1 The Quark Gluon Plasma and the Perfect Fluid Quantifying Degrees of Perfection Jamie Nagle University of Colorado, Boulder.

Slides:



Advertisements
Similar presentations
Mass, Quark-number, Energy Dependence of v 2 and v 4 in Relativistic Nucleus- Nucleus Collisions Yan Lu University of Science and Technology of China Many.
Advertisements

Supported by DOE 11/22/2011 QGP viscosity at RHIC and LHC energies 1 Huichao Song 宋慧超 Seminar at the Interdisciplinary Center for Theoretical Study, USTC.
TJH: ISMD 2005, 8/9-15 Kromeriz, Czech Republic TJH: 1 Experimental Results at RHIC T. Hallman Brookhaven National Laboratory ISMD Kromeriz, Czech Republic.
1Erice 2012, Roy A. Lacey, Stony Brook University.
R. Lacey, SUNY Stony Brook 1 Arkadij Taranenko Winter Workshop on Nuclear Dynamics Big Sky, MT February 12-17,2007 Nuclear Chemistry Group SUNY Stony Brook,
In relativistic heavy ion collisions a high energy density matter Quark-Gluon Plasma (QGP) may be formed. Various signals have been proposed which probe.
Motivation One of the major findings at the Relativistic Heavy Ion Collider (RHIC) is the suppression of the highly energetic particles which raises the.
Forward-Backward Correlations in Relativistic Heavy Ion Collisions Aaron Swindell, Morehouse College REU 2006: Cyclotron Institute, Texas A&M University.
The speed of sound in a magnetized hot Quark-Gluon-Plasma Based on: Neda Sadooghi Department of Physics Sharif University of Technology Tehran-Iran.
The Physics of Relativistic Heavy Ion Collisions
Relativistic Heavy-Ion Collisions: Recent Results from RHIC David Hardtke LBNL.
1 Questions about sQGP Carlos Arguello Columbia University 24 th Winter Workshop on Nuclear Dynamics April 10 th 2008.
Quark recombination in high energy collisions for different energies Steven Rose Worcester Polytechnic Institute Mentor: Dr. Rainer Fries Texas A&M University.
Forward-Backward Correlations in Heavy Ion Collisions Aaron Swindell, Morehouse College REU Cyclotron 2006, Texas A&M University Advisor: Dr. Che-Ming.
200 GeV Au+Au Collisions, RHIC at BNL Animation by Jeffery Mitchell.
Finite Size Effects on Dilepton Properties in Relativistic Heavy Ion Collisions Trent Strong, Texas A&M University Advisors: Dr. Ralf Rapp, Dr. Hendrik.
1 ALICE Status Orlando Villalobos Baillie University of Birmingham NuPECC Meeting Edinburgh 10 th October 2014.
Behind QGP Investigating the matter of the early Universe Investigating the matter of the early Universe Is the form of this matter Quark Gluon Plasma?
Strings and Things: The Discovery of the strongly interacting Quark Gluon Plasma at the Relativistic Heavy Ion Collider Richard Seto UCR Teachers Academy.
Christina Markert Physics Workshop UT Austin November Christina Markert The ‘Little Bang in the Laboratory’ – Accelorator Physics. Big Bang Quarks.
Photo-emission in hQCD and LHC Sang-Jin Sin (Hanyang 2010/08/11.
John Chin-Hao Chen1 Quark Gluon Plasma: the Hottest Matter on Earth John Chin-Hao Chen ( 陳勁豪 ) RIKEN Brookhaven Research Center Brookhaven National.
New States of Matter and RHIC Outstanding questions about strongly interacting matter: How does matter behave at very high temperature and/or density?
Discovery of the Higgs Boson Gavin Lawes Department of Physics and Astronomy.
Strange and Charm Probes of Hadronization of Bulk Matter at RHIC International Symposium on Multi-Particle Dynamics Aug 9-15, 2005 Huan Zhong Huang University.
Relativistic Heavy Ion Physics: the State of the Art.
Collective Flow in Heavy-Ion Collisions Kirill Filimonov (LBNL)
Precision Probes for Hot QCD Matter Rainer Fries Texas A&M University & RIKEN BNL QCD Workshop, Washington DC December 15, 2006.
The Color Glass Condensate Outstanding questions: What is the high energy limit of QCD? How do gluons and quarks arise in hadrons? What are the possible.
STRING PERCOLATION AND THE GLASMA C.Pajares Dept Particle Physics and IGFAE University Santiago de Compostela CERN The first heavy ion collisions at the.
November 18, Shanghai Anomalous Viscosity of an Expanding Quark-Gluon Plasma Masayuki ASAKAWA Department of Physics, Osaka University S. A.
High Energy Nuclear Physics and the Nature of Matter Outstanding questions about strongly interacting matter: How does matter behave at very high temperature.
EXPERIMENTAL EVIDENCE FOR HADRONIC DECONFINEMENT In p-p Collisions at 1.8 TeV * L. Gutay - 1 * Phys. Lett. B528(2002)43-48 (FNAL, E-735 Collaboration Purdue,
09/15/10Waye State University1 Elliptic Flow of Inclusive Photon Ahmed M. Hamed Midwest Critical Mass University of Toledo, Ohio October, 2005 Wayne.
Ultra-relativistic heavy ion collisions Theoretical overview ICPAQGP5, KOLKATA February 8, 2005 Jean-Paul Blaizot, CNRS and ECT*
High Pt physics with TOF ALICE B.V.Zagreev ITEP
Relativistic Heavy Ion Collider and Ultra-Dense Matter.
1 Highlights of RHIC Results Ju Hwan Kang Yonsei University 2008 APCTP Workshop on "Nuclear Physics in Science Business Belt: Future Heavy Ion Accelerator.
Hadron Collider Physics 2012, 12/Nov/2012, KyotoShinIchi Esumi, Univ. of Tsukuba1 Heavy Ion results from RHIC-BNL ShinIchi Esumi Univ. of Tsukuba Contents.
Quark-Gluon Plasma Sijbo-Jan Holtman.
Physics of Dense Matter in Heavy-ion Collisions at J-PARC Masakiyo Kitazawa J-PARC 研究会、 2015/8/5 、 J-PARC.
QuarkNet 2006 Lets go smash some Atoms! Peripheral Collision:Central Collision Head-On Collision: Largest # of Nucleons Participate Glancing Collision:
U N C L A S S I F I E D Operated by the Los Alamos National Security, LLC for the DOE/NNSA Slide 0 Study of the Quark Gluon Plasma with Hadronic Jets What:
1 Tatsuya Chujo Univ. of Tsukuba Hadron Physics at RHIC HAWAII nd DNP-APS/JPS Joint Meeting (Sep. 20, 2005)
1 The Golden Age for Studying Hot QCD Matter Jamie Nagle University of Colorado 2008 Annual Meeting of the Division of Nuclear Physics October 23, 2008;
John Harris (Yale) LHC Conference, Vienna, Austria, 15 July 2004 Heavy Ions - Phenomenology and Status LHC Introduction to Rel. Heavy Ion Physics The Relativistic.
Shear and Bulk Viscosities of Hot Dense Matter Joe Kapusta University of Minnesota New Results from LHC and RHIC, INT, 25 May 2010.
Heavy-Ion Physics - Hydrodynamic Approach Introduction Hydrodynamic aspect Observables explained Recombination model Summary 전남대 이강석 HIM
High-p T Particles and RHIC Paradigm of Jet Quenching Ahmed M. Hamed NN2012 The 11 th International Conference on Nucleus-Nucleus Collisions 1.
Olena Linnyk Charmonium in heavy ion collisions 16 July 2007.
Hydrodynamic Flow from Fast Particles Jorge Casalderrey-Solana. E. V. Shuryak, D. Teaney SUNY- Stony Brook.
HIM06-12 SHLee1 Some Topics in Relativistic Heavy Ion Collision Su Houng Lee Yonsei Univ., Korea 1.J. P. Blaizot 2.J. Kapusta 3.U. A. Wiedemann.
24 Nov 2006 Kentaro MIKI University of Tsukuba “electron / photon flow” Elliptic flow measurement of direct photon in √s NN =200GeV Au+Au collisions at.
1 Probing dense matter at extremely high temperature Rudolph C. Hwa University of Oregon Jiao Tong University, Shanghai, China April 20, 2009.
Relativistic Heavy Ion Collider Where Are We and Where Are We Going? Jamie Nagle University of Colorado at Boulder RHIC & AGS User’s Reception APS Meeting,
New Physics at the Relativistic Heavy Ion Collider Associate Professor Jamie Nagle University of Colorado at Boulder XXXIV SLAC Summer Institute July 17-28,
Xin-Nian Wang/LBNL QCD and Hadronic Physics Beijing, June 16-20, 2005 Xin-Nian Wang 王新年 Lawrence Berkeley National Laboratory Jet Tomography of Strongly.
Elliptic Flow of Inclusive Photon Elliptic Flow of Inclusive Photon Ahmed M. Hamed Midwest Critical Mass University of Toledo, Ohio Oct. 22,
What have we learned from the RHIC experiments so far ? Berndt Mueller (Duke University) KPS Meeting Seoul, 22 April 2005.
What do the scaling characteristics of elliptic flow reveal about the properties of the matter at RHIC ? Michael Issah Stony Brook University for the PHENIX.
Elliptic flow from initial states of fast nuclei. A.B. Kaidalov ITEP, Moscow (based on papers with K.Boreskov and O.Kancheli) K.Boreskov and O.Kancheli)
Towards understanding the Quark-Gluon Plasma
Review of ALICE Experiments
Cyrille Marquet Columbia University
Collective Dynamics at RHIC
QCD (Quantum ChromoDynamics)
Properties of the Quark-Gluon Plasma
QGP at RHIC: Seen through Modified Jet Fragmentation
of Hadronization in Nuclei
Introduction of Heavy Ion Physics at RHIC
Presentation transcript:

1 The Quark Gluon Plasma and the Perfect Fluid Quantifying Degrees of Perfection Jamie Nagle University of Colorado, Boulder

2 What do terms like “Quark Soup” and “Perfect Liquid” mean? How does that compare with a “Quark Gluon Plasma”? Good questions !

3 Quark Gluon Plasma

4 Can we melt the hadrons and liberate quark and gluon degrees of freedom? Energy density for “g” massless d.o.f. Hadronic Matter: quarks and gluons confined For T ~ 200 MeV, 3 pions with spin=0 Quark Gluon Matter: 8 gluons; 2 quark flavors, antiquarks, 2 spins, 3 colors 37 ! Degrees of Freedom

5 Lattice QCD Confirmation Temperature / T c  /T 4 And it reaches 80% of the non-interacting gas limit. QCD does reveal a transition (smooth cross over perhaps) with almost an order of magnitude change in the thermodynamic degrees of freedom.

6 “Freely Roaming” Quarks and Gluons? “Quarks and gluons freely roam within the volume of the fireball created by the collision.” This implies that thermodynamic degrees of freedom are associated with specific moving quasi-particles. Quasi-particle = collective medium excitation that has a width which is much smaller than its energy and acts like a ballistic particle Is this “freely roaming” picture right? 2000

7 Crank the Energy Up and Do the Experiment ! 10,000 virtual gluons, quarks, and antiquarks from the nuclear wavefunctions are made physical in the laboratory ! What is the nature of this ensemble of partons?

8 Relativistic Heavy Ion Collider online since Design Au+Au energy and luminosity achieved. All experiments successfully taking data Polarized proton proton (spin) program underway STAR RHIC is doing great !

9

10 Out of a maximum energy of 39.4 TeV in central Gold Gold reactions, 26 TeV is deposited in the fireball. Energy density is far above the expected transition point. 26 TeV Fireball !

11 0 fm/c 2 fm/c 7 fm/c >7 fm/c Diagram from Peter Steinberg Time Evolution

12  ,  0, K , K *0 (892), K s 0, , p, d,  0, , ,  ,  0, K , K *0 (892), K s 0, , p, d,  0, , , ,  *(1385), ,  ,  *(1385),  *(1520),  ±,  (+ antiparticles) (+ antiparticles) in equilibrium at T > 170 MeV What Happens to All That Energy?

13 How Does the Matter Behave? Simple answer is with a very high degree of collectivity.

14 First time hydrodynamics without any viscosity describes heavy ion reactions. *viscosity = resistance of liquid to shear forces (and hence to flow) Thermalization time t=0.6 fm/c and  =20 GeV/fm 3 Like a Perfect Liquid? v2 p T (GeV)

15 Hydrodynamics Assume early equilibration and initial geometry Equations of Motion Equation of State from lattice QCD

16 Liquid  Hadrons Previous hydrodynamics assumes Liquid  Hadrons Mapping knows nothing of hadron structure, only masses. This breaks down at higher p T !

17 Flow “Knows” Quark Content ! Fluid  QuasiParticles  Hadrons Evidence for fluid breaking up into quasiparticles with quantum numbers of quarks before hadrons. n q = number of valence quarks

18 What Does This Mean? PHENIX: “Scaling suggests that partonic collectivity dominates the transverse expansion dynamics.” STAR: “[Scaling indicates] a pre-hadronization state in which the flowing medium reflects quark degrees of freedom.” Not exactly. Inviscid fluids do not carry quasi-particles, almost by definition (they create viscosity). Thus, thermodynamic degrees of freedom do not correspond to ballistic quasi-particles during the “perfect fluid time.” However, as the fluid breaks down, it may be that quasi-particles are formed that have an anisotropy pattern. Then these quasi-particles hadronize and their anisotropy is imprinted on all hadrons.

19 String Theory ? What could this have to do with our physics? The Maldacena duality, know also as AdS/CFT correspondence, has opened a way to study the strong coupling limit using classical gravity where it is difficult even with lattice Quantum Chromodynamics. It has been postulated that there is a universal lower viscosity bound for all strongly coupled systems, as determined in this dual gravitational system.

20 Critical future goal to put the QCD data point on this plot. ? Universal Viscosity Bound

21 Probing the Matter Calibrated LASER Matter we want to study Calibrated Light Meter Calibrated Heat Source Take an out of equilibrium probe and see how it equilibrates !

22 Sometimes a high energy photon is created in the collision. We expect it to pass through the plasma without pause. Probes of the Medium Photons do not equilibrate with the matter.

23 Sometimes we produce a high energy quark or gluon. If the plasma is dense enough we expect the quark or gluon to be swallowed up. Probes of the Medium Quarks and Gluons do approach equilibration. Can we determine a transport coefficient q? ^

24 (from quark and gluon jets) Scaling of photons shows excellent calibrated probe. Quarks and gluons disappear into medium, except consistent with surface emission. Survival Probability Size of Medium Experimental Results

25 Constraint on Transport Coefficient Future running and RHIC II luminosities will give a precision measure of the transport coefficient. A major goal is to make such a constraint on other properties like  /s as detailed before.

26 Alternative: Put a pebble (or rock) in the stream….and watch something out of equilibrium then equilibrate. Need 3-d relativistic viscous hydrodynamics to compare to bulk medium flow. Significant theory milestone! How to Quantify  /s? Charm Quark Beauty Quark Perfect Fluid?

27 Charm Quark Probes Teaney and Moore Very large interactions suppress high p T and induce large flow. Suppression FactorFlow

28 Constraining  /s Rapp and van Hees Phys.Rev.C71:034907,2005 Phys.Rev.C71:034907,2005 –Simultaneously describe R AA (E) and v 2 (e) with diffusion coefficient in range D HQ (2  T) ~4-6 Moore and Teaney Phys.Rev.C71:064904,2005 Phys.Rev.C71:064904,2005 –Find D HQ /(  /(  +p)) ~ 6 for N f =3 Combining –  +p = T s at  B =0 –This then gives  /s ~(1.33-2)/ 4  Within a factor of 2 of the bound. Need separation of c and b to pin this down better.

29 Jet correlations in proton-proton reactions. Strong back-to- back peaks. Jet correlations in central Gold-Gold. Away side jet disappears for particles p T > 2 GeV Jet correlations in central Gold-Gold. Away side jet reappears for particles p T >200 MeV Azimuthal Angular Correlations Jet Quenching !

30 Where Does the Energy Go?

31 How does the near perfect liquid react to this large energy deposition? Color shock wave? Reaction of the Medium Sensitive to –Speed of sound –Equation of state

32 Conclusions RHIC program is operating very successfully. The Quark-Gluon Plasma as “freely roaming” quasi-particles carrying the degrees of freedom unlikely at early stages. Near Perfect Liquid Discovered. Challenge is now to quantify and understand its properties. Exciting future program at RHIC II and at the LHC. Perfect Liquid?