High Density Quark Matter and Color Superconductivity
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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. -
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]. -
Surprises from the Search for Quark-Gluon Plasma?* When Was Quark-Gluon Plasma Seen?
Surprises from the search for quark-gluon plasma?* When was quark-gluon plasma seen? Richard M. Weiner Laboratoire de Physique Théorique, Univ. Paris-Sud, Orsay and Physics Department, University of Marburg The historical context of the recent results from high energy heavy ion reactions devoted to the search of quark-gluon plasma (QGP) is reviewed, with emphasis on the surprises encountered. The evidence for QGP from heavy ion reactions is compared with that available from particle reactions. Keywords: Quark-Gluon plasma in particle and nuclear reactions, hydrodynamics, equation of state, confinement, superfluidity. 1. Evidence for QGP in the Pre-SPS Era Particle Physics 1.1 The mystery of the large number of degrees of freedom 1.2 The equation of state 1.2.1 Energy dependence of the multiplicity 1.2.2 Single inclusive distributions Rapidity and transverse momentum distributions Large transverse momenta 1.2.3 Multiplicity distributions 1.3 Global equilibrium: the universality of the hadronization process 1.3.1 Inclusive distributions 1.3.2 Particle ratios -------------------------------------------------------------------------------------- *) Invited Review 1 Heavy ion reactions A dependence of multiplicity Traces of QGP in low energy heavy ion reactions? 2. Evidence for QGP in the SPS-RHIC Era 2.1 Implications of observations at SPS for RHIC 2.1.1 Role of the Equation of State in the solutions of the equations of hydrodynamics 2.1.2 Longitudinal versus transverse expansion 2.1.3 Role of resonances in Bose-Einstein interferometry; the Rout/Rside ratio 2.2 Surprises from RHIC? 2.2.1 HBT puzzle? 2.2.2 Strongly interacting quark-gluon plasma? Superfluidity and chiral symmetry Confinement and asymptotic freedom Outlook * * * In February 2000 spokespersons from the experiments on CERN’s Heavy Ion programme presented “compelling evidence for the existence of a new state of matter in which quarks, instead of being bound up into more complex particles such as protons and neutrons, are liberated to roam freely…”1. -
Diffractive Dissociation of Alpha Particles As a Test of Isophobic Short-Range Correlations Inside Nuclei ∗ Jennifer Rittenhouse West A, , Stanley J
Physics Letters B 805 (2020) 135423 Contents lists available at ScienceDirect Physics Letters B www.elsevier.com/locate/physletb Diffractive dissociation of alpha particles as a test of isophobic short-range correlations inside nuclei ∗ Jennifer Rittenhouse West a, , Stanley J. Brodsky a, Guy F. de Téramond b, Iván Schmidt c a SLAC National Accelerator Laboratory, Stanford University, Stanford, CA 94309, USA b Laboratorio de Física Teórica y Computacional, Universidad de Costa Rica, 11501 San José, Costa Rica c Departamento de Física y Centro Científico Tecnológico de Valparáiso-CCTVal, Universidad Técnica Federico Santa María, Casilla 110-V, Valparaíso, Chile a r t i c l e i n f o a b s t r a c t Article history: The CLAS collaboration at Jefferson Laboratory has compared nuclear parton distributions for a range Received 15 January 2020 of nuclear targets and found that the EMC effect measured in deep inelastic lepton-nucleus scattering Received in revised form 9 April 2020 has a strongly “isophobic” nature. This surprising observation suggests short-range correlations between Accepted 9 April 2020 neighboring n and p nucleons in nuclear wavefunctions that are much stronger compared to p − p or n − Available online 14 April 2020 n correlations. In this paper we propose a definitive experimental test of the nucleon-nucleon explanation Editor: W. Haxton of the isophobic nature of the EMC effect: the diffractive dissociation on a nuclear target A of high energy 4 He nuclei to pairs of nucleons n and p with high relative transverse momentum, α + A → n + p + A + X. The comparison of n − p events with p − p and n − n events directly tests the postulated breaking of isospin symmetry. -
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. -
Unit VI Superconductivity JIT Nashik Contents
Unit VI Superconductivity JIT Nashik Contents 1 Superconductivity 1 1.1 Classification ............................................. 1 1.2 Elementary properties of superconductors ............................... 2 1.2.1 Zero electrical DC resistance ................................. 2 1.2.2 Superconducting phase transition ............................... 3 1.2.3 Meissner effect ........................................ 3 1.2.4 London moment ....................................... 4 1.3 History of superconductivity ...................................... 4 1.3.1 London theory ........................................ 5 1.3.2 Conventional theories (1950s) ................................ 5 1.3.3 Further history ........................................ 5 1.4 High-temperature superconductivity .................................. 6 1.5 Applications .............................................. 6 1.6 Nobel Prizes for superconductivity .................................. 7 1.7 See also ................................................ 7 1.8 References ............................................... 8 1.9 Further reading ............................................ 10 1.10 External links ............................................. 10 2 Meissner effect 11 2.1 Explanation .............................................. 11 2.2 Perfect diamagnetism ......................................... 12 2.3 Consequences ............................................. 12 2.4 Paradigm for the Higgs mechanism .................................. 12 2.5 See also ............................................... -
Surface Pair-Density-Wave Superconducting and Superfluid States
Surface Pair-Density-Wave Superconducting and Superfluid States Mats Barkman,1 Albert Samoilenka,1 and Egor Babaev1 1Department of Physics, Royal Institute of Technology, SE-106 91 Stockholm, Sweden Fulde, Ferrell, Larkin, and Ovchinnikov (FFLO) predicted inhomogeneous superconducting and superfluid ground states, spontaneously breaking translation symmetries. In this Letter, we demon- strate that the transition from the FFLO to the normal state as a function of temperature or increased Fermi surface splitting is not a direct one. Instead the system has an additional phase transition to a different state where pair-density-wave superconductivity (or superfluidity) exists only on the boundaries of the system, while the bulk of the system is normal. The surface pair- density-wave state is very robust and exists for much larger fields and temperatures than the FFLO state. In regular BCS theory, the formation of Cooper pairs The Ginzburg-Landau description of superconductors binding together two electrons with opposite spin and op- in the presence of Zeeman splitting was derived from mi- posite momentum results in a uniform superconducting croscopic theory in Ref. [31]. The free energy functional state [1,2]. In 1964, Fulde and Ferrell [3] and Larkin and R d reads F [ ] = Ω d x where the free energy density is Ovchinnikov [4] (FFLO) independently predicted that F F under certain conditions there should appear an inho- =α 2 + β 2 + γ 4 + δ 2 2+ mogeneous state in the presence of a strong magnetic F j j jr jµ j j jr j (1) µ 2 2 + ( ∗)2( )2 + c.c. + ν 6; field, where Zeeman splitting of the Fermi surfaces leads j j jr j 8 r j j to the formation of Cooper pairs with nonzero total mo- mentum. -
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. -
Three-Flavor Color Superconductivity
Three-Flavor Color Superconductivity Dissertation zur Erlangung des Doktorgrades der Naturwissenschaften vorgelegt beim Fachbereich Physik der Johann Wolfgang Goethe-Universit¨at in Frankfurt am Main von Hossein Malekzadeh aus dem Iran Frankfurt am Main, Dezember 2007 (D 30) 2 vom Fachbereich Physik der Johann Wolfgang Goethe–Universit¨at als Dissertation angenommen. Dekan: Prof. Dr. W. Aßmus Gutachter: Prof. Dr. D.-H. Rischke, Prof. Dr. Adrian Dumitru Datum der Disputation: Dezember 7, 2007. Acknowledgements I would like to express my special thanks to Prof. Dirk Rischke for all the generous supports that during my Ph.D thesis he gave mentally and practically to me. I learned a lot of things from him which will be certainly very useful for me in future as well. Without his helps and encouragements it would be difficult to come to the end of this thesis. Thank you Dirk! I am also very grateful to Prof. Igor Shovkovy for very instructive discussions we had. He was the one who taught this stimulating field to me. Also, I had a lot of fun with him during lunch breaks and in other occasions. Since I wanted to take ten watermelons with my tow hands, I needed to work harder. On other words, along my Ph.D thesis, I wanted to work on other fields as well, although the project were not published. I had great times when I was collaborating with Prof. Adrian Dumitru and Prof. Michael Strickland. I thank both of you for teaching me those fascinating topics. I also had a wonderful chance to talk to Prof. -
Arxiv:1707.04966V3 [Astro-Ph.HE] 17 Dec 2017
From hadrons to quarks in neutron stars: a review Gordon Baym,1, 2, 3 Tetsuo Hatsuda,2, 4, 5 Toru Kojo,6, 1 Philip D. Powell,1, 7 Yifan Song,1 and Tatsuyuki Takatsuka5, 8 1Department of Physics, University of Illinois at Urbana-Champaign, 1110 W. Green Street, Urbana, Illinois 61801, USA 2iTHES Research Group, RIKEN, Wako, Saitama 351-0198, Japan 3The Niels Bohr International Academy, The Niels Bohr Institute, University of Copenhagen, Blegdamsvej 17, DK-2100 Copenhagen Ø, Denmark 4iTHEMS Program, RIKEN, Wako, Saitama 351-0198, Japan 5Theoretical Research Division, Nishina Center, RIKEN, Wako 351-0198, Japan 6Key Laboratory of Quark and Lepton Physics (MOE) and Institute of Particle Physics, Central China Normal University, Wuhan 430079, China 7Lawrence Livermore National Laboratory, 7000 East Ave., Livermore, CA 94550 8Iwate University, Morioka 020-8550, Japan (Dated: December 19, 2017) In recent years our understanding of neutron stars has advanced remarkably, thanks to research converging from many directions. The importance of understanding neutron star behavior and structure has been underlined by the recent direct detection of gravitational radiation from merging neutron stars. The clean identification of several heavy neutron stars, of order two solar masses, challenges our current understanding of how dense matter can be sufficiently stiff to support such a mass against gravitational collapse. Programs underway to determine simultaneously the mass and radius of neutron stars will continue to constrain and inform theories of neutron star interiors. At the same time, an emerging understanding in quantum chromodynamics (QCD) of how nuclear matter can evolve into deconfined quark matter at high baryon densities is leading to advances in understanding the equation of state of the matter under the extreme conditions in neutron star interiors.