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28.05.08ITEP meeting S.Kiselev1 Fast generators of direct photons Sergey Kiselev, ITEP, Moscow Introduction Definitions SPS and RHIC data New processes Prompt photons Thermal photons in 1+1 hydrodynamics Hot Hadron Gas (HHG) scenario Qurk Gluon Plasma (QGP) scenario To do
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Introduction 28.05.08ITEP meeting S.Kiselev2
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28.05.08ITEP meeting S.Kiselev3 Introduction - definitions Direct photons: not from hadron decays Quark gluon level: qq gγ, qg qγ, qq(g) qq(g)γ. Initial hard NN collisions, pQCD prompt γ Thermalised QGP stage thermal γ from QGP.
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28.05.08ITEP meeting S.Kiselev4 Introduction – definitions Hadron level: meson scatterings: ππ ργ, πρ πγ, πK K * γ, Kρ Kγ, KK * πγ, πK * Kγ,... Thermalised hadron stage thermal γ from HHG Decay photons: Long lived (c » c AB ~ 50-100 fm) π 0 γγ, γγ, ’ ργ/ωγ/2γ Shot lived (c c AB ~ 50-100 fm) ω πγ, a 1 πγ, Δ Nγ, K * Kγ, γ, ρ ππγ,...
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Introduction – SPS data 28.05.08ITEP meeting S.Kiselev5
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Introduction – RHIC data 28.05.08ITEP meeting S.Kiselev6
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28.05.08ITEP meeting S.Kiselev7 Photons in A+A Direct PhotonsDecay Photons hardthermalhard+thermal QGPHadron gas`direct`fragmentation Preequilibrium photons ??? jet- - conv. Medium induced bremsstr. Introduction - new processes at RHIC Hard scattered parton interacts with gluon in bulk matter
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28.05.08ITEP meeting S.Kiselev8 Prompt photons: pp data fit + binary scaling PHENIX hep-ph/0609037 (√s) 5 Ed 3 σ/d 3 p = F(x T,y) One can use a data tabulation of the F(x T,y) to generate prompt photons. A+B: Ed 3 N/d 3 p(b)= Ed 3 σ pp /d 3 p AB T AB (b)= Ed 3 σ pp /d 3 p N coll (b)/σ pp in Nuclear effects (Cronin, quenching, …) are not taken into account. Realization: GePP.C macros for ROOT
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28.05.08ITEP meeting S.Kiselev9 Generator of Prompt Photons (GePP): results Comparison with RHIC data Prediction for LHC
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28.05.08ITEP meeting S.Kiselev10 Bjorken -(1+1)-HydroDynamics (BHD) Proper time and rapidity y Phys.Rev.D27(1983)140 There is no dependence on Lorenz boost variable y: Landau hydrodynamical model, viscosity and conductivity are neglected
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28.05.08ITEP meeting S.Kiselev11 Photon spectrum in BHD Photon spectra follow from convoluting the photon production rates with the space–time evolution of the collision For a longitudinally expanding cylinder For proper time and rapidity y ` For an ideal gas Main parameters: initial 0, T 0 and T f (at freeze-out) Connection with the local rest frame Input function – production rate E dN/d 4 xd 3 p (E,T) Phys.Rep.364(2002)98
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28.05.08ITEP meeting S.Kiselev12 HHG scenario C.Song, Phys.Rev.C47(1993)2861 an effective chiral Lagrangian with π, ρ and a 1 mesons to calculate the processes ππ →ργ, πρ → πγ, and ρ →ππγ. C.Song and G.Fai, Phys.Rev.C58(1998)1689. parameterizations for photon rates. Realization: GeT_HHG.C macros for ROOT
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28.05.08ITEP meeting S.Kiselev13 GeT_HHG: comparison with SPS and RHIC Choosing T 0 and 0 one can fit data in the hadron scenario comparison with data, T f = 100 MeV
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28.05.08ITEP meeting S.Kiselev14 GeT_HHG: prediction for LHC
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28.05.08ITEP meeting S.Kiselev15 GeT_HHG: sensitivity to the parameters sensitivity to T 0 sensitivity to T f
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28.05.08ITEP meeting S.Kiselev16 QGP scenario: QGP and HHG phases QGP: ideal massless parton gas (µ q =0)HHG: ideal massless pion gas First order phase transition at critical temperature T c B bag constant N c colors N f flavors g number of degrees of freedom
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QGP scenario: mixed phase 28.05.08ITEP meeting S.Kiselev17 Mixed phase Main parameters: initial 0, T 0, T c and T f
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Rates from QGP -1 st order 28.05.08ITEP meeting S.Kiselev18 Perturbative thermal QCD applying Hard thermal loop (HTL) resummation Phys.Lett.B510(2001)98
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Rates from QGP -2 nd order 28.05.08ITEP meeting S.Kiselev19 Thermal photon production in the QGP is a non-perturbative mechanism that can not be accessed in perturbative HTL resummed thermal field theory 2-loop contribution is the same order in α s One must consider the QGP rates as an educated guess
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To do 28.05.08ITEP meeting S.Kiselev20 Write and test the macros GeT_QGP.C Think on the “hard+thermal” generator
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