History of Particle Colliders
Total Page:16
File Type:pdf, Size:1020Kb
Load more
Recommended publications
-
Computer-Assisted Composition a Short Historical Review
MUMT 303 New Media Production II Charalampos Saitis Winter 2010 Computer-Assisted Composition A short historical review Computer-assisted composition is considered amongst the major musical developments that characterized the twentieth century. The quest for ‘new music’ started with Erik Satie and the early electronic instruments (Telharmonium, Theremin), explored the use of electricity, moved into the magnetic tape recording (Stockhausen, Varese, Cage), and soon arrived to the computer era. Computers, science, and technology promised new perspectives into sound, music, and composition. In this context computer-assisted composition soon became a creative challenge – if not necessity. After all, composers were the first artists to make substantive use of computers. The first traces of computer-assisted composition are found in the Bells Labs, in the U.S.A, at the late 50s. It was Max Matthews, an engineer there, who saw the possibilities of computer music while experimenting on digital transmission of telephone calls. In 1957, the first ever computer programme to create sounds was built. It was named Music I. Of course, this first attempt had many problems, e.g. it was monophonic and had no attack or decay. Max Matthews went on improving the programme, introducing a series of programmes named Music II, Music III, and so on until Music V. The idea of unit generators that could be put together to from bigger blocks was introduced in Music III. Meanwhile, Lejaren Hiller was creating the first ever computer-composed musical work: The Illiac Suit for String Quartet. This marked also a first attempt towards algorithmic composition. A binary code was processed in the Illiac Computer at the University of Illinois, producing the very first computer algorithmic composition. -
Accelerator and Beam Physics Research Goals and Opportunities
Accelerator and Beam Physics Research Goals and Opportunities Working group: S. Nagaitsev (Fermilab/U.Chicago) Chair, Z. Huang (SLAC/Stanford), J. Power (ANL), J.-L. Vay (LBNL), P. Piot (NIU/ANL), L. Spentzouris (IIT), and J. Rosenzweig (UCLA) Workshops conveners: Y. Cai (SLAC), S. Cousineau (ORNL/UT), M. Conde (ANL), M. Hogan (SLAC), A. Valishev (Fermilab), M. Minty (BNL), T. Zolkin (Fermilab), X. Huang (ANL), V. Shiltsev (Fermilab), J. Seeman (SLAC), J. Byrd (ANL), and Y. Hao (MSU/FRIB) Advisors: B. Dunham (SLAC), B. Carlsten (LANL), A. Seryi (JLab), and R. Patterson (Cornell) January 2021 Abbreviations and Acronyms 2D two-dimensional 3D three-dimensional 4D four-dimensional 6D six-dimensional AAC Advanced Accelerator Concepts ABP Accelerator and Beam Physics DOE Department of Energy FEL Free-Electron Laser GARD General Accelerator R&D GC Grand Challenge H- a negatively charged Hydrogen ion HEP High-Energy Physics HEPAP High-Energy Physics Advisory Panel HFM High-Field Magnets KV Kapchinsky-Vladimirsky (distribution) ML/AI Machine Learning/Artificial Intelligence NCRF Normal-Conducting Radio-Frequency NNSA National Nuclear Security Administration NSF National Science Foundation OHEP Office of High Energy Physics QED Quantum Electrodynamics rf radio-frequency RMS Root Mean Square SCRF Super-Conducting Radio-Frequency USPAS US Particle Accelerator School WG Working Group 1 Accelerator and Beam Physics 1. EXECUTIVE SUMMARY Accelerators are a key capability for enabling discoveries in many fields such as Elementary Particle Physics, Nuclear Physics, and Materials Sciences. While recognizing the past dramatic successes of accelerator-based particle physics research, the April 2015 report of the Accelerator Research and Development Subpanel of HEPAP [1] recommended the development of a long-term vision and a roadmap for accelerator science and technology to enable future DOE HEP capabilities. -
The Institute of Physics
REGIONAL NEWS 21 The Institute of Physics The forerunner of the Institute of do involves physics - switching on a light, physicists in commerce and industry. The Physics, the Physical Society of London, making a phone call or even baking a Council has established several Profession was created in 1874 at a time when the potato in a microwave oven. In industry, al Groups in areas such as consultancy, understanding of the physical world had physicists are helping companies to devel engineering physics and advanced been given an enormous impetus with the op novel materials that have physical prop systems. publication by James Clerk Maxwell of his erties more versatile that those previously In these days of shrinking science theory of electromagnetism. The creation developed, and they are designing new budgets, the academic physics community of the Physical Society was the response of generations of microchips which are has turned increasingly to its professional the embryonic society of professional and smaller and hence faster. The information representative, the Institute of Physics, to amateur physicists in Britain to what they revolution within which we are currently lobby Government about the importance believed was a major progression of their being buffeted would have been impos and relevance of physics. In common with ideas. Indeed, one could say that it was at sible without physicists and their research other science subjects, calls to justify Gov this time that much of physics began to - transistors, liquid crystal displays, mag ernment expenditure have increased in take on the appearance we recognize netic discs, optical fibres, semiconductor recent years. -
2016 VISPA Newsletter
Physics and Astronomy VISPA 2016 NEWSLETTER VICTORIA SUBATOMIC PHYSICS AND ACCELERATOR RESEARCH CENTRE Photo credit: CERN ATLAS candidate event for the production of a Higgs boson decaying into two Z bosons that each decay into a muon-antimuon pair. In this issue: ATLAS and the Higgs Discovery ......2 ARIEL and the Accelerator Physics The Future is Here: Research Graduate Program at VISPA ..........8 Training in VISPA. .10 VISPA members of T2K awarded 2016 Breakthrough Prize in Dark Energy and ALTAIR: Experimental Remembering Alan Astbury and Fundamental Physics ................4 Particle Astrophysics in VISPA ........9 the Inaugural Astbury Lecture ......11 Flavour Physics in VISPA ..............6 Research Computing in High Perspectives on New Physics Energy Physics. .10 at the Intensity Frontier .............12 MEMBER LIST FACULTY Name Research Area Justin Albert Experimental particle and astroparticle physics Dean Karlen Experimental particle physics ATLAS and the Higgs Discovery Richard Keeler Experimental particle physics Pavel Kovtun Theoretical physics Robert Kowalewski Experimental particle physics The Large Hadron Collider (LHC) at the CERN laboratory is the highest energy particle Michel Lefebvre Experimental particle physics collider in operation. The ATLAS detector is one of two multipurpose detectors Robert McPherson Experimental particle physics designed to record high energy collisions at the LHC. The UVic ATLAS group has been Maxim Pospelov Theoretical physics Adam Ritz Theoretical physics a member of the ATLAS Collaboration since its foundation in 1992, and contributed J. Michael Roney Experimental particle physics to the design and construction of the ATLAS detector. The LHC started operation in Randy Sobie Experimental particle physics 2010 with proton-proton collisions at 7 TeV centre of mass energy; the energy was EMERITUS FACULTY increased to 8 TeV in 2012. -
Il Nostro Mondo
IL NOSTRO MONDO THE DESIGN, CONSTRUCTION AND PERFORMANCE OF THE CERN INTERSECTING STORAGE RINGS (ISR) A RECOLLECTION OF WORLD’S FIRST PROTON-PROTON COLLIDER KURT HÜBNER CERN, Geneva, Switzerland 1 Design which had a beam energy of 160 MeV. The interaction points to increase the collision rate The concept of colliding beams appeared design of these colliders started in 1957. but without special lattice insertions as one first in a German patent by Rolf Widerøe In 1961, the Accelerator Research Group would use these days. registered in 1943 and published in 1952. Division was expanded into the Accelerator Combined-function magnets were chosen However, at that time the intensity of beams Division as experienced manpower had as in the PS, i.e. the main magnets had a was too low for an exploitable collision rate as become available after the running-in of the magnetic dipole field to bend the beam and a beam accumulation had not yet been invented. PS in 1960. At the same time it was decided quadrupole field to focus the beam. This type The first ideas of a realistic design were to construct a small accelerator to test rf of magnet provided space for the elaborate published in 1956 by Gerard O’Neill and by the stacking, a technique to be experimentally pole-face windings foreseen to control the MURA Group lead by Donald Kerst in the USA. proven, as it was essential for the performance magnetic field to a very high precision. It also MURA had come up with beam accumulation and success of the ISR. -
Accelerator Physics and Modeling
BNL-52379 CAP-94-93R ACCELERATOR PHYSICS AND MODELING ZOHREH PARSA, EDITOR PROCEEDINGS OF THE SYMPOSIUM ON ACCELERATOR PHYSICS AND MODELING Brookhaven National Laboratory UPTON, NEW YORK 11973 ASSOCIATED UNIVERSITIES, INC. UNDER CONTRACT NO. DE-AC02-76CH00016 WITH THE UNITED STATES DEPARTMENT OF ENERGY DISCLAIMER This report was prepared as an account of work sponsored by an agency of the Unite1 States Government Neither the United States Government nor any agency thereof, nor any of their employees, nor any of their contractors, subcontractors, or 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 product, process, or service by trade name, trademark, manufacturer, or otherwise, doea not necessarily constitute or imply its endorsement, recomm.ndation, or favoring by the UnitedStates Government or any agency, contractor or subcontractor thereof. The views and opinions of authors expressed herein do not necessarily state or reflect those of the United States Government or any agency, contractor or subcontractor thereof- Printed in the United States of America Available from National Technical Information Service U.S. Department of Commerce 5285 Port Royal Road Springfieid, VA 22161 NTIS price codes: Am&mffi TABLE OF CONTENTS Topic, Author Page no. Forward, Z . Parsa, Brookhaven National Lab. i Physics of High Brightness Beams , 1 M. Reiser, University of Maryland . Radio Frequency Beam Conditioner For Fast-Wave 45 Free-Electron Generators of Coherent Radiation Li-Hua NSLS Dept., Brookhaven National Lab, and A. -
Pos(ICRC2019)446
New Results from the Cosmic-Ray Program of the NA61/SHINE facility at the CERN SPS PoS(ICRC2019)446 Michael Unger∗ for the NA61/SHINE Collaborationy Karlsruhe Institute of Technology (KIT), Postfach 3640, D-76021 Karlsruhe, Germany E-mail: [email protected] The NA61/SHINE experiment at the SPS accelerator at CERN is a unique facility for the study of hadronic interactions at fixed target energies. The data collected with NA61/SHINE is relevant for a broad range of topics in cosmic-ray physics including ultrahigh-energy air showers and the production of secondary nuclei and anti-particles in the Galaxy. Here we present an update of the measurement of the momentum spectra of anti-protons produced in p−+C interactions at 158 and 350 GeV=c and discuss their relevance for the understanding of muons in air showers initiated by ultrahigh-energy cosmic rays. Furthermore, we report the first results from a three-day pilot run aimed at investigating the ca- pability of our experiment to measure nuclear fragmentation cross sections for the understanding of the propagation of cosmic rays in the Galaxy. We present a preliminary measurement of the production cross section of Boron in C+p interactions at 13.5 AGeV=c and discuss prospects for future data taking to provide the comprehensive and accurate reaction database of nuclear frag- mentation needed in the era of high-precision measurements of Galactic cosmic rays. 36th International Cosmic Ray Conference -ICRC2019- July 24th - August 1st, 2019 Madison, WI, U.S.A. ∗Speaker. yhttp://shine.web.cern.ch/content/author-list c Copyright owned by the author(s) under the terms of the Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License (CC BY-NC-ND 4.0). -
Accelerator Physics Third Edition
Preface Accelerator science took off in the 20th century. Accelerator scientists invent many in- novative technologies to produce and manipulate high energy and high quality beams that are instrumental to progresses in natural sciences. Many kinds of accelerators serve the need of research in natural and biomedical sciences, and the demand of applications in industry. In the 21st century, accelerators will become even more important in applications that include industrial processing and imaging, biomedical research, nuclear medicine, medical imaging, cancer therapy, energy research, etc. Accelerator research aims to produce beams in high power, high energy, and high brilliance frontiers. These beams addresses the needs of fundamental science research in particle and nuclear physics, condensed matter and biomedical sciences. High power beams may ignite many applications in industrial processing, energy production, and national security. Accelerator Physics studies the interaction between the charged particles and elec- tromagnetic field. Research topics in accelerator science include generation of elec- tromagnetic fields, material science, plasma, ion source, secondary beam production, nonlinear dynamics, collective instabilities, beam cooling, beam instrumentation, de- tection and analysis, beam manipulation, etc. The textbook is intended for graduate students who have completed their graduate core-courses including classical mechanics, electrodynamics, quantum mechanics, and statistical mechanics. I have tried to emphasize the fundamental physics behind each innovative idea with least amount of mathematical complication. The textbook may also be used by advanced undergraduate seniors who have completed courses on classical mechanics and electromagnetism. For beginners in accelerator physics, one begins with Secs. 2.I–2.IV in Chapter 2, and follows by Secs. -
Fifty Years of the CERN Proton Synchrotron Volume II
CERN–2013–005 12 August 2013 ORGANISATION EUROPÉENNE POUR LA RECHERCHE NUCLÉAIRE CERN EUROPEAN ORGANIZATION FOR NUCLEAR RESEARCH Fifty years of the CERN Proton Synchrotron Volume II Editors: S. Gilardoni D. Manglunki GENEVA 2013 ISBN 978–92–9083–391–8 ISSN 0007–8328 DOI 10.5170/CERN–2013–005 Copyright c CERN, 2013 Creative Commons Attribution 3.0 Knowledge transfer is an integral part of CERN’s mission. CERN publishes this report Open Access under the Creative Commons Attribution 3.0 license (http://creativecommons.org/licenses/by/3.0/) in order to permit its wide dissemination and use. This monograph should be cited as: Fifty years of the CERN Proton Synchrotron, volume II edited by S. Gilardoni and D. Manglunki, CERN-2013-005 (CERN, Geneva, 2013), DOI: 10.5170/CERN–2013–005 Dedication The editors would like to express their gratitude to Dieter Möhl, who passed away during the preparatory phase of this volume. This report is dedicated to him and to all the colleagues who, like him, contributed in the past with their cleverness, ingenuity, dedication and passion to the design and development of the CERN accelerators. iii Abstract This report sums up in two volumes the first 50 years of operation of the CERN Proton Synchrotron. After an introduction on the genesis of the machine, and a description of its magnet and powering systems, the first volume focuses on some of the many innovations in accelerator physics and instrumentation that it has pioneered, such as transition crossing, RF gymnastics, extractions, phase space tomography, or transverse emittance measurement by wire scanners. -
The Charm of Theoretical Physics (1958– 1993)?
Eur. Phys. J. H 42, 611{661 (2017) DOI: 10.1140/epjh/e2017-80040-9 THE EUROPEAN PHYSICAL JOURNAL H Oral history interview The Charm of Theoretical Physics (1958{ 1993)? Luciano Maiani1 and Luisa Bonolis2,a 1 Dipartimento di Fisica and INFN, Piazzale A. Moro 5, 00185 Rome, Italy 2 Max Planck Institute for the History of Science, Boltzmannstraße 22, 14195 Berlin, Germany Received 10 July 2017 / Received in final form 7 August 2017 Published online 4 December 2017 c The Author(s) 2017. This article is published with open access at Springerlink.com Abstract. Personal recollections on theoretical particle physics in the years when the Standard Theory was formed. In the background, the remarkable development of Italian theoretical physics in the second part of the last century, with great personalities like Bruno Touschek, Raoul Gatto, Nicola Cabibbo and their schools. 1 Apprenticeship L. B. How did your interest in physics arise? You enrolled in the late 1950s, when the period of post-war reconstruction of physics in Europe was coming to an end, and Italy was entering into a phase of great expansion. Those were very exciting years. It was the beginning of the space era. L. M. The beginning of the space era certainly had a strong influence on many people, absolutely. The landing on the moon in 1969 was for sure unforgettable, but at that time I was already working in Physics and about to get married. My interest in physics started well before. The real beginning was around 1955. Most important for me was astronomy. It is not surprising that astronomy marked for many people the beginning of their interest in science. -
F. Richard Moore, Dreams of Computer Music: Then And
Dreams of Computer Music: Then and Now Author(s): F. Richard Moore Source: Computer Music Journal, Vol. 20, No. 1 (Spring, 1996), pp. 25-41 Published by: The MIT Press Stable URL: http://www.jstor.org/stable/3681267 Accessed: 28/01/2010 22:31 Your use of the JSTOR archive indicates your acceptance of JSTOR's Terms and Conditions of Use, available at http://www.jstor.org/page/info/about/policies/terms.jsp. JSTOR's Terms and Conditions of Use provides, in part, that unless you have obtained prior permission, you may not download an entire issue of a journal or multiple copies of articles, and you may use content in the JSTOR archive only for your personal, non-commercial use. Please contact the publisher regarding any further use of this work. Publisher contact information may be obtained at http://www.jstor.org/action/showPublisher?publisherCode=mitpress. Each copy of any part of a JSTOR transmission must contain the same copyright notice that appears on the screen or printed page of such transmission. JSTOR is a not-for-profit service that helps scholars, researchers, and students discover, use, and build upon a wide range of content in a trusted digital archive. We use information technology and tools to increase productivity and facilitate new forms of scholarship. For more information about JSTOR, please contact [email protected]. The MIT Press is collaborating with JSTOR to digitize, preserve and extend access to Computer Music Journal. http://www.jstor.org F.Richard Moore of Department of Music, and Center for Research Dreams Computer in Computing and the Arts University of California, San Diego Music-Then and Now La Jolla, California 92093-0037, USA [email protected] Computer music was first created nearly 40 years observations, first published in 1514, that led him ago in universities and research laboratoriesby to suggest that the earth revolves around the sun people dreaming of magical instruments for music. -
2013 January
Online Newsletter January 2013 Issue no 24 Branch committee REMS At Home - An Environmental Miscellany Dr Mark Telling CPhys MInstP, Chair On 10 January 71 members and guests were educated and entertained E-mail [email protected] by 5 invited speakers. The meeting was organised and orchestrated by Bob Boutland CPhys MInstP George Freeman, who unfortunately could not attend during Treasurer recuperation following an operation. Mike Quinton, (pictured below) Education representative introduced the speakers. and online newsletter editor E-mail [email protected] David Parkes CPhys MInstP Berkshire Centre representative E-mail [email protected] Stephen Elsmere Berkshire Centre representative E-mail [email protected] Leonard Lewell CPhys MInstP, London Centre Representative E-mail [email protected] Prof. R Mackintosh CPhys FInstP Milton Keynes Centre representative E-mail [email protected] Dr Diane Crann MInstP Hertfordshire Centre representative E-mail [email protected] J A Belling MInstP REMS visit secretary E-mail [email protected] The Barometer and its early use in forecasting on land and on sea” Marta Caballero E-mail [email protected] Anita McConnell Provided a very detailed story from the early days. It Student Representative was Torricelli and Viviani who showed in 1643-4 that there is such a thing as a vacuum noting that the height of the column mercury varied James Kneller daily with changes in the weather, but also with temperature. Pascal E-mail [email protected] Student Representative noted that a barometer recorded a lower pressure when taken up a mountain, the Puy de Dôme.