Photons
  • Get clean inclusive-photon sample
  • e.g. subtraction of charged particle background
  • Measure pT spectrum of p0 and h mesons with high
    accuracy
  • Calculate number of decay photons per p0
  • Usually with Monte-Carlo
  • mT scaling for h, w,
  • FinallySubtract decay background from inclusive
    photon spectrum

Handy formula
9
Cancellation of Systematic Errors
10
Direct Photons in pp PHENIX Result
  • Data show good agreement with NLO pQCD
    calculation
  • Important baseline for interpretation of AuAu
    results

11
Influence of Isolation Cut
  • No correction for direct photon loss due to
    isolation cut
  • Nevertheless, no difference between cross
    sections with and without isolation cut
  • Suggests small contribution of fragmentation
    photons, which would be found within jets

12
Direct Photons in AuAu at RHIC
final results shown in public for the first time
about to be published
  • Direct Photons at high pT follow Ncoll scaling?
    p0 suppression caused by medium created in AA
    collisions

13
Direct Photon Spectra
  • Ncoll scaling holds for all centrality classes
    (within errors)
  • Errors currently too large for statement about
    thermal photon signal

14
Comparing to p0s
  • p0s suppressed going to central collisions
  • Direct photons consistent with Ncoll scaling
  • p0 suppression caused by medium created in AA
    collisions

15
Model-independent Representation of p0
Suppression
  • Standard representation relies on assumption
    about scaling of hard scattering processes in
    AA
  • PHENIX result on high pT direct photon production
    confirms this assumption
  • Better Avoid model assumptions and use high pT
    direct photons as direct measure of number of
    hard scatterings in AA
  • Define
  • If direct photons exactly follow Ncoll scaling,
    then

Klaus Reygers
16
GAA in central AuAu at RHIC
PHENIX Preliminary data used
  • GAA agrees well with the standard RAA
    representation of the neutral pion suppression

17
Conclusions
  • pp
  • Spectrum consistent with pQCD calculations
  • AuAu
  • For the first time spectrum observed at high pT
  • confirms Ncoll scaling for hard processes
  • supports explanation of pion suppression as final
    state effect
  • no thermal photon signal yet

18
Backup Slides
19
Thermal Photons as QGP Signature
  • Conventional wisdom 1985
  • QGP has lots of free quarks
  • QGP radiates more than HG at same temperature
    (false!)
  • Lots of thermal radiation evidence for QGP
  • Conventional wisdom 2005
  • QGP has more d.o.f. than HG and therefore lower
    temperature at same energy density e (e g?T4)
  • At same energy density QGP radiates less than HG
  • Comparing HG and QGP scenariosLack of radiation
    is evidence for QGP!

20
Direct Photons at SPS WA98 Result
  • 20 direct photon excess at high pT in central
    PbPb collisions at CERN SPS
  • No signal within errors in peripheral collisions

Phys.Rev.Lett.853595-3599,2000
21
WA98 Result Just Hard Scattering and kT
Broadening?
  • High pT part of the spectrum explained by pQCD
    nuclear kT broadening
  • pp
  • AA
  • Intermediate pT range cannot be explained
    regardless of amount of kT

Dumitru et al., Phys. Rev. C 64, 054909 (2001)
22
WA98 Interpretation T or kT ?
  • QGP HG rates convoluted with simple fireball
    model plus pQCD hard photons
  • Data described with initial temperature Ti205
    MeV some nuclear kT broadening (Cronin-effect)
  • Data also described without kT broadening but
    with high initial temperature (Ti270 MeV)

Turbide, Rapp, Gale, Phys. Rev. C 69 (014902),
2004
23
What have we learned from SPS?
  • Evidence for thermal photons
  • Consistent with QGP scenario
  • But
  • Temperature and kT competing contributions
  • Pure hadronic scenario cannot be ruled out

24
Direct Photons in pp Tagging Method
  • Photon hits that form an invariant mass in the p0
    or h mass range are rejected as direct photon
    candidates
  • Signal/background ratio increased in low
    multiplicity environment
  • Accidental loss of genuine direct photons
    corrected for by embedding fake photon hits into
    real events
  • Remaining background of decay photons subtracted
    on statistical basis
  • No isolation cut

25
Beyond simple Ncoll ScalingkT Effects and
Photons from Quark-Jets
  • Effect of kT strongest where thermal QGP photons
    are expected
  • Interaction of fast quarks with QGP significant
    photon source for pT lt 6 GeV/c (Jet-Photons
    and
    )

26
Direct Photon Production in pp Hard Scattering
  • Processes in perturbative QCD
  • Compton
  • Annihilation
  • Bremsstrahlung
  • Typically 20-30 uncertainty in pQCD calculations
    related to choice of scales

27
Evidence for kT Broadening
  • Systematic pattern of deviation between NLO pQCD
    and data
  • Data above pQCD
  • Especially at low vs
  • Possible explanation kT broadening (which can
    be produced by multiple soft-gluon emission)

E706, hep-ex/0407011
28
Closer Look at Jet-Photon Prediction
  • Jet photons dominate below 7 GeV
  • pQCD calculation just LO
  • Compensated by k factor
  • Still underpredicts data by factor 2
  • Compare
  • NLO pQCD describes data in central and peripheral
  • No hot medium in peripheral
  • No room for jet photons?

Evidence for Direct Photons from Jet-Plasma
Interaction?
  • Possible observable consequence Negative v2 for
    direct photons
  • No answer with current uncertainties

29
What about Photon Bremsstrahlung in AA ?
calculation by W. Vogelsang
direct
Bremsstrahlung
  • Bremsstrahlung contribution large
  • Modification of Bremsstrahlung contribution
    expected in AA

30
Modification of Bremsstrahlung Contribution in AA
Jeon, Jalilian-Marian, Sarcevic,Nucl. Phys. A
715, 795 (2003)
  • Quark energy loss in QGP reduces bremsstrahlung
    contribution in AA
  • However, this is compensated by induced photon
    bremsstrahlung in QGP(according to Zakharov)
  • Net result direct photon RAA ? 1 at high pT
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