Title: Direct photons for the UHKM package
1Direct 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
2New 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
3New physical processes
Photons in AA
Direct Photons
Decay Photons
jet-g-conv.
hard
thermal
hardthermal
Preequilibriumphotons ???
QGP
Hadron gas
direct
fragmentation
Medium inducedg bremsstr.
4New physical processes - RHIC
PR C69 014903 (2004) S.Turbide et al.
2006 hep-ph/0609301
5New 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!
6New 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)
7UHKM 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.
8photons 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.
9Prompt 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
10Prompt photons RHIC pp data
11Thermal 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
12Conclusions
- 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
13Back up
14There 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
15How 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
16In 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