Exotic Antimatter Detected at RHIC Denes Molnar the Goal of Gozar’Sgoaltheof Research Is Eluci Help Maydiscovery the Discovery Experimental “This on March 4,2010

Total Page:16

File Type:pdf, Size:1020Kb

Exotic Antimatter Detected at RHIC Denes Molnar the Goal of Gozar’Sgoaltheof Research Is Eluci Help Maydiscovery the Discovery Experimental “This on March 4,2010 the Vol. 64B - No. 11 ulletin April 2, 2010 Exotic Antimatter Detected at RHIC Scientists report discovery of heaviest known antinucleus — the first D0680809 containing an anti-strange quark — laying the first stake in a new frontier of physics An international team of scien- known as “strangeness,” which tists studying high-energy colli- depends on the presence of sions of gold ions at the Relativ- strange quarks. Nuclei contain- Joseph Rubino istic Heavy Ion Collider (RHIC), ing one or more strange quarks a 2.4-mile-circumference particle are called hypernuclei. ‘Communicating accelerator located at BNL, has For all ordinary matter, with Science’ published evidence of the most no strange quarks, the strange- massive antinucleus discovered ness value is zero and the chart Alan Alda to date. The new antinucleus, is flat. Hypernuclei appear above discovered at RHIC’s STAR detec- the plane of the chart. The new To Give Talk, 4/9 tor, is a negatively charged state discovery of strange antimatter At 9 a.m. on April 9 in Berkner of antimatter containing an with an antistrange quark (an Hall, Lab Director Sam Aronson antiproton, an antineutron, and antihypernucleus) marks the first Michael Herbert will welcome Alan Alda, the ac- an anti-Lambda particle. It is also entry below the plane. claimed actor and host of PBS’ the first antinucleus containing This study of the new antihy- “Scientific American Frontiers,” an anti-strange quark. The results pernucleus also yields a valuable and Howie Schneider, Dean of were published online by Science sample of normal hypernuclei, Express on March 4, 2010. and has implications for our Stony Brook University School of CN2-21-99 Journalism and one of the found- “This experimental discovery understanding of the structure of ers of its Center for Communicat- may have unprecedented con- collapsed stars. ing Science, to open a program on sequences for our view of the “The strangeness value could At the STAR Detector at Brookhaven Lab’s Relativistic Heavy Ion Collider, “Communicating Science.” After world,” commented theoretical be non-zero in the core of col- scientists recently detected the heaviest known antinucleus — the first Alda’s keynote speech, a panel physicist Horst Stoecker, Vice containing an anti-strange quark. lapsed stars,” said Jinhui Chen, of experts — including BNL’s Jo- President of the Helmholtz As- one of the lead authors, a post- anna Fowler — will discuss “Who sociation of German National mental asymmetries in the early cording to the number of protons, doctoral researcher at Kent State Cares What the Public Thinks Laboratories. “This antimatter universe. which determine each element’s University and currently a staff about Science?” Aronson encour- pushes open the door to new chemical properties. Physicists scientist at the Shanghai Insti- ages as many BNLers as possible dimensions in the nuclear chart — New Nuclear Terrain use a more complex, three-di- tute of Applied Physics, “so the to attend this event, which also an idea that a few years ago would All terrestrial nuclei are made of mensional chart to also convey present measurements at RHIC includes afternoon workshops on have been viewed as impossible.” protons and neutrons (which in information on the number of will help us distinguish between- science communication. The discovery may help eluci- turn contain only up and down neutrons, which may change in models that describe these exotic For agenda information, see date models of neutron stars and quarks). The standard periodic different isotopes of the same states of matter.” pg. 3 and www.bnl.gov/csw/. opens up exploration of funda- table of elements is arranged ac- element, and a quantum number See Antimatter on pg. 2 Four Scientists at BNL Honored Two Pegram Lectures, 4/12, 4/13 With DOE Early Career Research Grants Harvard’s Christopher Stubbs Will Discuss Dark Energy, Search For Novel Gravitational Effects Christopher Stubbs, Chair of the Physics Department at Harvard University, will give two George Roger Stoutenburgh Roger Stoutenburgh B. Pegram Lectures — April 12 and 13 — both at 4 p.m. in Berkner Hall. Inaugurated in 1959, the Pegram lectures bring distinguished scholars to the Laboratory to speak on topics of both scientific and general inter- D0870210 D3040110 est. Sponsored by Brookhaven Marivi Fernandez-Serra Adrian Gozar Science Associates, the lectures are free and open to the public. Adrian Gozar, an associate Visitors to the Lab age 16 and issue and scientific observations scientist in BNL’s Condensed over must bring a photo ID. about it. Matter Physics & Materials In his April 12 lecture, titled An experimental physicist, Science Department, and “Dark Energy: A Crisis for Fun- Stubbs’ interests include experi- three university scientists damental Physics,” Stubbs will mental tests of the foundations who use BNL’s facilities discuss the astrophysical observa- of gravitational physics, searches — Marivi Fernandez-Serra, tions that show that the current for dark matter, and observa- Denes Molnar and Feng picture of fundamental physics is tional cosmology. With a Ph.D. Yuan — have been chosen Denes Molnar far from complete. The discovery in physics from the University to receive five-year research in 1998 that the expansion of the of Washington (UW) in 1988, he grants under the DOE Early Adrian universe is accelerating presents worked at the University of Cali- Career Research Program. They Gozar physicists with a profound chal- fornia (UC), Berkeley, UC Santa are among 69 researchers from Adrian Gozar is lenge. According to the current Barbara, and UW before joining across the nation who will receive funded by the laws of physics, the expansion Harvard in 2003, where he was up to $85 million in funding Office of Basic Feng Yuan should be slowing down because named Physics Chair in 2007. under the American Recovery Energy Scienc- of the force of gravity. In fact, Stubbs’ numerous awards and Reinvestment Act. The new es for “Investigation of the role of Gozar will use specially de- it is expanding at an ever-faster include a 1993 R&D 100 Award program is designed to bolster the inhomogeneities and phase seg- signed optical spectroscopy and rate. A hypothetical force, known from R&D Magazine for inventing nation’s scientific workforce by regation on correlated electron nano-imaging techniques to as dark energy, is believed to be the MACHO camera digital imag- providing support to exceptional dynamics by optical spectroscopy probe materials at the scale of causing this expansion. ing system, used in the experi- researchers during their crucial and nano-imaging.” a nanometer, or a billionth of a This inability to understand mental search for dark matter. He early years, when many scientists The goal of Gozar’s research is meter. An understanding of the the expansion based on current was a Sloan Fellow 1993-95, and a do their most formative work. to understand the optical prop- structural properties of these ma- physics theory is known as the Packard Foundation Fellow, 1994- Under the program, univer- erties of correlated electronic terials as they transition between “dark energy” problem, and it 99. He received the 1996 National sity-based researchers will re- systems — systems that are on different phases is a crucial step is arguably the most pressing Academy of Sciences Award for ceive at least $150,000 per year the brink of several competing in determining if their function- open question in modern phys- Initiative in Research, then in to cover summer salary and instabilities, or phases. High-tem- al properties can be improved for ics. In his April 12 talk, Stubbs 1999 he became a Fellow of the research expenses. For research- perature superconductors and potential applications. will explain why the problem American Physical Society and ers based at DOE national colossal magnetoresistive oxides Gozar earned a B.S. and M.S. constitutes a crisis, with wide- a Centennial Fellow of the Mc- laboratories, grants will be at are examples of such systems. in physics from the University of reaching ramifications. Donnell Foundation. He was also least $500,000 per year to cover Gozar will investigate differences Bucharest, Romania, in 1997 and In the April 13 talk, titled honored with the NASA Achieve- year-round salary plus research in these materials at transitions 1998, respectively, and a Ph.D. “Searching for Novel Gravita- ment Medal, 2000, and the expenses. An overview of the between insulating, metallic and in physics from the University... tional Effects,” he will discuss Gruber Foundation Cosmology work of each winner follows: superconducting phases. See Early Career Grants on pg. 2 experiments that explore the Prize, 2007. — Diane Greenberg The Bulletin April 2, 2010 Hispanic Heritage Club Dr. Mow Shiah Lin Offers $500 Scholarships Scholarship Offered Safety: Making it Personal The BERA Hispanic Heritage Club is Applications are now being ac- “Personnel safety is personal,” accepting applications for five $500 cepted for the sixth Dr. Mow Shi- says Gerry Van Derlaske of scholarships for high-school seniors. ah Lin Scholarship, sponsored National Synchrotron Light Applicants should: Be a high by the Asian Pacific American Source II (NSLS-II). With these school senior graduating in 2010; Association (APAA) at BNL. The four words, Van Derlaske sums have a minimum 3.0 cumulative annual $1,000 scholarship was up his outlook on safety. GPA on a 4.0 scale (or equivalent); initiated to honor the late BNL Encounter Van Derlaske at be accepted by a college for fall scientist for whom it is named. large-group meetings or walk- 2010 classes to pursue a degree in In memory of Lin’s distin- ing through any of the director- science or engineering; be a Long guished research, achievements, ate’s 16 or so buildings and you Island resident attending Bellport, and inventions, the scholarship will hear a safety report, a safety Brentwood Union Free, Central is granted each year to an Asian tip, a safety warning, or a safety Islip, Longwood, Patchogue-Med- immigrant with a student visa story.
Recommended publications
  • The First Few Microseconds
    the first few MICROSSECONDSECONDS In recent experiments, physicists have replicated conditions of the infant universe— with startling results BY MICHAEL RIORDAN AND WILLIAM A. ZAJC or the past fi ve years, hundreds of scientists have been using a pow- erful new atom smasher at Brookhaven National Laboratory on Long Island to mimic conditions that existed at the birth of the uni- verse. Called the Relativistic Heavy Ion Collider (RHIC, pro- nounced “rick”), it clashes two opposing beams of gold nuclei trav- Feling at nearly the speed of light. The resulting collisions between pairs of these atomic nuclei generate exceedingly hot, dense bursts of matter and en- ergy to simulate what happened during the fi rst few microseconds of the big bang. These brief “mini bangs” give physicists a ringside seat on some of the earliest moments of creation. During those early moments, matter was an ultrahot, superdense brew of particles called quarks and gluons rushing hither and thither and crashing willy-nilly into one another. A sprinkling of electrons, photons and other light elementary particles seasoned the soup. This mixture had a temperature in the trillions of degrees, more than 100,000 times hotter than the sun’s core. But the temperature plummeted as the cosmos expanded, just like an or- dinary gas cools today when it expands rapidly. The quarks and gluons slowed down so much that some of them could begin sticking together briefl y. After nearly 10 microseconds had elapsed, the quarks and gluons became shackled together by strong forces between them, locked up permanently within pro- tons, neutrons and other strongly interacting particles that physicists collec- tively call “hadrons.” Such an abrupt change in the properties of a material is called a phase transition (like liquid water freezing into ice).
    [Show full text]
  • Charged Kaon Ratios and Yields Measured with the STAR Detector at the Relativistic Heavy Ion
    Charged Kaon Ratios and Yields Measured with the STAR Detector at the Relativistic Heavy Ion Collider By C.L. Kunz B.S. Chemistry, McPherson College, 1997 Submitted in Partial Fulfillment of the Requirement for the Degree of Doctor of Philosophy Department of Chemistry Carnegie Mellon University Pittsburgh, Pennsylvania 15213 September 2003 This thesis is dedicated to my parents for their guidance and support. They have long been two of my best friends. Without them, I would not be here. ii © Copyright 2003 by Christopher Lee Kunz All Rights Reserved iii Table of Contents TABLE OF CONTENTS ...............................................................................................IV LIST OF TABLES ........................................................................................................ VII LIST OF FIGURES .....................................................................................................VIII ACKNOWLEDGMENTS ............................................................................................... X ABSTRACT................................................................................................................... XII SECTION 1........................................................................................................................ 1 1.1 INTRODUCTION .......................................................................................................... 1 SECTION 2.......................................................................................................................
    [Show full text]
  • Azimuthal Dependence of Pion Interferometry in Au + Au Collisions at a Center of Mass Energy of 130Agev
    Azimuthal Dependence of Pion Interferometry in Au + Au Collisions at a Center of Mass Energy of 130AGeV DISSERTATION Presented in Partial Fulfillment of the Requirements for the Degree Doctor of Philosophy in the Graduate School of The Ohio State University By Randall C. Wells, B.S., M.S. ***** The Ohio State University 2002 Dissertation Committee: Approved by Michael A. Lisa, Adviser Richard Furnstahl Adviser Thomas Humanic Department of Physics Douglas Schumacher UMI Number: 3081976 ________________________________________________________ UMI Microform 3081976 Copyright 2003 by ProQuest Information and Learning Company. All rights reserved. This microform edition is protected against unauthorized copying under Title 17, United States Code. ____________________________________________________________ ProQuest Information and Learning Company 300 North Zeeb Road PO Box 1346 Ann Arbor, MI 48106-1346 ABSTRACT The study of two-pion Bose–Einstein correlations provides a tool to extract both spatial and dynamic information regarding the freeze–out configuration of the emis- sion region created in heavy ion collisions. Noncentral heavy ion collisions are inher- ently spatially and dynamically anisotropic. The study of such collisions through the 2 φ dependence of the HBT radii, Rij, relative to the event plane allows one to observe the source from all angles, leading to a richer description of the interplay between geometry and dynamics. The initial heavy ion running of the Relativistic Heavy Ion Collider (RHIC) at Brookhaven National Laboratory provided Au + Au collisions at 130GeV .Thefocus of the heavy ion program at RHIC is the search for a new state of strongly interact- ing matter, the quark gluon plasma (QGP). STAR is a large acceptance detector at RHIC with azimuthal symmetry, allowing the study of a large variety of observables on an event–by–event basis to provide a better characterization of the freeze–out con- ditions.
    [Show full text]
  • Study Quark Gluon Plasma by Particle Correlations In
    STUDY QUARK GLUON PLASMA BY PARTICLE CORRELATIONS IN HEAVY ION COLLISIONS A Dissertation Submitted to the Faculty of Purdue University by Li Yi In Partial Fulfillment of the Requirements for the Degree of Doctor of Philosophy December 2014 Purdue University West Lafayette, Indiana ii To my parents. iii ACKNOWLEDGMENTS On the journey to my doctoral degree, I have been blessed by many individuals, totaling more than can be listed here. First and foremost, I would like to thank my advisor Prof. Fuqiang Wang for his guidance and support over years with my research and my career. Prof. Wang guided me through the adventure of research with his inspiring ideas, patience in mentoring, prudent attitude towards data analysis, and critical feedback on the results. I would like to thank Prof. Wei Xie, Prof. Andrew Hirsch, Prof. Rolf Scharenberg and Prof. Brijish Srivastava for their helpful advices and discussions during the regular group meetings. I also would like to thank Prof. Denes Molnar for his valuable and fun discussions through his heavy-ion course and in regards to my thesis. I also would like to thank Prof. Matthew L. Lister to serving on my thesis committee. I would like to express my thanks to my fellow graduate students in heavy-ion group for their daily discussions: Tyler Browning, Liang He, Xin Li, Kun Jiang, Kurt Jung, Michael Skoby, Deke Sun, Jian Sun, Quan Wang. I received much encour- agement and help from Joshua Konzer from the beginning of my studies through when he graduated. I feel grateful to David Garand for providing feedback on my presentations and paper works.
    [Show full text]
  • Investigating Parton Energy Loss in the Quark-Gluon Plasma with Jet-Hadron Correlations and Jet Azimuthal Anisotropy at STAR
    Investigating Parton Energy Loss in the Quark-Gluon Plasma with Jet-hadron Correlations and Jet Azimuthal Anisotropy at STAR A Dissertation Presented to the Faculty of the Graduate School of Yale University in Candidacy for the Degree of Doctor of Philosophy by Alice Elisabeth Ohlson Dissertation Director: John Harris December 2013 Copyright c 2013 by Alice Elisabeth Ohlson All rights reserved. ii Abstract Investigating Parton Energy Loss in the Quark-Gluon Plasma with Jet-hadron Correlations and Jet Azimuthal Anisotropy at STAR Alice Elisabeth Ohlson 2013 In high-energy collisions of gold nuclei at the Relativistic Heavy Ion Collider (RHIC) and of lead nuclei at the Large Hadron Collider (LHC), a new state of matter known as the Quark-Gluon Plasma (QGP) is formed. This strongly-coupled, deconfined state of quarks and gluons represents the high energy-density limit of quantum chro- modynamics. The QGP can be probed by high-momentum quarks and gluons (collec- tively known as partons) that are produced in hard scatterings early in the collision. The partons traverse the QGP and fragment into collimated “jets” of hadrons. Stud- ies of parton energy loss within the QGP, or medium-induced jet quenching, can lead to insights into the interactions between a colored probe (a parton) and the colored medium (the QGP). Two analyses of jet quenching in relativistic heavy ion collisions are presented here. In the jet-hadron analysis, the distributions of charged hadrons with respect to the axis of a reconstructed jet are investigated as a function of azimuthal angle and transverse momentum (pT). It is shown that jets that traverse the QGP are softer (consisting of fewer high-pT fragments and more low-pT constituents) than jets in p+p collisions.
    [Show full text]
  • Experimental Searches for the Chiral Magnetic Effect in Heavy-Ion
    Experimental searches for the chiral magnetic effect in heavy-ion collisions Jie Zhao,1 Fuqiang Wang1;2 1Department of Physics and Astronomy, Purdue University, West Lafayette, Indiana 47907, USA 2School of Science, Huzhou University, Huzhou, Zhejiang 313000, China June 28, 2019 Abstract The chiral magnetic effect (CME) in quantum chromodynamics (QCD) refers to a charge sep- aration (an electric current) of chirality imbalanced quarks generated along an external strong magnetic field. The chirality imbalance results from interactions of quarks, under the approximate chiral symmetry restoration, with metastable local domains of gluon fields of non-zero topological charges out of QCD vacuum fluctuations. Those local domains violate the and invariance, P CP potentially offering a solution to the strong problem in explaining the magnitude of the matter- CP antimatter asymmetry in today's universe. Relativistic heavy-ion collisions, with the likely creation arXiv:1906.11413v1 [nucl-ex] 27 Jun 2019 of the high energy density quark-gluon plasma and restoration of the approximate chiral symmetry, and the possibly long-lived strong magnetic field, provide a unique opportunity to detect the CME. Early measurements of the CME-induced charge separation in heavy-ion collisions are dominated by physics backgrounds. Major efforts have been devoted to eliminate or reduce those backgrounds. We review those efforts, with a somewhat historical perspective, and focus on the recent innovative experimental undertakings in the search for the CME in heavy-ion collisions. Keywords: heavy-ion collisions, chiral magnetic effect, three-point correlator, elliptic flow back- ground, invariant mass, harmonic plane 1 Contents 1 Introduction 3 1.1 The chiral magnetic effect .
    [Show full text]
  • Hot and Dense QCD Matter Unraveling the Mysteries of the Strongly Interacting Quark-Gluon-Plasma
    Hot and Dense QCD Matter Unraveling the Mysteries of the Strongly Interacting Quark-Gluon-Plasma A Community White Paper on the Future of Relativistic Heavy-Ion Physics in the US Executive Summary This document presents the response of the US relativistic heavy-ion community to the request for comments by the NSAC Subcommittee, chaired by Robert Tribble, that is tasked to recommend optimizations to the US Nuclear Science Program over the next five years. The study of the properties of hot and dense QCD matter is one of the four main areas of nuclear physics research described in the 2007 NSAC Long Range Plan. The US nuclear physics community plays a leading role in this research area and has been instrumental in its most important discovery made over the past decade, namely that hot and dense QCD matter acts as a strongly interacting system with unique and previously unexpected properties. The US relativistic heavy ion program has now entered a crucial phase, where many measurements of the fundamental properties of the strongly interacting QCD plasma are capable of achieving a precision ( 10%), sufficient to determine whether the conjectured lower bound of viscosity to entropy is achieved∼ and to identify the primary energy loss mechanisms for hard partons traversing the plasma. Nonetheless, there are still important discoveries to be made in the search for a critical point in the phase diagram and in seeking to understand the mysterious behavior of heavy quarks in the plasma. This document lays out the quantifiable deliverables and open questions the US relativistic heavy-ion program will address over the next several years, with the goal of gaining a comprehensive understanding of the dynamics and properties of the strongly interacting QCD matter, the long sought after Quark Gluon Plasma.
    [Show full text]
  • Observation of the Antimatter Helium-4 ( He, Α) Nucleus and The
    c Copyright 2012 by Liang Xue All Rights Reserved Dedicated to my parents ii Acknowledgments Acknowledgments First and foremost, I would like to express my heartfelt gratitude to my advisor Prof. Yugang Ma for the continuous support of my Ph.D study, for his patience, motivation, experience, and immense knowledge. His guidance helped me in all the time of my research and writing of this thesis. I could not have imagined having a better advisor for my Ph.D study. I hope that one day I would become as good as an advisor to my student as Prof. Ma has been to me. I would like to address special thanks and appreciation to my co-advisor Dr. Aihong Tang. During my years at Brookhaven National Laboratory (BNL) as a visitor, he brought me into the world of experimental high energy nuclear physics, showed me how to research a problem and achieve goals, taught me how to question thoughts and express ideas. He has given me plenty of opportunities to present my work in front of experts in the field, spent endless time reviewing and proofreading my papers. The many skills I have learnt from him will constantly remind me of how great a teacher he is throughout my life. My sincere thanks also goes to Prof. Nu Xu, Dr. Hank Crawford, Prof. Keane Declan, Dr. Zhangbu Xu, and Prof. Huan Zhong Huang, for helpful suggestions and fruitful discus- sions. Many thanks to Dr. Tonko Ljubicic, Dr. Jeff Landgraf, Dr. Yuri Fisyak, Dr. Gene Van Buren, and Dr. Jerome Lauret for their technical support.
    [Show full text]
  • Arxiv:1808.09619V1 [Nucl-Ex] 29 Aug 2018
    Antinuclei in Heavy-Ion Collisions Jinhui Chena, Declan Keaneb,∗, Yu-Gang Maa,c,∗∗, Aihong Tangd, Zhangbu Xud,e aShanghai Institute of Applied Physics, Chinese Academy of Sciences, Shanghai 201800, China bKent State University, Kent, Ohio 44242, USA cUniversity of Chinese Academy of Sciences, Beijing 100049, China dBrookhaven National Laboratory, Upton, New York 11973, USA eShandong University, Jinan, Shandong 250100, China Abstract We review progress in the study of antinuclei, starting from Dirac's equation and the discovery of the positron in cosmic-ray events. The development of proton accelerators led to the discovery of antiprotons, followed by the first antideuterons, demonstrating that antinucleons bind into antinuclei. With the development of heavy-ion programs at the Brookhaven AGS and CERN SPS, it was demonstrated that central collisions of heavy nuclei offer a fertile ground for research and discoveries in the area of antinuclei. In this review, we empha- size recent observations at Brookhaven's Relativistic Heavy Ion Collider and at CERN's Large Hadron Collider, namely, the antihypertriton and the antihelium- 4, as well as measurements of the mass difference between light nuclei and antinuclei, and the interaction between antiprotons. Physics implications of the new observations and different production mechanisms are discussed. We also consider implications for related fields, such as hypernuclear physics and space- based cosmic-ray experiments. arXiv:1808.09619v1 [nucl-ex] 29 Aug 2018 Keywords: Heavy ions, antinuclei, antihypernuclei, hypernuclei, muonic antiatoms, CPT symmetry, baryogenesis, coalescence ∗Corresponding author, [email protected] ∗∗Corresponding author, [email protected] Preprint submitted to Physics Reports August 30, 2018 Contents 1 Historical Introduction 3 1.1 The Dirac Equation .
    [Show full text]
  • Nuclear Science
    NUCLEAR SCIENCE A GUIDE TO THE NUCLEAR SCIENCE WALL CHART or You don’t have to be a Nuclear Physicist to Understand Nuclear Science. Nuclear Science—A Guide to the Nuclear Science Wall Chart ©2019 Contemporary Physics Education Project (CPEP) Contents 1. Overview 2. The Atomic Nucleus 3. Radioactivity 4. Fundamental Interactions 5. Symmetries and Antimatter 6. Nuclear Energy Levels 7. Nuclear Reactions 8. Heavy Elements 9. Phases of Nuclear Matter 10. Origin of the Elements 11. Particle Accelerators 12. Tools of Nuclear Science 13. “... but What is it Good for?” 14. Energy from Nuclear Science 15. Radiation in the Environment Appendix A Glossary of Nuclear Terms Appendix B Classroom Topics Appendix C Useful Quantities in Nuclear Science Appendix D Average Annual Exposure Appendix E Nobel Prizes in Nuclear Science Appendix F Radiation Effects at Low Dosages ii Nuclear Science—A Guide to the Nuclear Science Wall Chart ©2019 Contemporary Physics Education Project (CPEP) Fifth Edition – October 2019 iii Nuclear Science—A Guide to the Nuclear Science Wall Chart ©2019 Contemporary Physics Education Project (CPEP) Contributors to the Booklet Gordon Aubrecht Ohio State University, Marion and Columbus, OH A. Baha Balantekin University of Wisconsin, Madison, WI Wolfgang Bauer Michigan State University, East Lansing, MI John Beacom California Institute of Technology, Pasadena CA Elizabeth J. Beise University of Maryland, College Park, MD David Bodansky University of Washington, Seattle, WA Edgardo Browne Lawrence Berkeley National Laboratory, Berkeley,
    [Show full text]
  • Discovery of Quark-Gluon Plasma: Strangeness Diaries
    Eur. Phys. J. Special Topics 229, 1{140 (2020) c The Author(s) 2020 THE EUROPEAN https://doi.org/10.1140/epjst/e2019-900263-x PHYSICAL JOURNAL SPECIAL TOPICS Review Discovery of Quark-Gluon Plasma: Strangeness Diaries Johann Rafelski1,2 ;a 1 CERN-TH, 1211 Geneva 23, Switzerland 2 Department of Physics, The University of Arizona, Tucson, AZ, 85721, USA Received 4 November 2019 Published online 24 January 2020 Abstract. We look from a theoretical perspective at the new phase of matter, quark-gluon plasma (QGP), the new form of nuclear matter created at high temperature and pressure. Here I retrace the path to QGP discovery and its exploration in terms of strangeness production and strange particle signatures. We will see the theoretical arguments that have been advanced to create interest in this determining signa- ture of QGP. We explore the procedure used by several experimental groups making strangeness production an important tool in the search and discovery of this primordial state of matter present in the Universe before matter in its present form was formed. We close by looking at both the ongoing research that increases the reach of this observable to LHC energy scale pp collisions, and propose an interpretation of these unexpected results. It is very appropriate that you did reconstruct your version of the QGP discovery. Your quotations concerning me are correct and reproduce well my opinion, which I have not changed. CERN found good evidence for deconfinement, and it was at all appropriate to say that in public, independently from the status of RHIC at the time.
    [Show full text]
  • High Energy Heavy Ion Experiments
    UCRL-ID-119181 High Energy Heavy Ion Experiments J. Thomas P. Jacobs November 1994 DISTRIBUTION OF THIS DOCUMENT IS UNLIMITED DISCLAIMER This document was prepared as an account of work sponsored by an agency of the United States Government. Neither the United States Government nor the University of California nor any of their employees, makes any warranty, express or implied, or assumes any legal liability or responsibility 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. Reference herein to any specific commercial products, process, or service by trade name, trademark, manufacturer, or otherwise, does not necessarily constitute or imply its endorsement, recommendation, or favoring by the United States Government or the University of California. The views and opinions of authors expressed herein do not necessarily state or reflect those of the United States Government or the University of California, and shall not be used for advertising or product endorsement purposes. This report has been reproduced directly from the best available copy. Available to DOE and DOE contractors from the Office of Scientific and Technical Information P.O. Box 62, Oak Ridge, TN 37831 Prices available from (615) 576-8401, FTS 626-8401 Available to the public from the National Technical Information Service VS. Department of Commerce 5285 Port Royal Rd, Springfield, VA 22161 DISCLAIMER Portions of this document may be iilegible in
    [Show full text]