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Direct-Photon Production from SPS to RHIC Energies

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Quark-Gluon Compton scattering contributes at leading order (LO) ... Two photon correlations observed and attributed to Bose-Einstein correlations of direct photons ... – PowerPoint PPT presentation

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Title: Direct-Photon Production from SPS to RHIC Energies


1
Direct-Photon Production from SPS to RHIC
Energies
  • Klaus ReygersUniversity of Münsterfor the
    PHENIX Collaboration

2
Why Direct Photons? (I)
  • Direct Photons
  • Pragmatic DefinitionPhotons not coming from
    hadron decays
  • Difficult measurementLarge Background from
  • pp
  • Late 1970sDirect Photons suggested presence of
    pointlike charged objects within hadrons
  • Test of QCD
  • Focus now on constraining gluon distribution
    functions
  • Quark-Gluon Compton scattering contributes at
    leading order (LO)
  • This is in contrast to Deep Inelastic Scattering
    and Drell-Yan where gluon is involved only at NLO

3
Why Direct Photons? (II)
  • NucleusNucleus collisions
  • Photons dont interact with the fireball and
    carry information about early stage of the AA
    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
Direct Photon Production in pp Hard Scattering
  • Processes in pertubative QCD
  • Compton
  • Annihilation
  • Bremsstrahlung
  • Typically 20-30 uncertainty in pQCD calculations
    related to choice of scales

5
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
6
Photon Sources in AA
Photons in AA
Direct Photons
Decay Photons
7
Schematic Photon Spectrum in AA
  • Advantage in central AA at RHICDecay photon
    background strongly reduced due to to p0
    suppression

8
Realistic Calculation
Turbide, Rapp, Gale, Phys. Rev. C 69 (014902),
2004
  • Window for thermal photons from QGP in this
    calculationpT 1 - 3 GeV/c

9
Thermal Photons as QGP Signature
  • Conventional wisdom ca 1985
  • QGP has lots of quarks flying around
  • QGP radiates more than HG at the same temperature
    (false!)
  • Lots of thermal radiation is evidence for QGP
  • Current conventional wisdom
  • QGP has more d.o.f. than HG and therefore lower
    temperature at the same energy density e (e
    g?T4)
  • At the same energy density QGP radiates less then
    HG
  • Lack of radiation is evidence for QGP!

See talk by P. Stankus at CTEQ summer school
2004 http//www.cteq.org
10
Thermal Photon Rates in QGP
  • Final thermal photon spectrumQGP and HG photon
    rates convoluted with space-time evolution of the
    reaction
  • Thermal photon rate in QGP
  • Hard-thermal-loop resummation
  • Effective in-medium Quark and Gluon propagators
  • Processes
  • Quark-Gluon-Compton scattering
  • Quark-antiquark annihilation
  • Annihilation with Scattering (AWS)
  • Bremsstrahlung

T 250 MeV
2 ? 2
State-of-the-art result from Arnold, Moore, and
Yaffe (including Landau-Pomeranchuk-Migdaldestruc
tive interference effect)
11
Photon Rates in HG and QGP
  • Typical processes for direct photon production in
    hot hadron gas (HHG)
  • Hadron gas at T200 MeV radiates more than QGP at
    the same temperature

Steffen and Thoma, Phys. Lett. B 510, 98 (2001)
12
Measurement of Direct Photons
  • Measure pT spectrum of p0 and h mesons with high
    accuracy
  • Calculate number of decay photon per p0
  • Usually with Monte-Carlo
  • mT scaling for (h), h, w,
  • Get clean inclusive photon sample
  • Charged background subtraction
  • FinallySubtract decay background from inclusive
    photon spectrum

Handy formula
13
Why this is Difficult
Signal !
14
WA98 Result
  • 20 direct photon excess at high pT in central
    PbPb collisions at CERN SPS
  • No signal within errors in peripheral collisions

15
WA98 Direct Photon Spectrum
16
WA98 Interpretation I pQCD with Nuclear 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)
17
WA98 Interpretation II T or kT ?
  • QGP HG rates convoluted with simple fireball
    model plus pQCD hard photons
  • Data described with initial temperate Ti205 MeV
    some nuclear kT broadening (Cronin -effect)
  • Data also described without kT broadening but
    with high initial temperature (Ti270 MeV)
  • Other Models (see e.g. Huovinen et al., Nucl.
    Phys. A 650 (227) 1999) explain data without
    assuming QGP

Turbide, Rapp, Gale, Phys. Rev. C 69 (014902),
2004
18
WA98 New low-pT Points
  • Two photon correlations observed and attributed
    to Bose-Einstein correlations of direct photons
  • Correlation strength used to extract direct
    photon signal at low pT
  • New points not described by current models

WA98, Phys. Rev. Lett. 93 (022301), 2004
19
Direct Photons at RHIC pp
  • Data show good agreement with NLO pQCD
    calculation
  • Important baseline for interpretation of AuAu
    results

20
Direct Photons at RHIC AuAu
  • Strong direct photon signal in central AuAu
  • Direct Photons at high pT follow Ncoll scaling
  • Errors currently too large for statement about
    thermal photon signal

21
Centrality Dependence
PHENIX preliminary
  • Ncoll scaling holds for all centrality classes
    (within errors)

22
Beyond simple Ncoll ScalingkT Effects and
Photons from Quark-Jets
23
What about Photon Bremsstrahlung in AA ?
calculation by W. Vogelsang
direct
Bremsstrahlung
  • Bremsstrahlung contribution large
  • Modification of Bremsstrahlung contribution
    expected in AA

24
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

25
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
  • However, it seems natural to avoid model
    assumptions and to use high pT direct photons as
    a direct measure of the number of hard
    scatterings in AA
  • Define
  • If direct photons exactly follow Ncoll scaling
    then

26
gdirect / p0
Blue points are anotherrepresentation of the
PHENIX preliminary double ratio
(PHENIX preliminary)
27
GAA in central AuAu at RHIC
  • GAA agrees well with the standard RAA
    representation of the neutral pion suppression

28
GAA at CERN SPS
WA98 data
  • GAA consistent with 1 at high pT (pT gt3 GeV/c)
  • Moderate p0 suppression also consistent with data

29
Summary
  • PbPb at CERN SPSDirect photon signal
    consistent with QGP scenario, however, models
    without QGP are also able to explain the data
  • AuAu at RHICDirect photon signal observed at
    high pT confirms Ncoll scaling for hard
    processes and supports explanation of pion
    suppression as final state effect

30
Backup Slides
31
RAA for Different Energies
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