Trigger and Data Acquisition
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HERA Collisions CERN LHC Magnets
The Gallex (gallium-based) solar neutrino experiment in the Gran Sasso underground Laboratory in Italy has seen evidence for neutrinos from the proton-proton fusion reaction deep inside the sun. A detailed report will be published in our next edition. again, with particles taken to 26.5 aperture models are also foreseen to GeV and initial evidence for electron- CERN test coil and collar assemblies and a proton collisions being seen. new conductor distribution will further Earlier this year, the big Zeus and LHC magnets improve multipole components. H1 detectors were moved into A number of other models and position to intercept the first HERA With test magnets for CERN's LHC prototypes are being built elsewhere collisions, and initial results from this proton-proton collider regularly including a twin-aperture model at new physics frontier are eagerly attaining field strengths which show the Japanese KEK Laboratory and awaited. that 10 Tesla is not forbidden terri another in the Netherlands (FOM-UT- tory, attention turns to why and NIHKEF). The latter will use niobium- where quenches happen. If 'training' tin conductor, reaching for an even can be reduced, superconducting higher field of 11.5 T. At KEK, a magnets become easier to commis single aperture configuration was sion. Tests have shown that successfully tested at 4.3 K, reaching quenches occur mainly at the ends of the short sample limit of the cable the LHC magnets. This should be (8 T) in three quenches. This magnet rectifiable, and models incorporating was then shipped to CERN for HERA collisions improvements will soon be reassem testing at the superfluid helium bled by the industrial suppliers. -
Muon Bundles As a Sign of Strangelets from the Universe
Draft version October 19, 2018 Typeset using LATEX default style in AASTeX61 MUON BUNDLES AS A SIGN OF STRANGELETS FROM THE UNIVERSE P. Kankiewicz,1 M. Rybczynski,´ 1 Z. W lodarczyk,1 and G. Wilk2 1Institute of Physics, Jan Kochanowski University, 25-406 Kielce, Poland 2National Centre for Nuclear Research, Department of Fundamental Research, 00-681 Warsaw, Poland Submitted to ApJ ABSTRACT Recently the CERN ALICE experiment, in its dedicated cosmic ray run, observed muon bundles of very high multiplicities, thereby confirming similar findings from the LEP era at CERN (in the CosmoLEP project). Originally it was argued that they apparently stem from the primary cosmic rays with a heavy masses. We propose an alternative possibility arguing that muonic bundles of highest multiplicity are produced by strangelets, hypothetical stable lumps of strange quark matter infiltrating our Universe. We also address the possibility of additionally deducing their directionality which could be of astrophysical interest. Significant evidence for anisotropy of arrival directions of the observed high multiplicity muonic bundles is found. Estimated directionality suggests their possible extragalactic provenance. Keywords: astroparticle physics: cosmic rays: reference systems arXiv:1612.04749v2 [hep-ph] 17 Mar 2017 Corresponding author: M. Rybczy´nski [email protected], [email protected], [email protected], [email protected] 2 Kankiewicz et al. 1. INTRODUCTION Cosmic ray physics is our unique source of information on events in the energy range which will never be accessible in Earth-bound experiments Dar & De Rujula(2008); Letessier-Selvon & Stanev(2011). This is why one of the most important aspects of their investigation is the understanding of the primary cosmic ray (CR) flux and its composition. -
India-CMS Newsletter Member Institutes/ Universities of India-CMS
India-CMS Newsletter Member Institutes/ Universities of India-CMS Vol 1. No. 1, July 2015 1. Nuclear Physics Division (NPD) Bhabha Atomic Research Center (BARC) Mumbai http://www.barc.gov.in/ First volume produced at: 2. Indian Institute of Science Education and Research (IISER) Department of Physics Pune http://www.iiserpune.ac.in Panjab University Sector 14 Chandigarh - 160014 3. Indian Institute of Technology (IIT), Bhubaneswar Bhubaneswar http:// www.iitbbs.ac.in 4. Department of Physics Indian Institute of Technology (IIT), Bombay Mumbai http://www.iitb.ac.in/en/education/academic-divisions 5. Indian Institute of Technology (IIT), Madras Chennai https://www.iitm.ac.in 6. School of Physical Sciences National Institute of Science Education and Research (NISER), Edited and Compiled by: Bhubaneswar http://physics.niser.ac.in/ Manjit Kaur Department of Physics 7. Department of Physics Panjab University Panjab University Chandigarh Chandigarh http://physics.puchd.ac.in/ [email protected] 8. Division of High Energy Nuclear and Particle Physics Ajit Mohanty Saha Institute of Nuclear Physics (SINP) Director Kolkata http://www.saha.ac.in/web/henppd-home Saha Institute of Nuclear Physics (SINP) Kolkatta 9. Department of High Energy Physics [email protected] Tata Institute of Fundamental Research (TIFR), Mumbai http://www.tifr.res.in/ ~dhep/ Abhimanyu Chawla Department of Physics 10. Department of Physics & Astrophysics Panjab University University of Delhi Chandigarh Delhi http://www.du.ac.in/du/index.php?page=physics-astrophysics [email protected] 11. Visva Bharti Santiniketan, West Bengal 731204 http://www.visvabharati.ac.in/Address.html 1 2 Contents Message ........................................................................................................................................................ 3 Message ....................................................................................................................................................... -
A BOINC-Based Volunteer Computing Infrastructure for Physics Studies At
Open Eng. 2017; 7:379–393 Research article Javier Barranco, Yunhai Cai, David Cameron, Matthew Crouch, Riccardo De Maria, Laurence Field, Massimo Giovannozzi*, Pascal Hermes, Nils Høimyr, Dobrin Kaltchev, Nikos Karastathis, Cinzia Luzzi, Ewen Maclean, Eric McIntosh, Alessio Mereghetti, James Molson, Yuri Nosochkov, Tatiana Pieloni, Ivan D. Reid, Lenny Rivkin, Ben Segal, Kyrre Sjobak, Peter Skands, Claudia Tambasco, Frederik Van der Veken, and Igor Zacharov LHC@Home: a BOINC-based volunteer computing infrastructure for physics studies at CERN https://doi.org/10.1515/eng-2017-0042 Received October 6, 2017; accepted November 28, 2017 1 Introduction Abstract: The LHC@Home BOINC project has provided This paper addresses the use of volunteer computing at computing capacity for numerical simulations to re- CERN, and its integration with Grid infrastructure and ap- searchers at CERN since 2004, and has since 2011 been plications in High Energy Physics (HEP). The motivation expanded with a wider range of applications. The tradi- for bringing LHC computing under the Berkeley Open In- tional CERN accelerator physics simulation code SixTrack frastructure for Network Computing (BOINC) [1] is that enjoys continuing volunteers support, and thanks to vir- available computing resources at CERN and in the HEP tualisation a number of applications from the LHC ex- community are not sucient to cover the needs for nu- periment collaborations and particle theory groups have merical simulation capacity. Today, active BOINC projects joined the consolidated LHC@Home BOINC project. This together harness about 7.5 Petaops of computing power, paper addresses the challenges related to traditional and covering a wide range of physical application, and also virtualized applications in the BOINC environment, and particle physics communities can benet from these re- how volunteer computing has been integrated into the sources of donated simulation capacity. -
Cosmic-Ray Studies with Experimental Apparatus at LHC
S S symmetry Article Cosmic-Ray Studies with Experimental Apparatus at LHC Emma González Hernández 1, Juan Carlos Arteaga 2, Arturo Fernández Tellez 1 and Mario Rodríguez-Cahuantzi 1,* 1 Facultad de Ciencias Físico Matemáticas, Benemérita Universidad Autónoma de Puebla, Av. San Claudio y 18 Sur, Edif. EMA3-231, Ciudad Universitaria, 72570 Puebla, Mexico; [email protected] (E.G.H.); [email protected] (A.F.T.) 2 Instituto de Física y Matemáticas, Universidad Michoacana, 58040 Morelia, Mexico; [email protected] * Correspondence: [email protected] Received: 11 September 2020; Accepted: 2 October 2020; Published: 15 October 2020 Abstract: The study of cosmic rays with underground accelerator experiments started with the LEP detectors at CERN. ALEPH, DELPHI and L3 studied some properties of atmospheric muons such as their multiplicity and momentum. In recent years, an extension and improvement of such studies has been carried out by ALICE and CMS experiments. Along with the LHC high luminosity program some experimental setups have been proposed to increase the potential discovery of LHC. An example is the MAssive Timing Hodoscope for Ultra-Stable neutraL pArticles detector (MATHUSLA) designed for searching of Ultra Stable Neutral Particles, predicted by extensions of the Standard Model such as supersymmetric models, which is planned to be a surface detector placed 100 meters above ATLAS or CMS experiments. Hence, MATHUSLA can be suitable as a cosmic ray detector. In this manuscript the main results regarding cosmic ray studies with LHC experimental underground apparatus are summarized. The potential of future MATHUSLA proposal is also discussed. Keywords: cosmic ray physics at CERN; atmospheric muons; trigger detectors; muon bundles 1. -
The Cell Geometry Is Adapted to the Manufacturing Process. One Side Of
R&D for the Future 443 The cell geometry is adapted to the manufacturing process. One side of the cell carries all the features required for the RF, whereas the other side is flat for bonding (Fig. 12.11). The cells are diamond machined, joined by diffusion bonding under hydrogen at about 1000°C and vacuum baked at 650°C. With exacting machining tolerances, typically in the 1 µm range, the tuning of the final structure is avoided. A number of test facilities is in operation worldwide including those at CERN which houses the only facility modelling the two-beam scheme in addition to a number of test stands powered by klystrons for high turn-around of testing structure variants. Nominal accelerating gradients of 100 MV/m have been achieved in the accelerating structures under development in a worldwide collaboration with the required low break-down rate while the PETSs have been tested at the nominal output power of 150 MW. However, more variants of these two structures have to be built and examined to address HOM damping, lifetime, breakdown statistics, industrial-scale fabrication, and better understanding of the break-down mechanisms. The Next Energy Frontier e+e− Collider: Innovation in Detectors Lucie Linssen Throughout the history of particle physics, both protons and electrons, with their respective antiparticles, have been used extensively for high energy colliders [Box 4.1]. The merits and difficulties of physics research with high luminosity proton–proton colliders are briefly described in the Box 8.3. Electrons, in contrast to protons, are genuine elementary particles. Apart from initial-state radiation and beamstrahlung effects (see below), they provide very good knowledge of the initial state of the collision. -
QCD Studies at L3
QCD Studies at L3 Swagato Banerjee Tata Institute of Fundamental Research Mumbai 400 005 2002 QCD Studies at L3 Swagato Banerjee Tata Institute of Fundamental Research Mumbai 400 005 A Thesis submitted to the University of Mumbai for the degree of Doctor of Philosophy in Physics March, 2002 To my parents Acknowledgement It has been an extremely enlightening and enriching experience working with Sunanda Banerjee, supervisor of this thesis. I would like to thank him for his forbearance and encouragement and for teaching me the different aspects of the subject with lots of patience. I thank all the members of the Department of High Energy Physics of Tata Institute of Fundamental Research (TIFR) for providing various facilities and support, and ideal ambiance for research. In particular, I would like to thank B.S. Acharya, T. Aziz, Sudeshna Banerjee, B.M. Bellara, P.V. Deshpande, S.T. Divekar, S.N. Ganguli, A. Gurtu, M.R. Krishnaswamy, K. Mazumdar, M. Maity, N.K. Mondal, V.S. Narasimham, P.M. Pathare, K. Sudhakar and S.C. Tonwar. Asesh Dutta, Dilip Ghosh, S. Gupta, Krishnendu Mukherjee, Sreerup Ray Chaudhuri, D.P. Roy, Sourov Roy, Gavin Salam and K. Sridhar provided valuable theoretical insight on various occasions. My heartfelt thanks to them. I thank the European Organisation for Nuclear Research (CERN) for its kind hospitality and all the members of the Large Electron Positron (LEP) accelerator group for successful operation over the last decade. The members of the L3 collaboration and the LEP QCD Working Group provided me a stim- ulating working environment. In particular, I thank Pedro Abreu, Satyaki Bhattacharya, Gerard Bobbink, Ingrid Clare, Robert Clare, Glen Cowan, Aaron Dominguez, Dominique Duchesneau, John Field, Ian Fisk, Roger Jones, Mehnaz Hafeez, Stephan Kluth, Wolfgang Lohmann, Wes- ley Metzger, Peter Molnar, Oliver Passon, Martin Pohl, Subir Sarkar, Chris Tully and Micheal Unger. -
The a to Z of Accelerators
present explanation for this behav The long timescale needed to terparts. But superconductivity iour is that superconductivity exists produce acceptable conductors of above 77K provides a powerful in many discrete regions within niobium-tin (10-12 years) following stimulant to solve the technological the sample but only weak coupling its discovery in 1962 inevitably problems of dealing with brittle exists between these regions. This comes to mind in assessing the materials. The next few months weak coupling is strongly dimin potential timeîscales for developing could give us many more surprises ished by an external field. Electro high field magnets with the new in an area where none were sus magnetic and structural character materials. These new oxides, like pected only a few months ago. izations of these compounds are niobium-tin and the other A15 The discovery of Bednorz and proceeding furiously and we may compounds are inherently brittle Muller has given a profound new soon expect to know whether this and this is bound to affect their stimulus to superconductivity and percolative nature of the supercon application in magnets, just as the last discovery has surely not ductivity is inherent in the material large scale construction of niobium- yet been made. or results from the way present tin magnets has lagged behind samples are being prepared. their ductile niobium-titanium coun The A to Z of accelerators With great skill, the organizers physics but this information was 1965. The attendance of over of the 1987 Particle Accelerator surpassed in volume by reports 1100 was another reflection of Conference arranged a vast pro from the many other areas where the wealth of activity in the field. -
Learning Physics from ALEPH Events
Learning Physics from ALEPH Events This document is an adaptation of the Web pages created by Joe Rothberg and Henri Videau at CERN. These pages can be found at http://aleph.web.cern.ch/aleph/educ/Welcome.html. Last updated: PTD, 5/Oct/2007 1 Introduction The aim of the following project is to provide some means for you to improve your knowledge of particle physics by studying some real data recently collected in the ALEPH experiment. To make it possible we provide some description of the experiment, of its detector and of some physics topics. It will help greatly if you have a copy of a recent particle physics text book to help you with any new concepts. A suggested text is “Introduction to High Energy Physics” by D.H.Perkins. You will need to access the world wide web throughout this project. Various URL’s (internet addresses) will be provided where you can find additional information on specific points. It is highly recommended that you take advantage of this extra information. You will also need access to your Windows account on the lab PC’s, so make sure you have your username validated in advance for this. 2 The Project The project is intended to require three days (21 hours) of study and work, with an additional 6 hours to write up. 1. On day one you should read the sections on “The LEP Collider”, “The ALEPH Exper- iment” and on “Starting with PAW”. After these sections are understood, there are a set of questions to be answered and the answers are to be included in your final report. -
Studies of Jet Energy Corrections at the CMS Experiment and Their Automation
Master’s thesis Theoretical and Computational Methods Studies of jet energy corrections at the CMS experiment and their automation Adelina Lintuluoto February 2021 Supervisor: Asst. prof. Mikko Voutilainen Advisor: Dr. Clemens Lange Examiners: Asst. prof. Mikko Voutilainen Dr. Kati Lassila-Perini UNIVERSITY OF HELSINKI DEPARTMENT OF PHYSICS PB 64 (Gustaf Hällströms gata 2a) 00014 Helsingfors universitet Tiedekunta – Fakultet – Faculty Koulutusohjelma – Utbildningsprogram – Degree programme Faculty of Science Master’s programme Opintosuunta – Studieinrikting – Study track Theoretical and computational methods Tekijä – Författare – Author Adelina Lintuluoto Työn nimi – Arbetets titel – Title Studies of jet energy corrections at the CMS experiment and their automation Työn laji – Arbetets art – Level Aika – Datum – Month and year Sivumäärä – Sidoantal – Number of pages Master’s thesis February 2021 69 Tiivistelmä – Referat – Abstract At the Compact Muon Solenoid (CMS) experiment at CERN (European Organization for Nuclear Research), the building blocks of the Universe are investigated by analysing the observed final-state particles resulting from high-energy proton-proton collisions. However, direct detection of final-state quarks and gluons is not possible due to a phenomenon known as colour confinement. Instead, event properties with a close correspondence with their distributions are studied. These event properties are known as jets. Jets are central to particle physics analysis and our understanding of them, and hence of our Universe, is dependent upon our ability to accurately measure their energy. Unfortunately, current detector technology is imprecise, necessitating downstream correction of measurement discrepancies. To achieve this, the CMS experiment employs a sequential multi-step jet calibration process. The process is performed several times per year, and more often during periods of data collection. -
Powermod™1 the Power You Need Sm
INTERNATIONAL JOURNAL OF HIGH-ENERGY PHYSICS 1 PowerMod™ The Power You Need sm High Voltage.Solid-State Modulators At Diversified Technologies, we manufacture leading-edge solid state, high power modulators from our patented, modular design. PowerMod™ systems can meet your pulsed power needs - at up to 200 kV, with peak currents up to 2000 A. V PowerMod*™ HVPM 100-300 30 MWModulator (36" x 48" x 60") PowerMod™ HVPM 20-150 Pulse: 20 kV, 100A, ljis/div PowerMod™ Modulators deliver the superior benefits of solid state technology including: • Very high operating efficiencies • < 3V/kV voltage drop accross the switch PowerMod™ HVPM 20-300 6 MW Modulator (19" x 30" x 24") • <1mA leakage • Arbitrary pusewidths from less than 1 jus to DC • PRFsto30kHz • Opening and closing operation Call us or visit our website today to learn more about the PowerMod™ line of solid-state high power systems. DIVERSIFIED TECHNOLOGIES, INC. 35 Wiggins Avenue Bedford, MA 01730 781-275-9444 www. d i vt ecs.com PowerMod*™ HVPM 2.5-150 3 75 KW Modulator (19" x 19.5" x 8.5") D 1999 Diversified Technologies, Inc. PowerMod™ is a trademark of Diversified Technologies, Inc. Contents Covering current developments in high- energy physics and related fields worldwide CERN Courier is distributed to Member State governments, institutes and laboratories affiliated with CERN, and to their personnel. It is published monthly except January and August, in English and French editions. The views expressed are not necessar ily those of the CERN management. CERN Editor: Gordon Fraser CERN, -
Baryon Production in Z Decay
Baryon Pro duction in Z Decay Christopher G Tully A DISSERTATION PRESENTED TO THE FACULTY OF PRINCETON UNIVERSITY IN CANDIDACY FOR THE DEGREE OF DOCTOR OF PHILOSOPHY RECOMMENDED FOR ACCEPTANCE BY THE DEPARTMENT OF PHYSICS January ABSTRACT How quarks b ecome conned into ordinary matter is a dicult theoretical question The p ointatwhich this o ccurs cannot b e measured by exp eriment but other prop erties related to connement can Baryon pro duction is a situation where one typ e of connement is chosen over another In this thesis pro duction rate measurements have b een p erformed for and baryons pro duced in hadronic decays of the Z The rates are low compared to meson pro duction but the particular prop erties of and decay allow these particles to be identied amongst the many mesons accompanying them The average number of and per hadronic Z decay was found to be D E N stat syst and D E N stat syst resp ectively These measurements take advantage of the unique photon detection capa bility of the L Exp eriment The rates are in agreement with those measured by other LEP detectors iii CONTENTS Abstract iii Acknowledgements v Intro duction Particle Creation and Detection Searching for Particle Decays Going Back in Time The History Behind SubNuclear Particles Quarks Discovery of the Pion The Quark Constituent Mo del