Measurements of Upsilon Meson Suppression in Heavy Ion Collisions with the CMS Experiment at the LHC Nicolas Filipovic
Total Page:16
File Type:pdf, Size:1020Kb
Load more
Recommended publications
-
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 . -
Decays of the Tau Lepton*
SLAC - 292 UC - 34D (E) DECAYS OF THE TAU LEPTON* Patricia R. Burchat Stanford Linear Accelerator Center Stanford University Stanford, California 94305 February 1986 Prepared for the Department of Energy under contract number DE-AC03-76SF00515 Printed in the United States of America. Available from the National Techni- cal Information Service, U.S. Department of Commerce, 5285 Port Royal Road, Springfield, Virginia 22161. Price: Printed Copy A07, Microfiche AOl. JC Ph.D. Dissertation. Abstract Previous measurements of the branching fractions of the tau lepton result in a discrepancy between the inclusive branching fraction and the sum of the exclusive branching fractions to final states containing one charged particle. The sum of the exclusive branching fractions is significantly smaller than the inclusive branching fraction. In this analysis, the branching fractions for all the major decay modes are measured simultaneously with the sum of the branching fractions constrained to be one. The branching fractions are measured using an unbiased sample of tau decays, with little background, selected from 207 pb-l of data accumulated with the Mark II detector at the PEP e+e- storage ring. The sample is selected using the decay products of one member of the r+~- pair produced in e+e- annihilation to identify the event and then including the opposite member of the pair in the sample. The sample is divided into subgroups according to charged and neutral particle multiplicity, and charged particle identification. The branching fractions are simultaneously measured using an unfold technique and a maximum likelihood fit. The results of this analysis indicate that the discrepancy found in previous experiments is possibly due to two sources. -
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. -
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. -
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. -
J. Stroth Asked the Question: "Which Are the Experimental Evidences for a Long Mean Free Path of Phi Mesons in Medium?"
J. Stroth asked the question: "Which are the experimental evidences for a long mean free path of phi mesons in medium?" Answer by H. Stroebele ~~~~~~~~~~~~~~~~~~~ (based on the study of several publications on phi production and information provided by the theory friends of H. Stöcker ) Before trying to find an answer to this question, we need to specify what is meant with "long". The in medium cross section is equivalent to the mean free path. Thus we need to find out whether the (in medium) cross section is large (with respect to what?). The reference would be the cross sections of other mesons like pions or more specifically the omega meson. There is a further reference, namely the suppression of phi production and decay described in the OZI rule. A “blind” application of the OZI rule would give a cross section of the phi three orders of magnitude lower than that of the omega meson and correspondingly a "long" free mean path. In the following we shall look at the phi production cross sections in photon+p, pion+p, and p+p interactions. The total photoproduction cross sections of phi and omega mesons were measured in a bubble chamber experiment (J. Ballam et al., Phys. Rev. D 7, 3150, 1973), in which a cross section ratio of R(omega/phi) = 10 was found in the few GeV beam energy region. There are results on omega and phi production in p+p interactions available from SPESIII (Near- Threshold Production of omega mesons in the Reaction p p → p p omega", Phys.Rev.Lett. -
Detection of a Hypercharge Axion in ATLAS
Detection of a Hypercharge Axion in ATLAS a Monte-Carlo Simulation of a Pseudo-Scalar Particle (Hypercharge Axion) with Electroweak Interactions for the ATLAS Detector in the Large Hadron Collider at CERN Erik Elfgren [email protected] December, 2000 Division of Physics Lule˚aUniversity of Technology Lule˚a, SE-971 87, Sweden http://www.luth.se/depts/mt/fy/ Abstract This Master of Science thesis treats the hypercharge axion, which is a hy- pothetical pseudo-scalar particle with electroweak interactions. First, the theoretical context and the motivations for this study are discussed. In short, the hypercharge axion is introduced to explain the dominance of matter over antimatter in the universe and the existence of large-scale magnetic fields. Second, the phenomenological properties are analyzed and the distin- guishing marks are underlined. These are basically the products of photons and Z0swithhightransversemomentaandinvariantmassequaltothatof the axion. Third, the simulation is carried out with two photons producing the axion which decays into Z0s and/or photons. The event simulation is run through the simulator ATLFAST of ATLAS (A Toroidal Large Hadron Col- lider ApparatuS) at CERN. Finally, the characteristics of the axion decay are analyzed and the crite- ria for detection are presented. A study of the background is also included. The result is that for certain values of the axion mass and the mass scale (both in the order of a TeV), the hypercharge axion could be detected in ATLAS. Preface This is a Master of Science thesis at the Lule˚a University of Technology, Sweden. The research has been done at Universit´edeMontr´eal, Canada, under the supervision of Professor Georges Azuelos. -
J = Τ MASS Page 1
Citation: P.A. Zyla et al. (Particle Data Group), Prog. Theor. Exp. Phys. 2020, 083C01 (2020) J 1 τ = 2 + + τ discovery paper was PERL 75. e e− → τ τ− cross-section threshold behavior and magnitude are consistent with pointlike spin- 1/2 Dirac particle. BRANDELIK 78 ruled out pointlike spin-0 or spin-1 particle. FELDMAN 78 ruled out J = 3/2. KIRKBY 79 also ruled out J=integer, J = 3/2. τ MASS VALUE (MeV) EVTS DOCUMENT ID TECN COMMENT 1776..86 0..12 OUR AVERAGE ± +0.10 1776.91 0.12 1171 1 ABLIKIM 14D BES3 23.3 pb 1, Eee = ± 0.13 − cm − 3.54–3.60 GeV 1776.68 0.12 0.41 682k 2 AUBERT 09AK BABR 423 fb 1, Eee =10.6 GeV ± ± − cm 1776.81+0.25 0.15 81 ANASHIN 07 KEDR 6.7 pb 1, Eee = 0.23 ± − cm − 3.54–3.78 GeV 1776.61 0.13 0.35 2 BELOUS 07 BELL 414 fb 1 Eee =10.6 GeV ± ± − cm 1775.1 1.6 1.0 13.3k 3 ABBIENDI 00A OPAL 1990–1995 LEP runs ± ± 1778.2 0.8 1.2 ANASTASSOV 97 CLEO Eee = 10.6 GeV ± ± cm . +0.18 +0.25 4 Eee . 1776 96 0.21 0.17 65 BAI 96 BES cm= 3 54–3 57 GeV − − 1776.3 2.4 1.4 11k 5 ALBRECHT 92M ARG Eee = 9.4–10.6 GeV ± ± cm +3 6 Eee 1783 4 692 BACINO 78B DLCO cm= 3.1–7.4 GeV − We do not use the following data for averages, fits, limits, etc. -
Understanding the J/Psi Production Mechanism at PHENIX Todd Kempel Iowa State University
Iowa State University Capstones, Theses and Graduate Theses and Dissertations Dissertations 2010 Understanding the J/psi Production Mechanism at PHENIX Todd Kempel Iowa State University Follow this and additional works at: https://lib.dr.iastate.edu/etd Part of the Physics Commons Recommended Citation Kempel, Todd, "Understanding the J/psi Production Mechanism at PHENIX" (2010). Graduate Theses and Dissertations. 11649. https://lib.dr.iastate.edu/etd/11649 This Dissertation is brought to you for free and open access by the Iowa State University Capstones, Theses and Dissertations at Iowa State University Digital Repository. It has been accepted for inclusion in Graduate Theses and Dissertations by an authorized administrator of Iowa State University Digital Repository. For more information, please contact [email protected]. Understanding the J= Production Mechanism at PHENIX by Todd Kempel A dissertation submitted to the graduate faculty in partial fulfillment of the requirements for the degree of DOCTOR OF PHILOSOPHY Major: Nuclear Physics Program of Study Committee: John G. Lajoie, Major Professor Kevin L De Laplante S¨orenA. Prell J¨orgSchmalian Kirill Tuchin Iowa State University Ames, Iowa 2010 Copyright c Todd Kempel, 2010. All rights reserved. ii TABLE OF CONTENTS LIST OF TABLES . v LIST OF FIGURES . vii CHAPTER 1. Overview . 1 CHAPTER 2. Quantum Chromodynamics . 3 2.1 The Standard Model . 3 2.2 Quarks and Gluons . 5 2.3 Asymptotic Freedom and Confinement . 6 CHAPTER 3. The Proton . 8 3.1 Cross-Sections and Luminosities . 8 3.2 Deep-Inelastic Scattering . 10 3.3 Structure Functions and Bjorken Scaling . 12 3.4 Altarelli-Parisi Evolution . -
Download This Article in PDF Format
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. -
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. -
Arxiv:1403.4425V1 [Hep-Ex] 18 Mar 2014 and Strong
July 30, 2018 7:30 Brief history for the search and discovery of the Higgs particle – A personal perspective Sau Lan Wu Department of Physics, University of Wisconsin, Madison, WI 53706, USA [email protected] In 1964, a new particle was proposed by several groups to answer the question of where the masses of elementary particles come from; this particle is usually referred to as the Higgs particle or the Higgs boson. In July 2012, this Higgs particle was finally found experimentally, a feat accomplished by the ATLAS Collaboration and the CMS Col- laboration using the Large Hadron Collider at CERN. It is the purpose of this review to give my personal perspective on a brief history of the experimental search for this particle since the ’80s and finally its discovery in 2012. Besides the early searches, those at the LEP collider at CERN, the Tevatron Collider at Fermilab, and the Large Hadron Collider at CERN are described in some detail. This experimental discovery of the Higgs boson is often considered to be the most important advance in particle physics in the last half a century, and some of the possible implications are briefly discussed. This review is partially based on a talk presented by the author at the conference “Higgs Quo Vadis,” Aspen Center for Physics, Aspen, CO, USA, March 10-15, 2013. Keywords: Higgs boson; standard model; Large Hadron Collider; Higgs discovery. PACS Nos.: 14.80.Bn, 13.85.-t, 13.66.Fg, 12.60.-i 1. Introduction 1.1. Fundamental interaction and gauge particles There are four types of interactions in nature: gravitational, weak, electromagnetic arXiv:1403.4425v1 [hep-ex] 18 Mar 2014 and strong.