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Direct photons for the UHKM package

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Title: Direct photons for the UHKM package


1
Direct photons for the UHKM package
  • Sergey Kiselev, ITEP, Moscow
  • Direct photon news
  • new experimental techniques
  • new physical processes
  • new data
  • Photons for the UHKM package
  • decay ?
  • prompt ?
  • thermal ?
  • hard-thermal ?
  • Conclusions

2
New experimental techniques
  • Last years large progress in experimental
    techniques to extract direct photons
  • Direct photons have been revealed by methods
  • Subtraction, WA98/2000, PHENIX/2005
  • Momentum correlation, WA98/2004
  • Internal conversion, PHENIX/2005, QM05
  • External conversion, PHENIX/2006, QM06
  • Tagging, PHENIX/2006, QM06

3
New physical processes
Photons in AA
Direct Photons
Decay Photons
jet-g-conv.
hard
thermal
hardthermal
Preequilibriumphotons ???
QGP
Hadron gas
direct
fragmentation
Medium inducedg bremsstr.
4
New physical processes - RHIC
PR C69 014903 (2004) S.Turbide et al.
2006 hep-ph/0609301
5
New data RAA
Nucl-ex/0701040
  • RAA seems to be below unity at very high-pT (pT gt
    14 GeV/c)
  • None of the theoretical calculations reproduces
    RAA in the full pT range

First data using pp data as reference!
6
New data v2
Within statistical and systematic errors v2 is
consistent with zero. v20 or cancellation of
different contributions?
S.Turbide, C.Gale, R.J.Fries, PRL 96 032303 (2006)
7
UHKM package
  • Universal Hydro Kinetic Model (UHKM)
    (http//uhkm.jinr.ru). Now includes
  • FASTMC FAST Monte-Carlo hadron freeze-out
    generator. Particles are generated on the
    chemical or thermal freeze-out hyper-surface
    represented by a parameterization or a numerical
    solution of relativistic hydrodynamics.
  • UKM Universal Kinetic Model. Treats further
    evolution (scattering and decays) solving
    relativistic Boltzmann equations numerically.
  • SPHES Smoothed Particle Hydrodynamics
    Equations Solver. Solves (13D) relativistic
    perfect hydrodynamics equations at given initial
    condition and equation of state and provides
    hadron freeze-out hyper-surface.

8
photons for UHKM
  • decay photons trivial (p0, ?, decays)
  • prompt photons (high pT)
  • pp data fit
  • AB binary scaling
  • thermal photons (low pT)
  • thermal rates from QGP/HadronGas have to be
    convoluted over the space-time history of the AB
    reaction given by hydrodynamics
  • hard-thermal (intermediate pT)
  • ? Should think how jet-? conversion,
    jet-bremsstrahlung could be implemented in UHKM.
    L.Malinina plans to implement jets. May be, in
    parallel, one can think on direct photon source.

9
Prompt photons data fit
A Compilation of Data, J. Phys. G, 23 (1997)
A1 Data fit D.Srivastava, Eur.Phys.J, C22 (2001)
129
pp
AB Ed3N/d3p(b)Ed3spp /d3p AB TAB
(b)Ed3spp/d3p Ncoll(b)/sppin
10
Prompt photons RHIC pp data
11
Thermal photons
  • Thermal rates from QGP
  • Perturbative QCD, the lowest order in ?s
  • qq ? g? qg ? q?
  • dN/d4xd3p ? ??s ln(0.23E/?sT) exp(-E/T) T2/E,
    ZP C53, 433
  • bremsstrahlung
  • dN/d4xd3p ? ??s exp(-E/T) T2/E, PL B510, 98
  • Thermal rates from HG
  • effective theory for hadron interactions
  • p? ? p? pp ? ?? ? ? p?
  • dN/d4xd3p ? T2.15 exp(-E/T) / exp((1.35
    ET)0.77), PL B510, 98
  • The thermal rates can be convoluted over the
    space-time history of the AB reaction given by
    SPHES

12
Conclusions
  • Progress in the direct photon sector as in
    experimental methods and theory
  • One can implement photons in the UHKM package
  • - decay photons
  • - prompt photons
  • - thermal photons
  • Should think on the hard-thermal source of photons

13
Back up
14
There are theoretical predictions with a sizable
azimuthal parameter v2
Thermal photons are produced throughout the
expansion history and reflect quark anisotropy
Jets lose more energy where the medium is thicker
- more jet-photon conversions (v2lt0), photons
from fragmentation of quenched jets (v2gt0)
S.Turbide, C.Gale, R.J.Fries, PRL 96 032303 (2006)
R. Chatterjee et al., PRL 96, 202302 (2006)
4
15
How does PHENIX measure direct photons and v2?
  • Measure inclusive photon yield, Ninc
  • Measure hadron contribution components p0 and h
  • By Monte Carlo calculate p0 and h decay
    background in inclusive sample, Nbg
  • Calculate direct photon excess over hadron
    decays, R
  • Measure inclusive and hadron v2 by reaction plane
    method
  • Calculate direct photon v2 as

R v2inc v2BG
v2dir
R 1
Use large statistics Run 4 AuAu data set
R N inc / NBG
See also poster 86 by Kentaro Miki
5
16
In pp Hard photonsdirect component
Annihilation
Compton
In AA picture is much more complicated
Photons in AA
Direct Photons
Decay Photons
Preequilibriumphotons
hard
thermal
hardthermal
QGP
Hadron gas
direct
fragmentation
jet-g-conv.
Medium inducedg bremsstr.
V20
V2gt0
V2gt0
V2gt0
V2lt0
V2lt0
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