The Dirac Spectrum and the BEC-BCS Crossover in QCD at Nonzero Isospin Asymmetry
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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. -
Particle Physics Dr Victoria Martin, Spring Semester 2012 Lecture 12: Hadron Decays
Particle Physics Dr Victoria Martin, Spring Semester 2012 Lecture 12: Hadron Decays !Resonances !Heavy Meson and Baryons !Decays and Quantum numbers !CKM matrix 1 Announcements •No lecture on Friday. •Remaining lectures: •Tuesday 13 March •Friday 16 March •Tuesday 20 March •Friday 23 March •Tuesday 27 March •Friday 30 March •Tuesday 3 April •Remaining Tutorials: •Monday 26 March •Monday 2 April 2 From Friday: Mesons and Baryons Summary • Quarks are confined to colourless bound states, collectively known as hadrons: " mesons: quark and anti-quark. Bosons (s=0, 1) with a symmetric colour wavefunction. " baryons: three quarks. Fermions (s=1/2, 3/2) with antisymmetric colour wavefunction. " anti-baryons: three anti-quarks. • Lightest mesons & baryons described by isospin (I, I3), strangeness (S) and hypercharge Y " isospin I=! for u and d quarks; (isospin combined as for spin) " I3=+! (isospin up) for up quarks; I3="! (isospin down) for down quarks " S=+1 for strange quarks (additive quantum number) " hypercharge Y = S + B • Hadrons display SU(3) flavour symmetry between u d and s quarks. Used to predict the allowed meson and baryon states. • As baryons are fermions, the overall wavefunction must be anti-symmetric. The wavefunction is product of colour, flavour, spin and spatial parts: ! = "c "f "S "L an odd number of these must be anti-symmetric. • consequences: no uuu, ddd or sss baryons with total spin J=# (S=#, L=0) • Residual strong force interactions between colourless hadrons propagated by mesons. 3 Resonances • Hadrons which decay due to the strong force have very short lifetime # ~ 10"24 s • Evidence for the existence of these states are resonances in the experimental data Γ2/4 σ = σ • Shape is Breit-Wigner distribution: max (E M)2 + Γ2/4 14 41. -
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. -
Electro-Weak Interactions
Electro-weak interactions Marcello Fanti Physics Dept. | University of Milan M. Fanti (Physics Dep., UniMi) Fundamental Interactions 1 / 36 The ElectroWeak model M. Fanti (Physics Dep., UniMi) Fundamental Interactions 2 / 36 Electromagnetic vs weak interaction Electromagnetic interactions mediated by a photon, treat left/right fermions in the same way g M = [¯u (eγµ)u ] − µν [¯u (eγν)u ] 3 1 q2 4 2 1 − γ5 Weak charged interactions only apply to left-handed component: = L 2 Fermi theory (effective low-energy theory): GF µ 5 ν 5 M = p u¯3γ (1 − γ )u1 gµν u¯4γ (1 − γ )u2 2 Complete theory with a vector boson W mediator: g 1 − γ5 g g 1 − γ5 p µ µν p ν M = u¯3 γ u1 − 2 2 u¯4 γ u2 2 2 q − MW 2 2 2 g µ 5 ν 5 −−−! u¯3γ (1 − γ )u1 gµν u¯4γ (1 − γ )u2 2 2 low q 8 MW p 2 2 g −5 −2 ) GF = | and from weak decays GF = (1:1663787 ± 0:0000006) · 10 GeV 8 MW M. Fanti (Physics Dep., UniMi) Fundamental Interactions 3 / 36 Experimental facts e e Electromagnetic interactions γ Conserves charge along fermion lines ¡ Perfectly left/right symmetric e e Long-range interaction electromagnetic µ ) neutral mass-less mediator field A (the photon, γ) currents eL νL Weak charged current interactions Produces charge variation in the fermions, ∆Q = ±1 W ± Acts only on left-handed component, !! ¡ L u Short-range interaction L dL ) charged massive mediator field (W ±)µ weak charged − − − currents E.g. -
Introduction to Flavour Physics
Introduction to flavour physics Y. Grossman Cornell University, Ithaca, NY 14853, USA Abstract In this set of lectures we cover the very basics of flavour physics. The lec- tures are aimed to be an entry point to the subject of flavour physics. A lot of problems are provided in the hope of making the manuscript a self-study guide. 1 Welcome statement My plan for these lectures is to introduce you to the very basics of flavour physics. After the lectures I hope you will have enough knowledge and, more importantly, enough curiosity, and you will go on and learn more about the subject. These are lecture notes and are not meant to be a review. In the lectures, I try to talk about the basic ideas, hoping to give a clear picture of the physics. Thus many details are omitted, implicit assumptions are made, and no references are given. Yet details are important: after you go over the current lecture notes once or twice, I hope you will feel the need for more. Then it will be the time to turn to the many reviews [1–10] and books [11, 12] on the subject. I try to include many homework problems for the reader to solve, much more than what I gave in the actual lectures. If you would like to learn the material, I think that the problems provided are the way to start. They force you to fully understand the issues and apply your knowledge to new situations. The problems are given at the end of each section. -
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. -
Lecture 5: Quarks & Leptons, Mesons & Baryons
Physics 3: Particle Physics Lecture 5: Quarks & Leptons, Mesons & Baryons February 25th 2008 Leptons • Quantum Numbers Quarks • Quantum Numbers • Isospin • Quark Model and a little History • Baryons, Mesons and colour charge 1 Leptons − − − • Six leptons: e µ τ νe νµ ντ + + + • Six anti-leptons: e µ τ νe̅ νµ̅ ντ̅ • Four quantum numbers used to characterise leptons: • Electron number, Le, muon number, Lµ, tau number Lτ • Total Lepton number: L= Le + Lµ + Lτ • Le, Lµ, Lτ & L are conserved in all interactions Lepton Le Lµ Lτ Q(e) electron e− +1 0 0 1 Think of Le, Lµ and Lτ like − muon µ− 0 +1 0 1 electric charge: − tau τ − 0 0 +1 1 They have to be conserved − • electron neutrino νe +1 0 0 0 at every vertex. muon neutrino νµ 0 +1 0 0 • They are conserved in every tau neutrino ντ 0 0 +1 0 decay and scattering anti-electron e+ 1 0 0 +1 anti-muon µ+ −0 1 0 +1 anti-tau τ + 0 −0 1 +1 Parity: intrinsic quantum number. − electron anti-neutrino ν¯e 1 0 0 0 π=+1 for lepton − muon anti-neutrino ν¯µ 0 1 0 0 π=−1 for anti-leptons tau anti-neutrino ν¯ 0 −0 1 0 τ − 2 Introduction to Quarks • Six quarks: d u s c t b Parity: intrinsic quantum number • Six anti-quarks: d ̅ u ̅ s ̅ c ̅ t ̅ b̅ π=+1 for quarks π=−1 for anti-quarks • Lots of quantum numbers used to describe quarks: • Baryon Number, B - (total number of quarks)/3 • B=+1/3 for quarks, B=−1/3 for anti-quarks • Strangness: S, Charm: C, Bottomness: B, Topness: T - number of s, c, b, t • S=N(s)̅ −N(s) C=N(c)−N(c)̅ B=N(b)̅ −N(b) T=N( t )−N( t )̅ • Isospin: I, IZ - describe up and down quarks B conserved in all Quark I I S C B T Q(e) • Z interactions down d 1/2 1/2 0 0 0 0 1/3 up u 1/2 −1/2 0 0 0 0 +2− /3 • S, C, B, T conserved in strange s 0 0 1 0 0 0 1/3 strong and charm c 0 0 −0 +1 0 0 +2− /3 electromagnetic bottom b 0 0 0 0 1 0 1/3 • I, IZ conserved in strong top t 0 0 0 0 −0 +1 +2− /3 interactions only 3 Much Ado about Isospin • Isospin was introduced as a quantum number before it was known that hadrons are composed of quarks. -
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.