Surprises from the Search for Quark-Gluon Plasma?* When Was Quark-Gluon Plasma Seen?
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The “Hot” Science of RHIC Status and Future
The “Hot” Science of RHIC Status and Future Berndt Mueller Brookhaven National Laboratory Associate Laboratory Director for Nuclear and Particle Physics BSA Board Meeting BNL, 29 March 2013 Friday, April 5, 13 RHIC: A Discovery Machine Polarized Jet Target (PHOBOS) 12:00 o’clock 10:00 o’clock (BRAHMS) 2:00 o’clock RHIC PHENIX 8:00 o’clock RF 4:00 o’clock STAR 6:00 o’clock LINAC EBIS NSRL Booster BLIP AGS Tandems Friday, April 5, 13 RHIC: A Discovery Machine Polarized Jet Target (PHOBOS) 12:00 o’clock 10:00 o’clock (BRAHMS) 2:00 o’clock RHIC PHENIX 8:00 o’clock RF 4:00 o’clock STAR 6:00 o’clock LINAC EBIS NSRL Booster BLIP AGS Tandems Pioneering Perfectly liquid quark-gluon plasma; Polarized proton collider Friday, April 5, 13 RHIC: A Discovery Machine Polarized Jet Target (PHOBOS) 12:00 o’clock 10:00 o’clock (BRAHMS) 2:00 o’clock RHIC PHENIX 8:00 o’clock RF 4:00 o’clock STAR 6:00 o’clock LINAC EBIS NSRL Booster BLIP Versatile AGS Wide range of: beam energies ion species polarizations Tandems Pioneering Perfectly liquid quark-gluon plasma; Polarized proton collider Friday, April 5, 13 RHIC: A Discovery Machine Polarized Jet Target (PHOBOS) 12:00 o’clock 10:00 o’clock (BRAHMS) 2:00 o’clock RHIC PHENIX 8:00 o’clock RF 4:00 o’clock STAR 6:00 o’clock LINAC EBIS NSRL Booster BLIP Versatile AGS Wide range of: beam energies ion species polarizations Tandems Pioneering Productive >300 refereed papers Perfectly liquid >30k citations quark-gluon plasma; >300 Ph.D.’s in 12 years Polarized proton collider productivity still increasing Friday, April 5, 13 Detector Collaborations 559 collaborators from 12 countries 540 collaborators from 12 countries 3 Friday, April 5, 13 RHIC explores the Phases of Nuclear Matter LHC: High energy collider at CERN with 13.8 - 27.5 ?mes higher Beam energy: PB+PB, p+PB, p+p collisions only. -
Jet Quenching in Quark Gluon Plasma: flavor Tomography at RHIC and LHC by the CUJET Model
Jet quenching in Quark Gluon Plasma: flavor tomography at RHIC and LHC by the CUJET model Alessandro Buzzatti Submitted in partial fulfillment of the requirements for the degree of Doctor of Philosophy in the Graduate School of Arts and Sciences Columbia University 2013 c 2013 Alessandro Buzzatti All Rights Reserved Abstract Jet quenching in Quark Gluon Plasma: flavor tomography at RHIC and LHC by the CUJET model Alessandro Buzzatti A new jet tomographic model and numerical code, CUJET, is developed in this thesis and applied to the phenomenological study of the Quark Gluon Plasma produced in Heavy Ion Collisions. Contents List of Figures iv Acknowledgments xxvii Dedication xxviii Outline 1 1 Introduction 4 1.1 Quantum ChromoDynamics . .4 1.1.1 History . .4 1.1.2 Asymptotic freedom and confinement . .7 1.1.3 Screening mass . 10 1.1.4 Bag model . 12 1.1.5 Chiral symmetry breaking . 15 1.1.6 Lattice QCD . 19 1.1.7 Phase diagram . 28 1.2 Quark Gluon Plasma . 30 i 1.2.1 Initial conditions . 32 1.2.2 Thermalized plasma . 36 1.2.3 Finite temperature QFT . 38 1.2.4 Hydrodynamics and collective flow . 45 1.2.5 Hadronization and freeze-out . 50 1.3 Hard probes . 55 1.3.1 Nuclear effects . 57 2 Energy loss 62 2.1 Radiative energy loss models . 63 2.2 Gunion-Bertsch incoherent radiation . 67 2.3 Opacity order expansion . 69 2.3.1 Gyulassy-Wang model . 70 2.3.2 GLV . 74 2.3.3 Multiple gluon emission . 78 2.3.4 Multiple soft scattering . -
From High-Energy Heavy-Ion Collisions to Quark Matter Episode I : Let the Force Be with You
From High-Energy Heavy-Ion Collisions to Quark Matter Episode I : Let the force be with you Carlos Lourenço, CERN CERN, August, 2007 1/41 The fundamental forces and the building blocks of Nature Gravity • one “charge” (mass) • force decreases with distance m1 m2 Electromagnetism (QED) Atom • two “charges” (+/-) • force decreases with distance + - + + 2/41 Atomic nuclei and the strong “nuclear” force The nuclei are composed of: quark • protons (positive electric charge) • neutrons (no electric charge) They do not blow up thanks to the neutron “strong nuclear force” • overcomes electrical repulsion • determines nuclear reactions • results from the more fundamental colour force (QCD) → acts on the colour charge of quarks (and gluons!) → it is the least well understood force in Nature proton 3/41 Confinement: a crucial feature of QCD We can extract an electron from an atom by providing energy electron nucleus neutral atom But we cannot get free quarks out of hadrons: “colour” confinement ! quark-antiquark pair created from vacuum quark Strong colour field “white” π0 “white” proton 2 EnergyE grows = mc with separation! (confined quarks) (confined quarks) “white” proton 4/41 Quarks, Gluons and the Strong Interaction A proton is a composite object No one has ever seen a free quark; made of quarks... QCD is a “confining gauge theory” and gluons V(r) kr “Confining” r 4 α − s 3 r “Coulomb” 5/41 A very very long time ago... quarks and gluons were “free”. As the universe cooled down, they got confined into hadrons and have remained imprisoned ever -
Hydrodynamic Models for Heavy-Ion Collisions, and Beyond
Symposium on Fundamental Issues in Fundamental Issues in Elementary Matter (2000) 000–000 Elementary Matter Bad Honnef, Germany September 25–29, 2000 Hydrodynamic Models for Heavy-Ion Collisions, and beyond A. Dumitru1,a, J. Brachmann2, E.S. Fraga3, W. Greiner2, A.D. Jackson4, J.T. Lenaghan4, O. Scavenius4, H. St¨ocker2 1 Physics Dept., Columbia Univ., 538 W. 120th Street, New York, NY 10027, USA 2 Institut f¨ur Theor. Physik, J.W. Goethe Univ., Robert-Mayer Str. 10, 60054 Frankfurt, Germany 3 Brookhaven National Laboratory, Upton, NY 11973, USA 4 The Niels Bohr Institute, Blegdamsvej 17, DK-2100 Copenhagen Ø, Denmark Abstract. A generic property of a first-order phase transition in equilibrium,andin the limit of large entropy per unit of conserved charge, is the smallness of the isentropic speed of sound in the “mixed phase”. A specific prediction is that this should lead to a non-isotropic momentum distribution of nucleons in the reaction plane (for energies ∼ 40A GeV in our model calculation). On the other hand, we show that from present effective theories for low-energy QCD one does not expect the thermal transition rate between various states of the effective potential to be much larger than the expansion rate, questioning the applicability of the idealized Maxwell/Gibbs construction. Ex- perimental data could soon provide essential information on the dynamicsof the phase transition. 1. Introduction arXiv:nucl-th/0010107 v1 31 Oct 2000 Heavy-ion collisions at high energy are devoted mainly to the study of strongly interact- ing matter at high temperature and density. In particular, a major focus is the search for observables related to restoration of chiral symmetry and deconfinement, as predicted by lattice QCD to occur at high temperature, and in thermodynamical equilibrium [ 1]. -
The Tale of the Hagedorn Temperature
Chapter 6 The Tale of the Hagedorn Temperature Johann Rafelski and Torleif Ericson Please note the Erratum to this chapter at the end of the book Abstract We recall the context and impact of Rolf Hagedorn’s discovery of limiting temperature, in effect a melting point of hadrons, and its influence on the physics of strong interactions. 6.1 Particle Production Collisions of particles at very high energies generally result in the production of many secondary particles. When first observed in cosmic-ray interactions, this effect was unexpected for almost everyone,1 but it led to the idea of applying the wide body of knowledge of statistical thermodynamics to multiparticle production processes. Prominent physicists such as Enrico Fermi, Lev Landau, and Isaak Pomeranchuk made pioneering contributions to this approach, but because difficulties soon arose this work did not initially become the mainstream for the study of particle production. However, it was natural for Rolf Hagedorn to turn to the problem. Hagedorn had an unusually diverse educational and research background, which included thermal, solid-state, particle, and nuclear physics. His initial work on statistical particle production led to his prediction, in the 1960s, of particle yields at the highest accelerator energies at the time at CERN’s proton synchrotron. Though there were few clues on how to proceed, he began by making the most of the ‘fireball’ concept, which was then supported by cosmic-ray studies. In this approach, all the energy of the collision was regarded as being contained within a small space- time volume from which particles radiated, as in a burning fireball. -
Deconfinement and Chiral Transition in Ads/QCD Wall Models
EPJ Web of Conferences 137, 03006 (2017) DOI: 10.1051/ epjconf/201713703006 XIIth Quark Confinement & the Hadron Spectrum Deconfinement and chiral transition in AdS/QCD wall models supplemented with a magnetic field David Dudal1;2;a, Diego R. Granado3;b, and Thomas G. Mertens4;2;c 1KU Leuven Campus Kortrijk - KULAK, Department of Physics, Etienne Sabbelaan 51 bus 7800, 8500 Kor- trijk, Belgium 2Ghent University, Department of Physics and Astronomy, Krijgslaan 281-S9, 9000 Gent, Belgium 3Departamento de Física, Universidade Federal Rural do Rio de Janeiro, BR 465-07, 23890-971, Seropédica, RJ, Brasil 4Joseph Henry Laboratories, Princeton University, Princeton, NJ 08544, USA Abstract. We discuss the phenomenon of (inverse) magnetic catalysis for both the de- confinement and chiral transition. We discriminate between the hard and soft wall model, which we suitably generalize to include a magnetic field. Our findings show a critical de- confinement temperature going down, in contrast with the chiral restoration temperature growing with increasing magnetic field. This is at odds with contemporary lattice data, so the quest for a holographic QCD model capable of capturing inverse magnetic catalysis in the chiral sector remains open. 1 Introduction The ongoing heavy ion collision programs (ALICE or RHIC) provide a fertile testing ground for novel experimental, phenomenological and theoretical features of strongly coupled QCD. During the early stages after the collision, a sufficiently hot heat bath is created that leads to the creation of a quark- gluon plasma, an exotic state of deconfined QCD matter. In units of the fundamental QCD scale, ΛQCD, the transition temperature Tdecon f ∼ ΛQCD, so the relevant physics is still strongly coupled. -
Lattice Investigations of the QCD Phase Diagram
Lattice investigations of the QCD phase diagram Dissertation ERSI IV TÄ N T U · · W E U P H P C E S I R T G A R L E B · 1· 972 by Jana Gunther¨ Major: Physics Matriculation number: 821980 Supervisor: Prof. Dr. Z. Fodor Hand in date: 15. December 2016 Die Dissertation kann wie folgt zitiert werden: urn:nbn:de:hbz:468-20170213-111605-3 [http://nbn-resolving.de/urn/resolver.pl?urn=urn%3Anbn%3Ade%3Ahbz%3A468-20170213-111605-3] Lattice investigations of the QCD phase diagram Acknowledgement Acknowledgement I want to thank my advisor Prof. Dr. Z. Fodor for the opportunity to work on such fascinating topics. Also I want to thank Szabolcs Borsanyi for his support and the discussions during the last years, as well as for the comments on this thesis. In addition I want to thank the whole Wuppertal group for the friendly working atmosphere. I also thank all my co-authors for the joint work in the various projects. Special thanks I want to say to Lukas Varnhorst and my family for their support throughout my whole studies. I gratefully acknowledge the Gauss Centre for Supercomputing (GCS) for providing computing time for a GCS Large-Scale Project on the GCS share of the supercomputer JUQUEEN [1] at Julich¨ Supercomputing Centre (JSC). GCS is the alliance of the three national supercomputing centres HLRS (Universit¨at Stuttgart), JSC (Forschungszentrum Julich),¨ and LRZ (Bayerische Akademie der Wissenschaften), funded by the German Federal Ministry of Education and Research (BMBF) and the German State Ministries for Research of Baden-Wurttemberg¨ (MWK), Bayern (StMWFK) and Nordrhein-Westfalen (MIWF). -
STATUS of the THEORY of QCD PLASMA BL1L—3 52 94 Joseph I, Kapusta Physics Department Brookhaven National Laboratory Upton, New York 11973
BNL-35294 STATUS OF THE THEORY OF QCD PLASMA BL1L—3 52 94 Joseph I, Kapusta Physics Department Brookhaven National Laboratory Upton, New York 11973 DISCLAIMER This report was prepared as an account of work sponsored hy an agency of the United States Government Neither the United States Government nor any agency thereof, nor any of thair employees, makes any warranty, express or implied, or assumes any legal liability or responsi- bility for the accuracy, completeness, or usefulness of any information, apparatus, product, or process disclosed, or represents that its use would not infringe privately owned rights. Refer- ence herein to any specific commercial product, process, or service by trade name, trademark, manufacturer, or otherwise does not necessarily constitute or imply its endorsement, recom- mendation, or favoring by the United States Government or any agency thereof. The views and opinions of authors expressed herein do not necessarily state or reflect those of the United States Government or any agency thereof. *Pennanent address: School of Physics and Astronomy, University of Minnesota, Minneapolis, Minnesota 55455 The submitted manuscript has been authored under contract DE-AC02-76CH00016 with the U.S. Department of Energy. Accordingly, the U.S. Government retains a nonexclusive, royalty-free license to publish or reproduce the published form of this contribution, or allow others to do so, for U.S. Government purposes. DJSTR/BUTION OF 7H/S OOCWMENr IS UNLIMITED STATUS OF THE THEORY OF QCD PLASMA Joseph I. Kapusta Physics Department Brookhaven National Laboratory Upton, New York 11973 ABSTRACT There is mounting evidence, based on many theoretical approaches, that color is deconfined and chiral symmetry is restored at temperatures greater Chan about 200 MeV. -
Excited Hadron States and the Deconfinement Transition
Excited Hadron States and the Deconfinement Transition Concluding Discussion Berndt Müller (Duke University) Workshop*) JLab - February 23-25, 2011 Friday, February 25, 2011 If we would hold a follow-up workshop in 2 years from now, which questions would we like to be answered? 2 Friday, February 25, 2011 Which QCD model describes the hadron (meson, baryon) spectrum best? E.g.: Constituent quark model MIT bag model Flux-tube model Holographic dual models Large Nc expansion Is there a “constituent gluon” model? If yes, how do we understand the large gluon mass? Scale breaking by the trace anomaly? Additional spontaneous scale invariance breaking? Is the constituent gluon a flux tube excitation? 3 Friday, February 25, 2011 What is the relation between the deconfinement transition and the chiral transition? Is it a well defined question? Are they at the “same” temperature? Do they drive each other? Where (at what T) and why does the hadron resonance gas model fail? Do unknown hadron states (hybrids, tetraquarks, glueballs) contribute significantly in the range of validity? If yes, which ones? 4 Friday, February 25, 2011 What are the requirements for a valid description of the hadronic break-up of the quark-gluon plasma? How must viscous hydrodynamics be matched to a kinetic description of the hadron gas? What are the minimal matching conditions? In which temperature range can the matching be performed? What are the most sensitive experimental tests? Where does the hot glue in the quark-gluon plasma go? Does it fragment into quark pairs? Does it initially end up in gluonic excitations? Is it possible to measure the average amount of excited glue in hadrons for a given mass or temperature on the lattice? 5 Friday, February 25, 2011 Can finite temperature lattice calculations determine average aspects of the hadron spectrum? Analogy with the Monte-Carlo shell model of Koonin, Ormand, Dean, Langanke, et al, who used MC methods to obtain level densities and Gamov-Teller strengths in the shell model for complex nuclei (e.g. -
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FEATURES in the past. This effect is ascribed to dark energy which acceleratt;s About the author the expansion. Erik H0g, Copenhagen University Observatory, has been involved Dark matter and dark energy are just convenient names used in the European efforts in space astrometrysince the earliest stud by astronomers when speaking ofthe large velocities seen in the ies in the 1970s. In 1999 he received "The Director ofScience motion ofvisible matter in the universe. It is the great challenge for Medal,for outstanding contribution to the science programme" ofthe present astronomy and physics to understand the true physical European Space Agency nature ofdark matter and dark energy. Finally some conclusions. The entire universe has probably a Bibliography finite volume, being slightly curved through the presence ofvisible Dreyer, J.L.E. 1953, A History ofAstronomyfrom Thales to Kepler, Dover and dark matter, and ofdark energy. The universe will probably Publications, Inc. expand forever and will do so faster and faster because ofthe pres Pedersen, Olaf 1992, The Book ofNature, Vatican Observatory Publications ence ofdark energy. Pedersen, Olaf 1993, Early Physics and Astronomy, A Historical Introduc tion, Cambridge University Press Acknowledgements The author is very grateful to Ulrich Bastian, Leif Hansen, Aase Stephenson, Bruce 1994, The Music ofthe Heavens, Kepler's Harmonic H0g, Bo Jacoby, Igor Novikov, and Kristian Pedersen for discus Astronomy, Princeton University Press sions and many useful comments on style and content ofprevious Van Helden, Albert 1985, Measuring the Universe, Cosmic Dimensions versions ofthis article. from Aristarchus to Halley, The University ofChicago Press WMAP 2003, Wilkinson Microwave Anisotropy Probe, http://map.gsfc.nasa.gov contribution to the validation ofthe EWT has been invaluable. -
Life Above the Hagedorn Temperature Quark-Gluon Plasma at SPS, RHIC & LHC
Life Above the Hagedorn Temperature Quark-Gluon Plasma at SPS, RHIC & LHC Berndt Mueller Brookhaven National Laboratory & Duke University Hagedorn Symposium CERN 13 November 2015 1965 was a momentous year cosmic microwave background Hagedorn mass spectrum 2 2015 almost unimaginable progress RHIC 3He+Au Planck: cosmological parameters PHENIX: QGP in p/d/3He+Au 3 Three things are needed… …to reach the summit: good equipment, good strategy, determination. In the study of hot, dense QCD matter this means: • High luminosity colliders • Large acceptance, high DAQ rate detectors with good particle ID • Realistic lattice QCD for thermo- dynamic quantities • Realistic transport codes • Weak (pQCD) and strong (AdS/CFT) coupling dynamical models • Multivariate model-data comparison After several decades of experimental and theoretical development, the necessary tools are now all in place. 4 The Relativistic Heavy Ion Collider …is hexagonal and 3.8 km long RHIC-AGS Complex at BNL 5 The Relativistic Heavy Ion Collider …is hexagonal and 3.8 km long RHIC-AGS Complex at BNL 5 The highest energies… 6 The highest energies… CMS ATLAS 6 Equation of State of QCD Matter 7 Equation of State EOS of flowing matter has conservative and dissipative contributions: (cons) (diss) Tµν = Tµν + Tµν = (ε + p)uµuν − pgµν 2 α α +η(∂µ uν + ∂ν uµ − 3 gµν ∂α u ) +ζ gµν ∂α u α When ζ(∂αu ) > p, the matter becomes unstable and cavitates. In general, Tµν is a dynamical quantity that relaxes to its equilibrium value on a time scale τπ that itself is related to the viscosity. While the shear viscosity η has a lower quantum bound, the bulk viscosity ζ vanishes for conformally invariant matter. -
Strangeness and the Quark-Gluon Plasma: Thirty Years of Discovery∗
Vol. 43 (2012) ACTA PHYSICA POLONICA B No 4 STRANGENESS AND THE QUARK-GLUON PLASMA: THIRTY YEARS OF DISCOVERY∗ Berndt Müller Department of Physics, Duke University, Durham, NC 27708, USA (Received December 27, 2011) I review the role of strange quarks as probes of hot QCD matter. DOI:10.5506/APhysPolB.43.761 PACS numbers: 12.38.Mh, 25.75.Nq, 25.75.Dw 1. The quark-gluon plasma: a strange state of matter Strange quarks play a crucial role in shaping the phase diagram of QCD matter (see Fig.1): • The mass ms of the strange quark controls the nature of the chiral and deconfinement transition in baryon symmetric QCD matter [1]. As a consequence, ms also influences the position of the critical point in the QCD phase diagram, if one exists. • The mass of the strange quark has an important effect on the stability limit of neutron stars and on the possible existence of a quark core in collapsed stars [2]. • Strange quarks enable the formation of a color–flavor locked, color superconducting quark matter phase at high baryon chemical potential and low temperature by facilitating the symmetry breaking SU(3)F × SU(3)C ! SU(3)F +C [3]. Strange quarks are also excellent probes of the structure of QCD matter because: • they are hard to produce at temperatures below Tc since their effective mass is much larger than Tc when chiral symmetry is broken, but easy to produce at temperatures above Tc since the current mass of the strange quark ms ≈ 100 MeV < Tc; ∗ Presented at the Conference “Strangeness in Quark Matter 2011”, Kraków, Poland, September 18–24, 2011.