Cern Courier March/April 2019 3
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CERN Courier–Digital Edition
CERNMarch/April 2021 cerncourier.com COURIERReporting on international high-energy physics WELCOME CERN Courier – digital edition Welcome to the digital edition of the March/April 2021 issue of CERN Courier. Hadron colliders have contributed to a golden era of discovery in high-energy physics, hosting experiments that have enabled physicists to unearth the cornerstones of the Standard Model. This success story began 50 years ago with CERN’s Intersecting Storage Rings (featured on the cover of this issue) and culminated in the Large Hadron Collider (p38) – which has spawned thousands of papers in its first 10 years of operations alone (p47). It also bodes well for a potential future circular collider at CERN operating at a centre-of-mass energy of at least 100 TeV, a feasibility study for which is now in full swing. Even hadron colliders have their limits, however. To explore possible new physics at the highest energy scales, physicists are mounting a series of experiments to search for very weakly interacting “slim” particles that arise from extensions in the Standard Model (p25). Also celebrating a golden anniversary this year is the Institute for Nuclear Research in Moscow (p33), while, elsewhere in this issue: quantum sensors HADRON COLLIDERS target gravitational waves (p10); X-rays go behind the scenes of supernova 50 years of discovery 1987A (p12); a high-performance computing collaboration forms to handle the big-physics data onslaught (p22); Steven Weinberg talks about his latest work (p51); and much more. To sign up to the new-issue alert, please visit: http://comms.iop.org/k/iop/cerncourier To subscribe to the magazine, please visit: https://cerncourier.com/p/about-cern-courier EDITOR: MATTHEW CHALMERS, CERN DIGITAL EDITION CREATED BY IOP PUBLISHING ATLAS spots rare Higgs decay Weinberg on effective field theory Hunting for WISPs CCMarApr21_Cover_v1.indd 1 12/02/2021 09:24 CERNCOURIER www. -
The ATLAS Experiment
The ATLAS Experiment Mapping the Secrets of the Universe Michael Barnett Physics Division July 2007 With help from: Joao Pequenao Paul Schaffner M. Barnett – July 2007 1 Large Hadron Collider CERN lab in Geneva Switzerland Protons will circulate in opposite directions and collide inside experimental areas 100 meters underground 17 miles around M. Barnett – July 2007 2 The ATLAS Experiment See animation M. Barnett – July 2007 3 Large Hadron Collider Numbers The fastest racetrack on the planet Trillions of protons will race around the 17-mile ring 11,000 times a second, traveling at 99.9999991% the speed of light. Seven times the energy of any previous accelerator. The emptiest space in the solar system Accelerating protons to almost the speed of light requires a vacuum as empty as interplanetary space. There is 10 times more atmosphere on the moon than there will be in the LHC. M. Barnett – July 2007 4 Large Hadron Collider Numbers The hottest spot in our galaxy Colliding protons will generate temperatures 100,000 times hotter than the sun (but in a minuscule space). Equivalent to a billionth of a second after the Big Bang M. Barnett – July 2007 5 LHC Exhibition at London Science Museum M. Barnett – July 2007 6 Large Hadron Collider Numbers The biggest most sophisticated detectors ever built Recording the debris from 600 million proton collisions per second requires building gargantuan devices that measure particles with 0.0004 inch precision. The most extensive computer system in the world Analyzing the data requires tens of thousands of computers around the world using the Grid. -
Aaron Taylor Physics and Astronomy This
Aaron Taylor Candidate Physics and Astronomy Department This dissertation is approved, and it is acceptable in quality and form for publication: Approved by the Dissertation Committee: Dr. Sally Seidel , Chairperson Dr. Pavel Reznicek Dr. Huaiyu Duan Dr. Douglas Fields Dr. Bruce Schumm CERN-THESIS-2017-006 04/11/2016 SEARCH FOR NEW PHYSICS PROCESSES WITH HEAVY QUARK SIGNATURES IN THE ATLAS EXPERIMENT by AARON TAYLOR B.A., Mathematics, University of California, Santa Cruz, 2011 M.S., Physics, University of New Mexico, 2014 DISSERTATION Submitted in Partial Fulfillment of the Requirements for the Degree of Doctor of Philosophy Physics The University of New Mexico Albuquerque, New Mexico May, 2017 ©2017, Aaron Taylor iii Acknowledgements I would like to thank Professor Sally Seidel, for her constant support and guidance in my research. I would also like to thank her for her patience in helping me to develop my technical writing and presentation skills; without her assistance, I would never have gained the skill I have in that field. I would like to thank Konstantin Toms, for his constant assistance with the ATLAS code, and for generally giving advice on how to handle data analysis. The Bs → 4μ analysis likely wouldn’t have gotten anywhere without him. I would like to deeply thank Pavel Reznicek, without whom I would never have gotten as great an understanding of ATLAS code as I currently have. It is no exaggeration to say that I would not have been half as successful as I have been without his constant patience and understanding. Thank you. Many thanks to Martin Hoeferkamp, who taught me much about instrumentation and physical measurements. -
CERN to Seek Answers to Such Fundamental 1957, Was CERN’S First Accelerator
What is the nature of our universe? What is it ----------------------------------------- DAY 1 -------- made of? Scientists from around the world go to The 600 MeV Synchrocyclotron (SC), built in CERN to seek answers to such fundamental 1957, was CERN’s first accelerator. It provided questions using particle accelerators and pushing beams for CERN’s first experiments in particle and nuclear the limits of technology. physics. In 1964, this machine started to concentrate on nuclear physics alone, leaving particle physics to the newer During February 2019, I was given a once in a lifetime and more powerful Proton Synchrotron. opportunity to be part of The Maltese Teacher Programme at CERN, which introduced me, as one of the participants, to cutting-edge particle physics through lectures, on-site visits, exhibitions, and hands-on workshops. Why do they do all this? The main objective of these type of visits is to bring modern science into the classroom. Through this report, my purpose is to give an insight of what goes on at CERN as well as share my experience with you students, colleagues, as well as the general public. The SC became a remarkably long-lived machine. In 1967, it started supplying beams for a dedicated radioactive-ion-beam facility called ISOLDE, which still carries out research ranging from pure What does “CERN” stand for? At an nuclear physics to astrophysics and medical physics. In 1990, intergovernmental meeting of UNESCO in Paris in ISOLDE was transferred to the Proton Synchrotron Booster, and the SC closed down after 33 years of service. December 1951, the first resolution concerning the establishment of a European Council for Nuclear Research SM18 is CERN’s main facility for testing large and heavy (in French Conseil Européen pour la Recherche Nucléaire) superconducting magnets at liquid helium temperatures. -
Slides Lecture 1
Advanced Topics in Particle Physics Probing the High Energy Frontier at the LHC Ulrich Husemann, Klaus Reygers, Ulrich Uwer University of Heidelberg Winter Semester 2009/2010 CERN = European Laboratory for Partice Physics the world’s largest particle physics laboratory, founded 1954 Historic name: “Conseil Européen pour la Recherche Nucléaire” Lake Geneva Proton-proton2500 employees, collider almost 10000 guest scientists from 85 nations Jura Mountains 8.5 km Accelerator complex Prévessin site (approx. 100 m underground) (France) Meyrin site (Switzerland) Probing the High Energy Frontier at the LHC, U Heidelberg, Winter Semester 09/10, Lecture 1 2 Large Hadron Collider: CMS Experiment: Proton-Proton and Multi Purpose Detector Lead-Lead Collisions LHCb Experiment: B Physics and CP Violation ALICE-Experiment: ATLAS Experiment: Heavy Ion Physics Multi Purpose Detector Probing the High Energy Frontier at the LHC, U Heidelberg, Winter Semester 09/10, Lecture 1 3 The Lecture “Probing the High Energy Frontier at the LHC” Large Hadron Collider (LHC) at CERN: premier address in experimental particle physics for the next 10+ years LHC restart this fall: first beam scheduled for mid-November LHC and Heidelberg Experimental groups from Heidelberg participate in three out of four large LHC experiments (ALICE, ATLAS, LHCb) Theory groups working on LHC physics → Cornerstone of physics research in Heidelberg → Lots of exciting opportunities for young people Probing the High Energy Frontier at the LHC, U Heidelberg, Winter Semester 09/10, Lecture 1 4 Scope -
Fabiola Gianotti
Fabiola Gianotti Date of Birth 29 October 1960 Place Rome, Italy Nomination 18 August 2020 Field Physics Title Director-General of the European Laboratory for Particle Physics, CERN, Geneva Most important awards, prizes and academies Honorary Professor, University of Edinburgh; Corresponding or foreign associate member of the Italian Academy of Sciences (Lincei), the National Academy of Sciences of the United States, the French Academy of Sciences, the Royal Society London, the Royal Academy of Sciences and Arts of Barcelona, the Royal Irish Academy and the Russian Academy of Sciences. Honorary doctoral degrees from: University of Uppsala (2012); Ecole Polytechnique Federale de Lausanne (2013); McGill University, Montreal (2014); University of Oslo (2014); University of Edinburgh (2015); University of Roma Tor Vergata (2017); University of Chicago (2018); University Federico II, Naples (2018); Université de Paris Sud, Orsay (2018); Université Savoie Mont Blanc, Annecy (2018); Weizmann Institute, Israel (2018); Imperial College, London (2019). National honours: Cavaliere di Gran Croce dell'Ordine al Merito della Repubblica, awarded by the Italian President Giorgio Napolitano (2014). Special Breakthrough Prize in Fundamental Physics (shared, 2013); Enrico Fermi Prize of the Italian Physical Society (shared, 2013); Medal of Honour of the Niels Bohr Institute, Copenhagen (2013); Wilhelm Exner Medal, Vienna (2017); Tate Medal of the American Institute of Physics for International Leadership (2019). Summary of scientific research Fabiola Gianotti is a particle physicist working at high-energy accelerators. In her scientific career, she has made significant contributions to several experiments at CERN, including UA2 at the proton-antiproton collider (SpbarpS), ALEPH at the Large Electron-Positron collider (LEP) and ATLAS at the Large Hadron Collider (LHC). -
Formation of Centauro and Strangelets in Nucleus–Nucleus Collisions at the LHC and Their Identification by the ALICE Experiment 1 A.L.S
HE.6.2.02 Formation of Centauro and Strangelets in Nucleus–Nucleus Collisions at the LHC and their Identification by the ALICE Experiment 1 A.L.S. Angelis1,J.Bartke2, M.Yu. Bogolyubsky3, S.N. Filippov4, E. Gładysz-Dziadus´2, Yu.V. Kharlov3,A.B.Kurepin4, A.I. Maevskaya4, G. Mavromanolakis1, A.D. Panagiotou1, S.A. Sadovsky3,P.Stefanski2 and Z. Włodarczyk5 1Division of Nuclear and Particle Physics, University of Athens,Greece. 2Institute of Nuclear Physics, Cracow, Poland. 3Institute for High Energy Physics, Protvino, Russia. 4Institute for Nuclear Research, Moscow,Russia. 5Institute of Physics, Pedagogical University, Kielce, Poland. Abstract We present a phenomenological model which describes the formation of a Centauro fireball in nucleus-nucleus interactions in the upper atmosphere and at the LHC, and its decay to non-strange baryons and Strangelets. We describe the CASTOR detector for the ALICE experiment at the LHC. CASTOR will probe, in an event- by-event mode, the very forward, baryon-rich phase space 5.6 ≤ η ≤ 7.2in5.5×A TeV central Pb + Pb collisions. We present results of simulations for the response of the CASTOR calorimeter, and in particular to the traversal of Strangelets. 1 Introduction: The physics motivation to study the very forward phase space in nucleus–nucleus collisions stems from the potentially very rich field of new phenomena, to be produced in and by an environment with very high baryochemical potential. The study of this baryon-dense region, much denser than the highest baryon density attained at the AGS or SPS, will provide important information for the understanding of a Deconfined Quark Matter (DQM) state at relatively low temperatures, with different properties from those expected in the higher temperature baryon-free region around mid-rapidity, thought to exist in the core of neutron stars. -
After Dinner Speech by Dr
1 After Dinner Speech by Dr. Josef Rembser CERN, Geneva 14 September 2009 Celebration in honour of Professor Herwig Schopper’s 85 th Birthday I. Dear Friends, honourable, dear Professor Schopper! On 28 February of this year, you celebrated your 85th Birthday. This evening we are looking back on this memorable date, wishing you many happy returns of the day. You have been blessed with a life full of harmony and accomplishments, always keeping young physically and intellectually. This is a special blessing granted to a person: Love and family, friendships and encounters, giving and receiving, working and achieving acknowledgements and honours in a fulfilling profession and in challenging missions. Tomorrow, a scientific Colloquium will honour you as researcher and scientific teacher . Today, on the eve of the colloquium, I would like to speak about Herwig Schopper as a research politician and a research manager . My personal remarks and remembrances will focus, dear Herwig Schopper, on the guiding contributions you made in shaping, promoting and advancing science and research and their relevant policies in Germany and in Europe. 2 Professor Heuer, I am grateful for your invitation. It is a pleasure for me to give today's After-Dinner speech in honour of our jubilee. For many years during my service in the German Ministry of Research and Technology (BMFT) in Bonn I had close personal and professional connections with you, dear Professor Schopper, regarding German science and research policy including CERN. II. In 1945, with the end of the 2 nd World War, Germany as guilty party and loser plunged the world and its own country into destruction and suffering, thus experiencing a historical catastrophe. -
Swapan Chattopadhyay Course Syllabus
NIU PHYSICS 659: Special Problems in Physics, Winter 2016 Instructor: Swapan Chattopadhyay Course Syllabus This is an independent study course involving personalized study, research, problem searching and problem solving in the field of Physics of Beams and Accelerator Science. The enrolled student will perform literature search via the web, available libraries, and references provided by the instructor and identify relevant publications and current up-to-date status of the fields/topics mentioned below, search for potential areas for further exploratory research and list and quantify a limited set of graduate dissertation areas/topics that are mature for getting engaged in. The areas/topics suggested for study/research in this semester are: 1. Theoretical, computational and experimental aspects of nonlinear dynamics of high intensity space-charge dominated proton beams as relevant for future proton accelerators for exploring neutrino physics and possibilities of scaled experiments at the Integrated Optics Test Accelerator (IOTA), under construction at Fermilab. The topics could address theoretical modelling or computer simulation or experimental measurements of nonlinear dynamics, dynamical diffusion, beam halo formation and resonance dynamics in general. 2. Explore and investigate possible research into the design and development of the 100 TeV- class proton collider as envisioned in the Future Circular Collider (FCC) design study at CERN and identify beam dynamics issues relevant for further research e.g. coherent beam instabilities; beam injection dynamics; beam-environment interaction via electromagnetic impedance, beam luminosity, beam lifetime and ring lattice. 3. Explore and investigate possible research into the proton-driven plasma wakefield experiment, AWAKE, under development at CERN. The possible research areas could be around beam-plasma high fidelity simulations, beam injection dynamics, beam and plasma diagnostics and scaling from present experiments to a proper collider. -
Calorimetry for Particle Physics
REVIEWS OF MODERN PHYSICS, VOLUME 75, OCTOBER 2003 Calorimetry for particle physics Christian W. Fabjan and Fabiola Gianotti CERN, 1211 Geneva 23, Switzerland (Published 15 October 2003) Calorimetry has become a well-understood, powerful, and versatile measurement method. Besides perfecting this technique to match increasingly demanding operation at high-energy particle accelerators, physicists are developing low-temperature calorimeters to extend detection down to ever lower energies, and atmospheric and deep-sea calorimeters to scrutinize the universe up to the highest energies. The authors summarize the state of the art, with emphasis on the physics of the detectors and innovative technologies. CONTENTS VI. Citius, Altius, Fortius 1280 A. Introduction 1280 B. Atmospheric calorimeters 1280 I. Introduction 1243 1. Setting the energy scale 1283 II. Electromagnetic Calorimetry 1244 2. Energy resolution 1283 A. Physics of the electromagnetic cascade 1244 C. Deep-water calorimeters 1283 B. Energy resolution of electromagnetic VII. Conclusions 1284 calorimeters 1246 Acknowledgments 1284 1. Stochastic term 1247 References 1284 2. Noise term 1247 3. Constant term 1247 4. Additional contributions 1248 C. Main techniques and examples of facilities 1249 I. INTRODUCTION 1. Homogeneous calorimeters 1249 a. Semiconductor calorimeters 1249 Calorimetry is an ubiquitous detection principle in b. Cherenkov calorimeters 1250 particle physics. Originally invented for the study of c. Scintillation calorimeters 1251 cosmic-ray phenomena, this method was developed and d. Noble-liquid calorimeters 1254 perfected for accelerator-based particle physics experi- 2. Sampling calorimeters 1256 mentation primarily in order to measure the energy of a. Scintillation sampling calorimeters 1257 electrons, photons, and hadrons. Calorimeters are b. Gas sampling calorimeters 1257 blocks of instrumented material in which particles to be c. -
Neutrino Oscillations: T2k and Na61 Experiments, R&D
NEUTRINO OSCILLATIONS: T2K AND NA61 EXPERIMENTS, R&D TOWARDS A FUTURE NEUTRINO PROGRAM 1 Research Plan The field of neutrino physics is certainly one of the most active in particle physics today. It is by now well established that neutrinos have mass and that the three families mix. In the minimal Standard Model, neutrinos are massless; massive neutrinos require either a new ad- hoc conservation law or new phenomena beyond the present framework, with a possible link to the grand unification scale via the see-saw mechanism. A deep field of research is thus open, that could last several decades and culminate with the discovery of leptonic CP violation – a key ingredient in the understanding of the baryon- anti-baryon asymmetry of the universe. Because observation of CP violation in neutrino oscillations requires appearance experiments, accessible at accelerators only, an important investment in accelerator-based neutrino beams and experiments is called for. The CHIPP Roadmap considers neutrino physics as one of the three pillars of particle physics in Switzerland, and so does the 15 years research plan of the DPNC at University of Geneva1. The neutrino group at DPNC has been actively involved in this quest since the nomination of Prof. A. Blondel in early 2000, where participation in the HARP experiment at CERN led us to the K2K experiment in Japan, in which the first observation of neutrino oscillation with a neutrino beam was achieved. The group received an added boost with the nomination of Alessandro Bravar (MER) in 2006. The research program comprises a progression of on- going experiments and far-reaching R&D activity as described in the SNF reports of October 2007 and October 2008. -
Macbook Were Made for Each Other
Congratulations, you and your MacBook were made for each other. Say hello to your MacBook. www.apple.com/macbook Built-in iSight camera and iChat Video chat with friends and family anywhere in the world. Mac Help isight Finder Browse your files like you browse your music with Cover Flow. Mac Help finder MacBook Mail iCal and Address Book Manage all your email Keep your schedule and accounts in one place. your contacts in sync. Mac Help Mac Help mail isync Mac OS X Leopard www.apple.com/macosx Time Machine Quick Look Spotlight Safari Automatically Instantly preview Find anything Experience the web back up and your files. on your Mac. with the fastest restore your files. Mac Help Mac Help browser in the world. Mac Help quick look spotlight Mac Help time machine safari iLife ’09 www.apple.com/ilife iPhoto iMovie GarageBand iWeb Organize and Make a great- Learn to play. Create custom search your looking movie in Start a jam session. websites and publish photos by faces, minutes or edit Record and mix them anywhere with places, or events. your masterpiece. your own song. a click. iPhoto Help iMovie Help GarageBand Help iWeb Help photos movie record website Contents Chapter 1: Ready, Set Up, Go 9 What’s in the Box 9 Setting Up Your MacBook 16 Putting Your MacBook to Sleep or Shutting It Down Chapter 2: Life with Your MacBook 20 Basic Features of Your MacBook 22 Keyboard Features of Your MacBook 24 Ports on Your MacBook 26 Using the Trackpad and Keyboard 27 Using the MacBook Battery 29 Getting Answers Chapter 3: Boost Your Memory 35 Installing Additional