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QCD and Heavy Ions: an overview D. Kharzeev BNL XXXIX Rencontres de Moriond, March 28 - April 4 2004.

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Presentation on theme: "QCD and Heavy Ions: an overview D. Kharzeev BNL XXXIX Rencontres de Moriond, March 28 - April 4 2004."— Presentation transcript:

1 QCD and Heavy Ions: an overview D. Kharzeev BNL XXXIX Rencontres de Moriond, March 28 - April 4 2004

2 Outline QCD of strong color fields: parton saturation and Color Glass Condensate Manifestations of CGC at RHIC: o hadron multiplicities o high p T suppression at forward rapidity Future tests: RHIC, LHC, eRHIC From CGC to Quark-Gluon Plasma

3 QCD and the classical limit QCD = Quark Model + Gauge Invariance For,.i Classical dynamics applies when the action is large: => Need weak coupling and strong fields

4 Asymptotic freedom and the classical limit of QCD Classical limit S>>1 requires weak coupling and strong fields; Large distances: strong fields but large coupling… Is there a place for classical methods?

5 Parton saturation and the classical limit of QCD At small Bjorken x, hard processes develop over.large longitudinal distances All partons contribute coherently => at sufficiently small x and/or.large A strong fields, weak coupling!

6 The phase diagram of high energy QCD … no numbers yet, but they will follow

7 Non-linear effects in the QCD evolution QCD evolution equations (DGLAP, BFKL) predict an increase of parton densities at small Bjorken x, in agreement with experiment; at “sufficiently small” x and/or large A non-linear effects must become important (GLR; MQ; JIMWLK; ILM). At large, equations can be written in a closed form - BK (dipole scatterings are assumed to be independent - similar to the mean field approximation in statistical physics) but correlations may be important - see e.g. E.Iancu, A.H.Mueller, hep-ph/0309276; A.H.Mueller, A.I.Shoshi, hep-ph/0402193

8 CGC and total multiplicities in Au-Au CGC predicts very simple dependence of multiplicity.on atomic number A / N part : Almost like in “wounded nucleon” and string-based models; Agrees unexpectedly well with “soft + hard” parameterizations (note: total multiplicities are dominated by small transverse momenta => classical dynamics applicable)

9 dN ch /d  @  =0 vs Energy Parton interactions at RHIC.are coherent !

10 Centrality dependence of hadron multiplicity => Talk by D. Hofman

11 Centrality dependence at different energies

12 Initial state parton saturation? QM2002: nucl-ex/0212009 ~0.25 from fits to HERA data: xG(x)~x  Describes energy dependence correctly! Kharzeev, Levin, Nardi, hep-ph/0111315 200 GeV 130 GeV Preliminary 19.6 GeV

13 Rachid Nouicer13 Parton Saturation Describes Au + Au Kharzeev & Levin, Phys. Lett. B523 (2001) 79 Au + Au at 130 GeV We need a simpler system such as d + Au in order to understand a complex system Au + Au The results of d+Au are crucial for testing the saturation approach PHOBOS Coll., R. Noucier Color Glass Condensate describes the Au-Au data

14 D-Au multiplicities Data from BRAHMS and PHOBOS Collaborations DK, E.Levin and M.Nardi, Nucl.Phys.A730(2004)448, + erratum, hep-ph/0212316

15 From CGC to Quark Gluon Plasma: approach to thermalization The data on azimuthal anisotropy of hadron production indicate strong final state interactions at short time scales U.Heinz, E.Shuryak, … => Talk by R.Snellings Problem: if interactions are perturbative, interaction probabilities are small - suppressed by powers of if interactions are non-perturbative, characteristic re-interaction time is about 1 fm Possible solution: CGC sets a fast time scale (~ 0.2 fm) and classical fields re-interact with ~ O(1) probability (almost) isentropic evolution => ideal hydrodynamics is reasonable R.Baier, A.H.Mueller, D. Schiff, D.T. Son, PLB502(2001)51; 539(2002)46; …

16 From CGC to Quark Gluon Plasma L. McLerran, T. Ludlam, Physics Today, October 2003

17 Signatures of the Quark Gluon Plasma O jet quenching o suppression of heavy quarkonia o collective flow o fluctuations and correlations o dilepton and photon enhancement o particle abundancies o exotica: DCC, parity violation, …

18 The discovery of high p T suppression at RHIC => Talk by D. d’Enterria

19 What happens at higher transverse momenta? PHENIX and STAR extend measurements to ~ 10 GeV

20 Centrality Dependence vs p T Phobos

21 Is this the jet quenching in QGP? Bjorken; Gyulassy, Wang; Baier, Dokshitzer, Mueller, Peigne, Schiff; Wiedemann, Salgado; Vitev, Levai, … Very likely;.but could there be alternative explanations? (2002)lternative DK, Levin, McLerran hep-ph/0210332 Yes, possibly: 1) Small x evolution leads to.the modification of gluon propagators - “anomalous dimension”: 2) Q s is the only relevant dimensionful parameter in the CGC;.thus everything scales in the ratio 3) Since Tthe A-dependence is changed => N part scaling!

22 D-Au collisions: suppression or enhancement?

23 R dAu vs p T Central Au+Au Phobos

24 p+p vs. d+Au Azimuthal correlations are qualitatively consistent Quantitative evaluation will constrain o Nuclear k T from initial state multiple scattering o Shadowing Models that predict “monojets” due to initial state effects ruled out No “data manipulation” D. Hardtke, STAR Coll. => Talk by F. Wang

25 Conclusion: high p T suppression is a final-state effect Can one prove that it is due to a radiative jet energy loss In the Quark-Gluon Plasma? Quite likely: one possibility is to use the heavy quarks Radiation off heavy quarks is suppressed (“dead cone”) => less quenching On the other hand, D mesons have about the same size as.pions and kaons, and so in the hadron absorption scenario.the suppression should be the same Yu.Dokshitzer, DK ‘01 => Talk by N. Armesto

26 However, the arguments for the CGC-caused,suppression should hold for sufficiently small x; Does this happen at RHIC? Study the forward rapidity region: Moving to y=+4 from y=0 increases the saturation scale.by factor of three RHIC results: Talks by B. Cole, E. Kistenev, M. Liu, F. Wang

27 Expectations for R dAu at large rapidity Agreement on the presence of suppression due to the quantum Small x evolution in the CGC picture: DK, E. Levin and L. McLerran, hep-ph/0210332; R. Baier, A. Kovner, U. Wiedemann, hep-ph/0305265 v2 DK, Yu.Kovchegov and K. Tuchin, hep-ph/0307037 v2 J. Albacete, N. Armesto, A. Kovner, C. Salgado, U. Wiedemann, hep-ph/0307179; Agreement on the presence of Cronin effect in the classical,approach and in the multiple scattering picture: L.McLerran and R.Venugopalan; Yu.Kovchegov and A.H.Mueller; J. Jalilian-Marian; A. Dumitru; F. Gelis;… X.N.Wang; M. Gyulassy; I. Vitev;…

28 Model predictions I. Vitev nucl-th/0302002 v2 D. Kharzeev, Yu. Kovchegov and K. Tuchin, hep-ph/0307037 CGC at y=0 Y=0 Y=3 Y=-3 Very high energy As y grows R. Debbe, BRAHMS Coll., Talk at DNP Meeting, Tucson, November 2003

29 d-Au Nuclear Modification factor at  ~3.2 BRAHMS preliminary RdAu compares the yield of negative particles produced in dAu to the scaled number of particles with same sign in p-p The scale is the number of binary collisions: N coll =7.2 (minimum biased) PRL 91 072305 (2003) R. Debbe, BRAHMS Collaboration, Talk at the DNP Meeting, Tucson, November 2003

30 R dAu at different rapidities All ratios extracted from minimum biased data samples Number of binary collisions in minimum biased events is estimated: N coll = 7.2±0.3 Statistical errors dominant over the systematic ones at  =2 and 3 Systematic error (not shown) ~15% The values for  =0 were published in: PRL 91 072305 (2003) R.Debbe, BRAHMS, QM’04

31 Centrality dependence All numerators and denominator are scaled by the appropriate estimated number of binary collisions (HIJING + BRAHMS GEANT) The ratios are corrected for trigger inefficiency. All other corrections (acceptance, tracking efficiency.. ) cancel out. R.Debbe, BRAHMS, QM’04

32 Centrality Dependence of Particle Production @Fwd/Bwd Directions 1.Stopped hadrons –Mesons + Baryons 2.Light mesons –Pions + Kaons 3.Heavy flavors –Charm + Beauty Au d Ming Liu, PHENIX, QM’04 => Talk by M. Liu

33 d+Au R CP at forward rapidities P T [GeV/c] R CP Au-Side R CP shows almost no variation with centrality d-side is interesting: more central is more suppressed L.Barnby, STAR, QM’04

34 d Au spectra at (not so) forward rapidity P. Steinberg, PHOBOS, QM’04

35 Rapidity dependence of R dAu

36 Is this “just shadowing”? Yes, it is - shadowing is the deviation of nuclear parton distributions from the nucleon’s ones. CGC is a theory of shadowing Conventional parameterizations of shadowing have so far failed in describing the rapidity and centrality dependence of the data (EKS, de Florian, Accardi-Gyulassy,… Some approaches (e.g. HIJING shadowing) describe suppression at y=3, but also predict it at y=0. NB:approaches relating shadowing to diffraction should work

37 Further tests of quantum evolution in the CGC Back-to-back correlations for jets separated by several units of rapidity are very sensitive to the evolution effects A.H.Mueller,H.Navelet and to the presence of CGC DK, E.Levin,L.McLerran, hep-ph/0403271 Open charm, dileptons, photons DK, K.Tuchin, hep-ph/0310.. in the forward region R.Baier,A.H.Mueller,D.Schiff, hep-ph/0403201

38 Phase diagram of high energy QCD

39 Summary High energy heavy ion program allows to study QCD in the domains of high parton density (small x, large A) and high energy density Novel exciting effects have been observed in Au-Au and forward d-Au interactions; they point towards the collective partonic behavior and non-linear dynamics at small x

40 Back-up slides

41 d Au Phenix Preliminary Stopped Hadrons!

42 d Au Stopped Hadrons! Phenix Preliminary

43 d Au Shadowing? Cronin effect & anti-shadowing? Stopped Hadrons! Phenix Preliminary

44 R CP (y): Muons from Light Meson Decays Phenix Preliminary R CP


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