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A Nearly Perfect Ink !? Theoretical Challenges from RHIC Dublin - 29 July 2005 LATTICE 2005 Berndt Mueller (Duke University)
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A perfect ink… Is brilliantly dark and opaque Yet flows smoothly and easily A painful challenge to fountain pen designers A delightful challenge to physicists: Are the two requirements really compatible? Hint:
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The road to the quark-gluon plasma STAR …Is hexagonal and 2.4 miles long
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Two wealths Challenges A wealth of … D A T A
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Cornerstone results from RHIC Anisotropic transverse flow “Jet” suppression Baryon/meson enhancement
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Azimuthal anisotropy v 2 pypy Coordinate space: initial asymmetry Momentum space: final asymmetry pxpx x y Semiperipheral collisions Signals early equilibration (t eq 0.6 fm/c)
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Jet quenching in Au+Au PHENIX Data: Identified 0 d+Au Au+Au No quenching Quenching!
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Baryons vs. mesons baryonsmesons R CP p T (GeV/c) behaves like meson ? (also -meson)
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Overview QCD Thermodynamics What are the dynamical degrees of freedom? Is there a critical point, and where is it? Thermalization How can it be so fast? Transport in a thermal medium Viscosity, energy loss, collective modes Hadronization Recombination vs. fragmentation
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QCD phase diagram BB Hadronic matter Critical endpoint ? Plasma Nuclei Chiral symmetry broken Chiral symmetry restored Color superconductor Neutron stars T 1 st order line ? Quark- Gluon RHIC
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Space-time picture eq Pre-equil. phase Bjorken formula
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Stages of a r.h.i. collision Initial collision ≈ break-up of the coherent gluon field (“color glass condensate”) Pre-equilibrium: the most puzzling stage Equilibrium (T > T c ): hydrodynamic expansion in longitudinal and transverse directions Hadronization: are there theoretically accessible domains in p T ? Hadronic stage (T < T c ): Boltzmann transport of the hadronic resonance gas
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Initial state: Gluon saturation ~ 1/Q 2 Details of space-time picture depend on gauge! Gribov, Levin, Ryskin ’83 Blaizot, A. Mueller ’87 McLerran, Venugopalan ‘94 “Color glass condensate (CGC)”
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CGC dynamics Initial state occupation numbers ~ 1/ s 1 → classical fields generated by random color sources on light cone: Boost invariance → Hamiltonian gauge field dynamics in transverse plane (x , ). 2-dim lattice simulation shows rapid equipartitioning of energy ( eq ~ Q s -1 ). Krasnitz, Nara & Venugopalan; Lappi (hep-ph/0303076 ) Challenge: (3+1) dim. simulation without boost invariance
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Saturation and dN/d Kharzeev & Levin Pseudorapidity = - ln tan Rapidity y = ln tanh(E+p L )/(E-p L ) Assume nucleus is “black” for all gluons with k T Q s : Q s (x) → Q s (y) with x = Q s e -|Y-y|. Also predicts beam energy dependence of dN/dy. Challenge: How much entropy is produced by simple decoherence, how much during the subsequent full equilibration?
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The(rmalization) mystery Experiment demands: th 0.6 fm/c “Bottom up” scenario ( Baier, A. Mueller, Schiff, Son ) : “Hard” gluons with k T ~ Q s are released from the CGC; Released gluons collide and radiate thermal gluons; Thermalization time th ~ [ s 13/5 Q s ] -1 ≈ 2-3 fm/c Perturbative dynamics among gluons does not lead to rapid thermalization. Quasi-abelian instability ( Mrowczynski; Arnold et al; Rebhan et al ): Non-isotropic gluon distributions induce exponentially growing field modes at soft scale k ~ gQ s ; These coherent fields deflect and isotropize the “hard” gluons.
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After thermalization…... matter is described by (relativistic) hydrodynamics ! Requires f L and small shear viscosity . HTL pert. theory (n f =3): Dimensionless quantity /s. Classical transp. th.: ≈ 1.5 T f, s ≈ 4 → /s ≈ 0.4T f. (Baym…; Arnold, Moore & Yaffe)
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Azimuthal anisotropy v 2 pypy Coordinate space: initial asymmetry Momentum space: final asymmetry pxpx x y Semiperipheral collisions Signals early equilibration (t eq 0.6 fm/c)
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– How small can it be? D. Teaney Boost invariant hydro with T 0 0 ~ 1 requires /s ~ 0.1. N=4 SUSY Yang-Mills theory (g 1): /s = 1/4 (Kovtun, Son, Starinets). Absolute lower bound on /s ? /s = 1/4 implies f ≈ (5 T) -1 ≈ 0.3 d Challenge: (3+1) dim. relativistic viscous fluid dynamics QGP(T ≈T c ) = sQGP
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First attempts Nakamura & Sakai SU(3) YM Related (warm-up?) problem: EM conductivity ≈ q 2 f /2T. n f = 3 QGP → / ≈ 20 T 2. Caveat: f (glue) f (quarks) Method: spectral function repr. of G and G ret, fit of spectral fct. to G . Challenge: Calculate /s for real QCD
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QCD equation of state 20% Challenge: Devise method for determining from data Challenge: Identify the degrees of freedom as function of T Is the (s)QGP a gaseous, liquid, or solid plasma ? Challenge: QCD e.o.s. with light domain wall quarks
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A possible method Eliminate T from and s : Lower limit on requires lower limit on s and upper limit on . BM & K. Rajagopal, hep-ph/0502174
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Measuring and s Entropy is related to produced particle number and is conserved in the expansion of the (nearly) ideal fluid: dN/dy → S → s = S/V. Energy density is more difficult to determine: Energy contained in transverse degrees of freedom is not conserved during hydrodynamical expansion. Focus in the past has been on obtaining a lower limit on ; here we need an upper limit. New aspect at RHIC: parton energy loss. dE/dx is telling us something important – but what exactly?
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Entropy Two approaches: 1) Use inferred particle numbers at chemical freeze-out from statistical model fits of hadron yields; 2) Use measured hadron yields and HBT system size parameters as kinetic freeze-out (Pratt & Pal). Method 2 is closer to data, but requires more assumptions. Good news: results agree within errors: dS/dy = 5100 ± 400 for Au+Au (6% central, 200 GeV/NN) → s = (dS/dy)/( R 2 0 ) = 33 ± 3 fm -3
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Jet quenching in Au+Au PHENIX Data: Identified 0 d+Au Au+Au No quenching Quenching!
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High-energy parton loses energy by rescattering in dense, hot medium. q q Radiative energy loss: “Jet quenching” = parton energy loss qq g Scattering centers = color charges L Density of scattering centers Range of color force Scattering power of the QCD medium:
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Energy loss at RHIC Data suggest large energy loss parameter: RHIC Eskola, Honkanen, Salgado & Wiedemann p T = 4.5–10 GeV Dainese, Loizides, Paic
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The Baier plot Plotted against , is the same for a gas and for a perturbative QGP. Suggests that is really a measure of the energy density. Data suggest that may be larger than compatible with Baier plot. Nonperturbat. calculation is needed. Pion gas QGP Cold nuclear matter ˆ q ˆ q ˆ q RHIC data sQGP Challenge: Realistic calculation of gluon radiation in medium
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Eikonal formalism quark xx x - + Gluon radiation: x = 0 xx Kovner, Wiedemann
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Eikonal form. II Challenge: Compute F +i (x)F + i (0) for x 2 = 0 on the lattice Not unlike calculation of gluon structure function, maybe moments are calculable using euclidean techniques.
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Where does E loss go? STARp+pAu+Au Lost energy of away-side jet is redistributed to rather large angles! Trigger jetAway-side jet
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Wakes in the QGP Mach cone requires collective mode with (k) < k : J. Ruppert and B. Müller, Phys. Lett. B 618 (2005) 123 Colorless sound ? Colored sound = longitudinal gluons ? Transverse gluons Angular distribution depends on energy fraction in collective mode and propagation velocity T. Renk & J. Ruppert
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Baryons vs. mesons baryonsmesons R CP p T (GeV/c) behaves like meson ? (also -meson)
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Hadronization mechanisms Fragmentation Recombination
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Recombination wins… … for a thermal source Baryons compete with mesons Fragmentation dominates for a power-law tail
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Quark number scaling of v 2 In the recombination regime, meson and baryon v 2 can be obtained from the quark v 2 :
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Hadronization RHIC data (Runs 4 and 5) will provide wealth of data on: Identified hadron spectra up to much higher p T (~10 GeV/c); Elliptic flow v 2 up to higher p T with particle ID; Identified di-hadron correlations; Spectra and v 2 for D-mesons…. D D recombinationfragmentation Challenge: Unified framework treating recombination as special case of QCD fragmentation “in medium”. A. Majumder & X.N. Wang, nucl-th/0506040
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Some other challenges Where is the QCD critical point in ( ,T)? What is the nature of the QGP in T c < T < 2T c ? How well is QCD below T c described by a weakly interacting resonance gas? Thermal photon spectral function (m 2,T). Are there collective modes with (k) < k ? Can lattice simulations help understand the dynamics of bulk (thermal) hadronization?
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Don’t be afraid… “Errors are the doors to discovery” James Joyce
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Back-up slides
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Hard-soft dynamics Nonabelian Vlasov equations generalizing “hard-thermal loop” effective theory. Can be defined on (spatial 3-D) lattice with particles described as test charges or by multipole expansion (Hu & Müller, Moore, Bödeker, Rummukainen). Poss. problem: short-distance lattice modes have wrong (k). k ~ gQ s k ~ Q s Challenge: Full (3+1) dim. simulation of hard-soft dynamics
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Reco: Thermal quarks Quark distribution function at “freeze-out” Relativistic formulation using hadron light-cone frame: For a thermal distribution, the hadron wavefunctions can be integrated out, eliminating the model dependence of predictions. Remains exactly true even if higher Fock states are included!
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Heavy quarks Heavy quarks (c, b) provide a hard scale via their mass. Three ways to make use of this: Color screening of (Q-Qbar) bound states; Energy loss of “slow” heavy quarks; D-, B-mesons as probes of collective flow. RHIC program: c-quarks and J/ ; LH”I”C program: b-quarks and . RHIC data for J/ are forthcoming (Runs 4 & 5).
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J/ suppression ? V qq is screened at scale (gT) -1 heavy quark bound states dissolve above some T d. Karsch et al. Color singlet free energy Quenched lattice simulations, with analytic continuation to real time, suggest T d 2T c ! S. Datta et al. (PRD 69, 094507) Challenge: Compute J/ spectral function in unquenched QCD
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C-Cbar kinetics J/ LHC RHIC J/ , can be ionized by thermal gluons. If resonances persist above T c, J/ and can be formed by recombination in the medium: J/ may be enhanced at LHC! Challenge: Multiple scattering theory of heavy quarks in a thermal medium Analogous to the multiple scattering theory for high-p T partons, but using methods (NRQCD etc.) appropriate for heavy quarks.
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