Collisions at Very High Energy
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The Five Common Particles
The Five Common Particles The world around you consists of only three particles: protons, neutrons, and electrons. Protons and neutrons form the nuclei of atoms, and electrons glue everything together and create chemicals and materials. Along with the photon and the neutrino, these particles are essentially the only ones that exist in our solar system, because all the other subatomic particles have half-lives of typically 10-9 second or less, and vanish almost the instant they are created by nuclear reactions in the Sun, etc. Particles interact via the four fundamental forces of nature. Some basic properties of these forces are summarized below. (Other aspects of the fundamental forces are also discussed in the Summary of Particle Physics document on this web site.) Force Range Common Particles It Affects Conserved Quantity gravity infinite neutron, proton, electron, neutrino, photon mass-energy electromagnetic infinite proton, electron, photon charge -14 strong nuclear force ≈ 10 m neutron, proton baryon number -15 weak nuclear force ≈ 10 m neutron, proton, electron, neutrino lepton number Every particle in nature has specific values of all four of the conserved quantities associated with each force. The values for the five common particles are: Particle Rest Mass1 Charge2 Baryon # Lepton # proton 938.3 MeV/c2 +1 e +1 0 neutron 939.6 MeV/c2 0 +1 0 electron 0.511 MeV/c2 -1 e 0 +1 neutrino ≈ 1 eV/c2 0 0 +1 photon 0 eV/c2 0 0 0 1) MeV = mega-electron-volt = 106 eV. It is customary in particle physics to measure the mass of a particle in terms of how much energy it would represent if it were converted via E = mc2. -
People and Things
Physics monitor People and things Books received CERN Council Bookshelf At the meeting of CERN's governing Future High Energy Colliders, Editor body, Council, in December, Luciano Weak Neutral Currents - The Zohreh Parsa, AIP Conference Maiani was elected the next Director Discovery of the Electro-Weak Force, Proceedings 397, ISBN 1-56396- General of the Organization, to take edited by David B. Cline, Addison 729-4 office on 1 January 1999, when the Wesley (Frontiers of Physics Series), current Director General, Chris ISBN 0-201-93347-0 Llewellyn Smith, will have completed Proceedings of a meeting held in his five year mandate. A Addison Wesley's Frontiers of Santa Barbara in October 1996 (see distinguished theorist, Luciano Physics Series began in 1961, and March 1997 issue of the CERN Maiani is currently President of the David Cline's anthology on weak Courier, page 16). Italian INFN and has been President neutral currents is the 97th volume in of CERN Council since January the series. 'Frontiers' books usually 1997. make extensive use of lecture notes The Interpretation of Quantum At the same meeting, leading or reprints, and Cline's volume takes Mechanics and the Measurement German science administrator and the latter route. It is divided into 9 Process, by Peter Mittelstaedt, head of Germany's CERN delegation chapters: The Weak Interaction Cambridge University Press 0 521 Hans C. Eschelbacher was elected Uncovered; Forty Years of Weak 55445 4 £30/$44.95 President of CERN Council for an Interactions; The Search for Other initial period of one year from 1 Forms of Weak Interaction; The January 1998, replacing Luciano Electroweak Interaction Picture A volume of interest to the more Maiani. -
A Tribute to Bj0rn Wiik General Distribution: Jacques Dallemagne, CERN, 1211 Geneva 23, Switzerland
W M£W HSmzS OF THS p\J\Q fAMM WQ 722S: w PCI mmm FOR w - FOR. SUN, HP, b£C, MMs, Direct single shot and DMA transfers On-board PCI MMU On-board PCI chained DMA controller Generic C library and drivers for Windows NT, MacOS, SOLARIS, Digital UNIX, HPUX, LINUX PWC ?02S: Tf/e FUNCTION COMMWE zeptAcenem FOR W VIC ?2S0 / 22S7 VME transparent mapping in the PCI memory space VME transparent slot 1 and arbiter Full VME master / slave Support D&, D16, D32, D64, direct transfers On-board VME linked list DMA controller The CES-f3Pnet (CES backplane Driver Network) offers an efficient interprocessor communication and synchronization mechanism, combining microsecond-level resolution and network-oriented services over the PVIC. The CES-l3Pnet offers three types of services to ensure efficient communications between CES processors: • An extension of the POSIX inter processes communication (shared memory semaphores - message queues) • An efficient and straightforward message passing system • A full TCF/IF stack using the PVIC as a network device W CjPtO: fi USeZ-PZOQMMMm Q6N6RAL PUZPK6 f/WT / OlUM PHC Stepper motor Controller Timer and counter 32-bit Input / Outputs (TTL or DIFF) Multiple lines PS 455 / PS 232 / PS 422 . Up to 6 GPIOs connected on a single PI02 with PMC carrier boards extension SOFTWARE C\6F Programming Kit for FPGA equations LynxOS and VxWorks drivers for PI02 family CES Geneva, Switzerland Tel: +41-22 792 57 45 Fax: +41-22 792 57 4d EMail: ces^ces.ch CES.D Germany Tel: +49-60 51 96 97 4 ' Fax: +49-60 51 96 97 35 CE6 Creative Electronic Systems 5A, 70 Route du Pont-3utin, CH-1213 Petit-Lancy 1, Switzerland Internet: http://www.ces.ch CREATIVE ELECTRONIC SYSTEMS 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. -
1.1. Introduction the Phenomenon of Positron Annihilation Spectroscopy
PRINCIPLES OF POSITRON ANNIHILATION Chapter-1 __________________________________________________________________________________________ 1.1. Introduction The phenomenon of positron annihilation spectroscopy (PAS) has been utilized as nuclear method to probe a variety of material properties as well as to research problems in solid state physics. The field of solid state investigation with positrons started in the early fifties, when it was recognized that information could be obtained about the properties of solids by studying the annihilation of a positron and an electron as given by Dumond et al. [1] and Bendetti and Roichings [2]. In particular, the discovery of the interaction of positrons with defects in crystal solids by Mckenize et al. [3] has given a strong impetus to a further elaboration of the PAS. Currently, PAS is amongst the best nuclear methods, and its most recent developments are documented in the proceedings of the latest positron annihilation conferences [4-8]. PAS is successfully applied for the investigation of electron characteristics and defect structures present in materials, magnetic structures of solids, plastic deformation at low and high temperature, and phase transformations in alloys, semiconductors, polymers, porous material, etc. Its applications extend from advanced problems of solid state physics and materials science to industrial use. It is also widely used in chemistry, biology, and medicine (e.g. locating tumors). As the process of measurement does not mostly influence the properties of the investigated sample, PAS is a non-destructive testing approach that allows the subsequent study of a sample by other methods. As experimental equipment for many applications, PAS is commercially produced and is relatively cheap, thus, increasingly more research laboratories are using PAS for basic research, diagnostics of machine parts working in hard conditions, and for characterization of high-tech materials. -
Chapter 3 the Fundamentals of Nuclear Physics Outline Natural
Outline Chapter 3 The Fundamentals of Nuclear • Terms: activity, half life, average life • Nuclear disintegration schemes Physics • Parent-daughter relationships Radiation Dosimetry I • Activation of isotopes Text: H.E Johns and J.R. Cunningham, The physics of radiology, 4th ed. http://www.utoledo.edu/med/depts/radther Natural radioactivity Activity • Activity – number of disintegrations per unit time; • Particles inside a nucleus are in constant motion; directly proportional to the number of atoms can escape if acquire enough energy present • Most lighter atoms with Z<82 (lead) have at least N Average one stable isotope t / ta A N N0e lifetime • All atoms with Z > 82 are radioactive and t disintegrate until a stable isotope is formed ta= 1.44 th • Artificial radioactivity: nucleus can be made A N e0.693t / th A 2t / th unstable upon bombardment with neutrons, high 0 0 Half-life energy protons, etc. • Units: Bq = 1/s, Ci=3.7x 1010 Bq Activity Activity Emitted radiation 1 Example 1 Example 1A • A prostate implant has a half-life of 17 days. • A prostate implant has a half-life of 17 days. If the What percent of the dose is delivered in the first initial dose rate is 10cGy/h, what is the total dose day? N N delivered? t /th t 2 or e Dtotal D0tavg N0 N0 A. 0.5 A. 9 0.693t 0.693t B. 2 t /th 1/17 t 2 2 0.96 B. 29 D D e th dt D h e th C. 4 total 0 0 0.693 0.693t /th 0.6931/17 C. -
Electron - Positron Annihilation
Electron - Positron Annihilation γ µ K Z − − − + + + − − − + + + − − − − + + + − − − + + + + W ν h π D. Schroeder, 29 October 2002 OUTLINE • Electron-positron storage rings • Detectors • Reaction examples e+e− −→ e+e− [Inventory of known particles] e+e− −→ µ+µ− e+e− −→ q q¯ e+e− −→ W +W − • The future:Linear colliders Electron-Positron Colliders Hamburg Novosibirsk 11 GeV 12 GeV 47 GeV Geneva 200 GeV Ithaca Tokyo Stanford 12 GeV 64 GeV 8 GeV 12 GeV 30 GeV 100 GeV Beijing 12 GeV 4 GeV Size (R) and Cost ($) of an e+e− Storage Ring βE4 $=αR + ( E = beam energy) R d $ βE4 Find minimum $: 0= = α − dR R2 β =⇒ R = E2, $=2 αβ E2 α SPEAR: E = 8 GeV, R = 40 m, $ = 5 million LEP: E = 200 GeV, R = 4.3 km, $ = 1 billion + − + − Example 1: e e −→ e e e− total momentum = 0 θ − total energy = 2E e e+ Probability(E,θ)=? e+ E-dependence follows from dimensional analysis: density = ρ− A density = ρ+ − + × 2 Probability = (ρ− ρ+ − + A) (something with units of length ) ¯h ¯hc When E m , the only relevant length is = e p E 1 =⇒ Probability ∝ E2 at SPEAR Augustin, et al., PRL 34, 233 (1975) 6000 5000 4000 Ecm = 4.8 GeV 3000 2000 Number of Counts 1000 Theory 0 −0.8 −0.40 0.40.8 cos θ Prediction for e+e− −→ e+e− event rate (H. J. Bhabha, 1935): event dσ e4 1 + cos4 θ 2 cos4 θ 1 + cos2 θ ∝ = 2 − 2 + rate dΩ 32π2E2 4 θ 2 θ 2 cm sin 2 sin 2 Interpretation of Bhabha’sformula (R. -
Bhabha-Scattering Consider the Theory of Quantum Electrodynamics for Electrons, Positrons and Photons
Quantum Field Theory WS 18/19 18.01.2019 and the Standard Model Prof. Dr. Owe Philipsen Exercise sheet 11 of Particle Physics Exercise 1: Bhabha-scattering Consider the theory of Quantum Electrodynamics for electrons, positrons and photons, 1 1 L = ¯ iD= − m − F µνF = ¯ [iγµ (@ + ieA ) − m] − F µνF : (1) QED 4 µν µ µ 4 µν Electron (e−) - Positron (e+) scattering is referred to as Bhabha-scattering + − + 0 − 0 (2) e (p1; r1) + e (p2; r2) ! e (p1; s1) + e (p2; s2): i) Identify all the Feynman diagrams contributing at tree level (O(e2)) and write down the corresponding matrix elements in momentum space using the Feynman rules familiar from the lecture. ii) Compute the spin averaged squared absolut value of the amplitudes (keep in mind that there could be interference terms!) in the high energy limit and in the center of mass frame using Feynman gauge (ξ = 1). iii) Recall from sheet 9 that the dierential cross section of a 2 ! 2 particle process was given as dσ 1 = jM j2; (3) dΩ 64π2s fi in the case of equal masses for incoming and outgoing particles. Use your previous result to show that the dierential cross section in the case of Bhabha-scattering is dσ α2 1 + cos4(θ=2) 1 + cos2(θ) cos4(θ=2) = + − 2 ; (4) dΩ 8E2 sin4(θ=2) 2 sin2(θ=2) where e2 is the ne-structure constant, the scattering angle and E is the respective α = 4π θ energy of electron and positron in the center-of-mass system. Hint: Use Mandelstam variables. -
QCD at Colliders
Particle Physics Dr Victoria Martin, Spring Semester 2012 Lecture 10: QCD at Colliders !Renormalisation in QCD !Asymptotic Freedom and Confinement in QCD !Lepton and Hadron Colliders !R = (e+e!!hadrons)/(e+e!"µ+µ!) !Measuring Jets !Fragmentation 1 From Last Lecture: QCD Summary • QCD: Quantum Chromodymanics is the quantum description of the strong force. • Gluons are the propagators of the QCD and carry colour and anti-colour, described by 8 Gell-Mann matrices, !. • For M calculate the appropriate colour factor from the ! matrices. 2 2 • The coupling constant #S is large at small q (confinement) and large at high q (asymptotic freedom). • Mesons and baryons are held together by QCD. • In high energy collisions, jets are the signatures of quark and gluon production. 2 Gluon self-Interactions and Confinement , Gluon self-interactions are believed to give e+ q rise to colour confinement , Qualitative picture: •Compare QED with QCD •In QCD “gluon self-interactions squeeze lines of force into Gluona flux tube self-Interactions” ande- Confinementq , + , What happens whenGluon try self-interactions to separate two are believedcoloured to giveobjects e.g. qqe q rise to colour confinement , Qualitativeq picture: q •Compare QED with QCD •In QCD “gluon self-interactions squeeze lines of force into a flux tube” e- q •Form a flux tube, What of happensinteracting when gluons try to separate of approximately two coloured constant objects e.g. qq energy density q q •Require infinite energy to separate coloured objects to infinity •Form a flux tube of interacting gluons of approximately constant •Coloured quarks and gluons are always confined within colourless states energy density •In this way QCD provides a plausible explanation of confinement – but not yet proven (although there has been recent progress with Lattice QCD) Prof. -
The W and Z at LEP
50YEARSOFCERN The W and Z at LEP 1954-2004 The Large Electron Positron collider made significant contributions to the process of establishing the Standard Model as the basis for matter and 5 forces, and also built a platform for physics scenarios beyond the model. The Standard Model of particle physics is arguably one of the greatest achievements in physics in the 20th century. Within this framework the electroweak interactions, as introduced by Sheldon Glashow, Abdus Salam and Steven Weinberg, are formulated as an SU(2)xll(l) gauge field theory with the masses of the fundamental particles generated by the Higgs mechanism. Both of the first two crucial steps in establishing experimentally the electroweak part of the Standard Model occurred at CERN. These were the discovery of neutral currents in neutrino scattering by the Gargamelle collab oration in 1973, and only a decade later the discovery by the UA1 and UA2 collaborations of the W and Z gauge bosons in proton- antiproton collisions at the converted Super Proton Synchrotron (CERN Courier May 2003 p26 and April 2004 pl3). Establishing the theory at the quantum level was the next logical step, following the pioneering theoretical work of Gerard 't Hooft Fig. 1. The cover page and Martinus Veltman. Such experimental proof is a necessary (left) of the seminal requirement for a theory describing phenomena in the microscopic CERN yellow report world. At the same time, performing experimental analyses with high 76-18 on the physics precision also opens windows to new physics phenomena at much potential of a 200 GeV higher energy scales, which can be accessed indirectly through e+e~ collider, and the virtual effects. -
A Historical Review of the Discovery of the Quark and Gluon Jets
EPJ manuscript No. (will be inserted by the editor) JETS AND QCD: A Historical Review of the Discovery of the Quark and Gluon Jets and its Impact on QCD⋆ A.Ali1 and G.Kramer2 1 DESY, D-22603 Hamburg (Germany) 2 Universit¨at Hamburg, D-22761 Hamburg (Germany) Abstract. The observation of quark and gluon jets has played a crucial role in establishing Quantum Chromodynamics [QCD] as the theory of the strong interactions within the Standard Model of particle physics. The jets, narrowly collimated bundles of hadrons, reflect configurations of quarks and gluons at short distances. Thus, by analysing energy and angular distributions of the jets experimentally, the properties of the basic constituents of matter and the strong forces acting between them can be explored. In this review, which is primarily a description of the discovery of the quark and gluon jets and the impact of their obser- vation on Quantum Chromodynamics, we elaborate, in particular, the role of the gluons as the carriers of the strong force. Focusing on these basic points, jets in e+e− collisions will be in the foreground of the discussion and we will concentrate on the theory that was contempo- rary with the relevant experiments at the electron-positron colliders. In addition we will delineate the role of jets as tools for exploring other particle aspects in ep and pp/pp¯ collisions - quark and gluon densi- ties in protons, measurements of the QCD coupling, fundamental 2-2 quark/gluon scattering processes, but also the impact of jet decays of top quarks, and W ±, Z bosons on the electroweak sector. -
Probing 23% of the Universe at the Large Hadron Collider
Probing 23% of the Universe at the Large Hadron Collider Will Flanagan1 Advisor: Dr Teruki Kamon2 In close collaboration with Bhaskar Dutta2, Alfredo Gurrola2, Nikolay Kolev3, Tom Crockett2, Michael VanDyke2, and Abram Krislock2 1University of Colorado at Boulder, Cyclotron REU Program 2Texas A&M University 3University of Regina Introduction What is cosmologically significant about ‘focus Analysis With recent astronomical measurements, point’? We first decide which events we want to look for. χ~0 ~0 we know that 23% of the Universe is The 1is allowed to annihilate with itself since it is Since χ 1 is undetectable (otherwise it wouldn’t be ‘dark composed of dark matter, whose origin is its own antimatter particle. The χ~ 0 -χ~0 annihilation matter’!), we look for events with a 1 1 Red – Jet distribution unknown. Supersymmetry (SUSY), a leading cross section is typically too small (predicting a relic after MET cut large amount of missing transverse theory in particle physics, provides us with a cold dark χ~0 Z channel dark matter density that is too energy. Also, due to the nature of 1 u- matter candidate, the lightest supersymmetric particle Z0 large). The small µ of focus these decays (shown below) we also χ~0 (LSP). SUSY particles, including the LSP, can be 1 u point x require two energetic jets. 2 f 1 Ω ~0 ~h dx created at the Large Hadron Collider (LHC) at CERN. allows for a larger annihilation χ1 ∫ 0 σ v { ann g~ 2 energetic jets + 2 leptons We perform a systematic study to characterize the cross section for our dark 0.23 698 u- + MET 2 g~ SUSY signals in the "focus point" region, one of a few matter candidate by opening πα ~ u - σ annv = 2 u l cosmologically-allowed parameter regions in our SUSY up the ‘Z channel’ (pictured 321 8M χ~0 l+ 0.9 pb 2 ~+ model. -
Pos(LL2018)010 -Right Asymmetry and the Relative § , Lidia Kalinovskaya, Ections
Electroweak radiative corrections to polarized Bhabha scattering PoS(LL2018)010 Andrej Arbuzov∗† Bogoliubov Laboratory of Theoretical Physics, JINR, Dubna, 141980 Russia E-mail: [email protected] Dmitri Bardin,‡ Yahor Dydyshka, Leonid Rumyantsev,§ Lidia Kalinovskaya, Renat Sadykov Dzhelepov Laboratory of Nuclear Problems, JINR, Dubna, 141980 Russia Serge Bondarenko Bogoliubov Laboratory of Theoretical Physics, JINR, Dubna, 141980 Russia In this report we present theoretical predictions for high-energy Bhabha scattering with taking into account complete one-loop electroweak radiative corrections. Longitudinal polarization of the initial beams is assumed. Numerical results for the left-right asymmetry and the relative correction to the distribution in the scattering angle are shown. The results are relevant for several future electron-positron collider projects. Loops and Legs in Quantum Field Theory (LL2018) 29 April 2018 - 04 May 2018 St. Goar, Germany ∗Speaker. †Also at the Dubna University, Dubna, 141980, Russia. ‡deceased §Also at the Institute of Physics, Southern Federal University, Rostov-on-Don, 344090 Russia 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). https://pos.sissa.it/ EW RC to polarized Bhabha scattering Andrej Arbuzov 1. Introduction The process of electron-positron scattering known as the Bhabha scattering [1] is one of the + key processes in particle physics. In particular it is used for the luminosity determination at e e− colliders. Within the Standard Model the scattering of unpolarized electron and positrons has been thoroughly studied for many years [2–12]. Corrections to this process with polarized initial particles were discussed in [13, 14].