Fermilab's Tevatron & Large Hadron Collider (LHC) Teruki Kamon

Total Page:16

File Type:pdf, Size:1020Kb

Fermilab's Tevatron & Large Hadron Collider (LHC) Teruki Kamon FermilabFermilab’’ss TevatronTevatron && LargeLarge HadronHadron ColliderCollider (LHC)(LHC) Teruki Kamon PHYS 627 Taken from slides by Ron Moore, Paul Derwent, Mike Syphers (FNAL) (Apr 2005) Modified/updated by Teruki Kamon for PHYS 627 Hadron Collisions at the Tevatron and the LHC 1 AA littlelittle bitbit ofof EinsteinEinstein…… Recall the well-known equation: E = mc 2 Measure energy in “electron volts” = eV (1 eV ≈ 1.6 x 10−19 Joule) 2 Measure mass in units of eV/c … (1 eV/c2 ≈ 1.78 x 10−36 kg) …but often use units where c ≡ 1, so mass can also be measured in eV For a moving particle: 1 v 2 2 2 2 γ = β ≡ E = (mc ) + ( pc) = γ mc 1 − β 2 c 2 2 Total Energy = Rest Energy + Kinetic Energy E = mc + (γ − 1 )mc Ultra-relativistic: γ >> 1 can neglect rest mass Hadron Collisions at the Tevatron and the LHC 2 FixedFixed TargetTarget vs.vs. CollidersColliders w/ow/o calculuscalculus Hadron Collisions at the Tevatron and the LHC 3 FixedFixed TargetTarget vs.vs. CollidersColliders w/w/ calculuscalculus Fixed Target Center of Mass Energy Energy E s = 2mE ultrarelativistic limit Head-On Collision Energy E Energy E s = 2E Compare protons @ 1 TeV: Fixed Target: ECM = 43 GeV Collider: ECM = 2000 GeV Big advantage for colliders! ⇒ Most efficient use of beam energy for physics! Challenge to get a high collision rate to look for interesting (rare) processes Fixed target still essential for secondary beams: antiprotons, kaons, µ’s, ν’s Hadron Collisions at the Tevatron and the LHC 4 Hadron Collisions at the Tevatron and the LHC 5 σ int σ int σ int A 3.46 x 109 crossings Skip Hadron Collisions at the Tevatron and the LHC 6 LuminosityLuminosity N N L = f 1 2 Luminosity is measure of the collision rate in a collider 4πσ 2 − 2 −1 Units are cm s f is collision frequency 32 − 2 − 1 × Peak luminosity ~ 1.2 10 cm s N 1, N 2 are # particles in each beam 32 − 2 − 1 Goal ~ 4.0 ×10 cm s σ is beam size −24 2 32 − 2 − 1 − 1 10 cm = 1 barn; 10 cm s = 360 nb /hr To reach higher luminosity… More beam May be hard…Tevatron needs more antiprotons Higher collision frequency (more bunches) Not for Tevatron – will keep using 36 bunches of protons and antiprotons Smaller beam Tevatron beams are ~30 µm wide at interaction points Linear colliders have nm size beams All can be hard to achieve due to instabilities that may develop Want high luminosity to study rare processes Luminosity × Cross Section = Event Rate 32 −2 − 1 e.g., 1 × 10 cm s × 10 pb = 3.6 events/hr Hadron Collisions at the Tevatron and the LHC 7 ModelModel ofof AcceleratorAccelerator Accelerating device + magnetic field to bring it back to accelerate again += Hadron Collisions at the Tevatron and the LHC 8 Hadron Collisions at the Tevatron and the LHC 9 WhereWhere isis thethe FermilabFermilab?? Hadron Collisions at the Tevatron and the LHC 10 Looking Down on the Fermilab Accelerator Complex ~5 mi. CDF D0 Hadron Collisions at the Tevatron and the LHC 11 CloselyClosely LookingLooking DownDown onon thethe FermilabFermilab Wilson Hall Tevatron Main 1 km Injector Hadron Collisions at the Tevatron and the LHC 12 NuMI (120 GeV protons) MiniBoone (8 GeV) 1 6 2 3 7 5 4 9 Accelerator Highest Energy Cockroft Walton 750 keV 8 Linac 400 Mev 10 Booster 8 GeV Main injector 150 GeV TEVATRON 980 GeV MachineMachine EnergiesEnergies ((cc == 1)1) Comparing relativistic β, γ for electrons and protons at various energies… electron proton rest mass 511 keV 938 MeV Machine KE βγβγ Cockroft-Walton 750 keV 0.926794588 2.47 0.707389304 1.00 FNAL Linac 400 MeV 0.999999186 784 0.818829208 1.43 FNAL Booster 8 GeV 0.999999998 15657 0.994538328 9.53 Main Injector 150 GeV 1 293543 0.999980691 161 ILC 500 GeV 1 978475 0.999998247 534 Tevatron 980 GeV 1 1.918E+06 0.999999543 1046 LHC 7 TeV 1 1.761E+07 0.999999995 9596 VLHC? 100 TeV 1 1.957E+08 1 106611 1 keV = 103 eV 1 MeV = 106 eV 1 GeV = 109 eV 1 TeV = 1012 eV Mass of top quark ≈ 175 GeV Hadron Collisions at the Tevatron and the LHC 14 HiHi--riserise BuildingBuilding •25 keV H− ion source •750 keV Cockcroft- Walton accelerator Hadron Collisions at the Tevatron and the LHC 15 CockcroftCockcroft--WaltonWalton •25 keV H− ion source •750 keV Cockcroft-Walton accelerator Hadron Collisions at the Tevatron and the LHC 16 LinacLinac Accelerate H− ions to 400 MeV − 116 MeV Alvarez linac (201.25MHz) H ions 400 MeV side-coupled cavity linac (805 MHz) Hadron Collisions at the Tevatron and the LHC 17 BoosterBooster Booster: 8 GeV Synchrotron Runs at 15 Hz Stripper foil at injection removes electrons from H− ions Accelerates protons from 400 MeV to 8 GeV Most protons (>75%) going through Booster are delivered to MiniBoone (eventually NuMI) Hadron Collisions at the Tevatron and the LHC 18 Main Injector & Recycler Ring Recycler Main Injector Hadron Collisions at the Tevatron and the LHC 19 MainMain InjectorInjector (MI)(MI) Replaced Main Ring (formerly in Tevaron tunnel) Higher repetition rate for stacking pbars Simultaneous stacking and fixed target running Many operating modes 12 Pbar production: ~ 6-7 x 10 120-GeV protons to pbar target “Slip-stacking” – merge two booster batches of beam on 1 MI ramp cycle “Tevatron protons/pbars”: Accelerate 8 GeV to 150 GeV 9 Coalesce 7-9 proton bunches at 90% eff into “270-300 x 10 proton” bunch 9 Coalesce 5-7 pbar bunches at 75-90% eff into “20-80 x 10 antiproton” bunch Transfer 8-GeV protons/pbars to the Recycler Provide protons for neutrino production 8-GeV protons for MiniBoone 120-GeV protons for NuMI 120-GeV protons to Switchyard (fixed target area) Hadron Collisions at the Tevatron and the LHC 20 DebuncherDebuncher && AccemulatorAccemulator Debuncher Two rings Accumulator Hadron Collisions at the Tevatron and the LHC 21 PbarPbar (Antiproton)(Antiproton) SourceSource (1) > 6 x 1012 120-GeV protons per pulse strike Ni target every 2-3 sec; (2) Li lens (740 Tesla/m) collects negative secondaries; (3) Pulsed dipole “PMAG” bends pbars down AP-2 line to Debuncher ε≈(14-18) x 10−6 pbars/proton on target Pbars “debunched”, cooled briefly in Debuncher prior to Accumulator Hadron Collisions at the Tevatron and the LHC 22 PbarPbar (Antiproton)(Antiproton) SourceSource Stack rate = 6-14 mA/hr Depending on stack size; Limited by stochastic cooling systems in Accumulator Transverse beam size increases linearly with stack size - That’s a drawback… In a really good 24 hour period, nearly 200 x 1010 pbars can be accumulated. −12 −24 Pbar Production Rate = 3.3 x 10 g/day (Mpbar ≈ 1.67 x 10 g) 800 million years to make 1 g of antimatter! Hadron Collisions at the Tevatron and the LHC 23 TevatronTevatron OverviewOverview Proton-pbar collisions (Ebeam = 980 GeV) Revolution time ~ 21 µs Virtually all of the Tevatron magnets are superconducting (Cooled by liquid helium, operate at 4 K) 150 GeV beams are injected from MI Protons injected from P1 line at F17; Pbars injected from A1 line at E48 36 bunches of proton and pbars circulate in same beam pipe, but separated by “electrostatic separators” 3 trains of 12 bunches with 396 ns separation (see the next page) 2 low β (small beam size) intersection points (CDF and D0) 8 RF cavities (near F0) to keep beam in bucket, acceleration 1113 RF buckets (53.1 MHz ⇒ 18.8 ns bucket length) Hadron Collisions at the Tevatron and the LHC 24 ProtonProton BunchBunch PositionsPositions 3 trains of 12 bunches with 396 ns separation P12 P13 P1 P24 P25 P36 Hadron Collisions at the Tevatron and the LHC 25 ProtonsProtons andand PbarsPbars atat HEPHEP Proton Collide Collide bunches @ CDF @ D0 P1-P12 A25-A36 A13-A24 A P13-P24 A1-A12 A25-A36 2 4~ P25-P36 A13-A24 A1-A12 P1 3 P25~P36 Hadron Collisions at the Tevatron and the LHC 26 ProtonProton--PbarPbar CollisionCollision PointPoint Hadron Collisions at the Tevatron and the LHC 27 First Collisions at the Tevatron Run 493 Event 11 Run 493 Event 15 October 13, 1985 Hadron Collisions at the Tevatron and the LHC 28 LargeLarge HadronHadron ColliderCollider HighlightsHighlights ~27km circumference 1232 bends Main bends are 14.3 meters long The strength of each magnet is 8.33 Tesla Huge synchrotron radiation loss. SynchrotronSynchrotron RadiationRadiation Accelerated charges produce radiation. r e ⎡ nr × (nr × β&)⎤ Useful equations for ideal conditions in SI E a = ⎢ ⎥ c R ⎣ ⎦ ret qvB v = r c r r c r 2 & S = E × B = E nr γm 4π 4π a 2 2 dP c r 2 e 2 e 2 = RE = nr × (nr × β&) = vr& sin 2 Θ dΩ 4π a 4πc 4πc 3 2 2 e 2 P = vr& 3 c 3 Above we integrated over the angle Θ, and below switched to more familiar units SI 2 r 2 q ⎛ dp ⎞ 4 1 dE dpr = ⎜ ⎟ ⎛ q ⎞ 2 2 Pγ 2 3 From here were can get if << 6π m c dt Pγ ∝ ⎜ ⎟ U B ε ο ⎝ ⎠ ⎝ m ⎠ c dτ dτ Go to, for example, Jackson’s Classical Electrodynamics book, find more convenient expression in terms of v, ρ, γ Hadron Collisions at the Tevatron and the LHC 31.
Recommended publications
  • Supersymmetry Searches at the Tevatron
    SUPERSYMMETRY SEARCHES AT THE TEVATRON For CDF and DØ collaborations R. Demina Department of Physics and Astronomy, University of Rochester, Rochester, USA, 14627 CDF and DØ collaborations analyzed up to 200 pb-1 of the delivered data in search for different supersymmetry signatures, so far with negative results. We present results on searches for chargino and neutralino associated production, squarks and gluinos, sbottom quarks, gauge mediated SUSY breaking and long lived heavy particles. Supersymmetry1 is a popular extension of the Standard Model originally suggested over 25 years ago. It postulates the symmetry between fermionic and bosonic degrees of freedom. As a result a variety of hypothetical particles is introduced. With presently available experimental data physicists were able to prove that if supersymmetric particles exist they must be heavier than their Standard Model partners2. In other words the Supersymmetry is broken. One possible exception is supersymmetric top quark (stop), which still has a chance to be lighter or of the same mass as top quark. With 2-4 fb-1 of data Tevatron experiments will be able to extend the limit on stop mass above that of top quark or discover it and thus establish the Supersymmetry3. Theory suggests several possible scenarios of Supersymmetry breaking mediated by gravitational or gauge interactions. In gravity mediated scenarios the number of free parameters in the model is reduced to five because of the unification of masses and couplings imposed at the grand unification scale. These parameters are M0 (M½) – masses of all bosons (fermions) at GUT scale, A0- trilinear coupling and µ0 – something Higgs and tan(β) – ratio of vacuum expectations of the Higgs doublet.
    [Show full text]
  • NRP-3 the Effect of Beryllium Interaction with Fast Neutrons on the Reactivity of Etrr-2 Research Reactor
    Seventh Conference of Nuclear Sciences & Applications 6-10 February 2000, Cairo, Egypt NRP-3 The Effect Of Beryllium Interaction With Fast Neutrons On the Reactivity Of Etrr-2 Research Reactor Moustafa Aziz and A.M. EL Messiry National Center for Nuclear Safety Atomic Energy Autho , Cairo , Egypt ABSTRACT The effect of beryllium interactions with fast neutrons is studied for Etrr_2 research reactors. Isotope build up inside beryllium blocks is calculated under different irradiation times. A new model for the Etrr_2 research reactor is designed using MCNP code to calculate the reactivity and flux change of the reactor due to beryllium poison. Key words: Research Reactors , Neutron Flux , Beryllium Blocks, Fast Neutrons and Reactivity INTRODUCTION Beryllium irradiated by fast neutrons with energies in the range 0.7-20 Mev undergoes (n,a) and (n,2n) reactions resulting in subsequent formation of the isotopes lithium (Li-6), tritium (H-3) and helium (He-3 and He-4 ). Beryllium interacts with fast neutrons to produce 6He that decay 6 6 ( T!/2 =0.8 s) to produce Li . Li interacts with neutron to produce tritium which suffer /? (T1/2 = 12.35 year) decay and converts to 3He which finally interact with neutron to produce tritium. These processes some times defined as Beryllium poison. Negative effect of this process are met whenever beryllium is used in a thermal reactor as a reflector or moderator . Because of their large thermal neutron absorption cross sections , the buildup of He-3 and Li-6 concentrations ,initiated by the Be(n,a) reaction , results in large negative reactivities which alter the reactivity , flux and power distributions.
    [Show full text]
  • The Large Hadron Collider Lyndon Evans CERN – European Organization for Nuclear Research, Geneva, Switzerland
    34th SLAC Summer Institute On Particle Physics (SSI 2006), July 17-28, 2006 The Large Hadron Collider Lyndon Evans CERN – European Organization for Nuclear Research, Geneva, Switzerland 1. INTRODUCTION The Large Hadron Collider (LHC) at CERN is now in its final installation and commissioning phase. It is a two-ring superconducting proton-proton collider housed in the 27 km tunnel previously constructed for the Large Electron Positron collider (LEP). It is designed to provide proton-proton collisions with unprecedented luminosity (1034cm-2.s-1) and a centre-of-mass energy of 14 TeV for the study of rare events such as the production of the Higgs particle if it exists. In order to reach the required energy in the existing tunnel, the dipoles must operate at 1.9 K in superfluid helium. In addition to p-p operation, the LHC will be able to collide heavy nuclei (Pb-Pb) with a centre-of-mass energy of 1150 TeV (2.76 TeV/u and 7 TeV per charge). By modifying the existing obsolete antiproton ring (LEAR) into an ion accumulator (LEIR) in which electron cooling is applied, the luminosity can reach 1027cm-2.s-1. The LHC presents many innovative features and a number of challenges which push the art of safely manipulating intense proton beams to extreme limits. The beams are injected into the LHC from the existing Super Proton Synchrotron (SPS) at an energy of 450 GeV. After the two rings are filled, the machine is ramped to its nominal energy of 7 TeV over about 28 minutes. In order to reach this energy, the dipole field must reach the unprecedented level for accelerator magnets of 8.3 T.
    [Show full text]
  • Three Extra Mirror Or Sequential Families: a Case for Heavy Higgs and Inert Doublet
    Three Extra Mirror or Sequential Families: a Case for Heavy Higgs and Inert Doublet Homero Mart´ınez,1 Alejandra Melfo,2, 3 Fabrizio Nesti,4 and Goran Senjanovi´c2 1CEA, Saclay, DSM-IRFU-SPP, France 2ICTP, Trieste, Italy 3U. de Los Andes, M´erida, Venezuela 4U. di Ferrara, Ferrara, Italy (Dated: October 24, 2018) We study the possibility of the existence of extra fermion families and an extra Higgs doublet. We find that requiring the extra Higgs doublet to be inert leaves space for three extra families, allowing for mirror fermion families and a dark matter candidate at the same time. The emerging scenario is very predictive: it consists of a Standard Model Higgs boson, with mass above 400 GeV, heavy new quarks between 340 and 500 GeV, light extra neutral leptons, and an inert scalar with a mass below MZ . PACS numbers: 14.65.Jk, 12.60.Fr, 14.60.Hi, 14.60.St Introduction. It may not be well known that the idea with regard to high precision analysis they behave exactly of parity restoration in weak interactions is as old as as ordinary fermions, and thus a reader who is uncom- the suggestion of its breakdown. In their classic paper, fortable with the above setbacks can view our study as Lee and Yang [1] proposed the existence of what we will referring to the more general question of whether the SM call mirror fermions, so as to make the world left-right can host three (or more) extra families. symmetric at high energies. By this they meant another If one defines the SM by its structure, i.e.
    [Show full text]
  • Anomalous Muon Magnetic Moment, Supersymmetry, Naturalness, LHC Search Limits and the Landscape
    OU-HEP-210415 Anomalous muon magnetic moment, supersymmetry, naturalness, LHC search limits and the landscape Howard Baer1∗, Vernon Barger2†, Hasan Serce1‡ 1Homer L. Dodge Department of Physics and Astronomy, University of Oklahoma, Norman, OK 73019, USA 2Department of Physics, University of Wisconsin, Madison, WI 53706 USA Abstract The recent measurement of the muon anomalous magnetic moment aµ ≡ (g − 2)µ=2 by the Fermilab Muon g − 2 experiment sharpens an earlier discrepancy between theory and the BNL E821 experiment. We examine the predicted ∆aµ ≡ aµ(exp) − aµ(th) in the context of supersymmetry with low electroweak naturalness (restricting to models which give a plausible explanation for the magnitude of the weak scale). A global analy- sis including LHC Higgs mass and sparticle search limits points to interpretation within the normal scalar mass hierarchy (NSMH) SUSY model wherein first/second generation matter scalars are much lighter than third generation scalars. We present a benchmark model for a viable NSMH point which is natural, obeys LHC Higgs and sparticle mass constraints and explains the muon magnetic anomaly. Aside from NSMH models, then we find the (g − 2)µ anomaly cannot be explained within the context of natural SUSY, where a variety of data point to decoupled first/second generation scalars. The situation is worse within the string landscape where first/second generation matter scalars are pulled arXiv:2104.07597v2 [hep-ph] 16 May 2021 to values in the 10 − 50 TeV range. An alternative interpretation for SUSY models with decoupled scalar masses is that perhaps the recent lattice evaluation of the hadronic vac- uum polarization could be confirmed which leads to a Standard Model theory-experiment agreement in which case there is no anomaly.
    [Show full text]
  • Bright Prospects for Tevatron Run II
    INTERNATIONAL JOURNAL OF HIGH-ENERGY PHYSICS CERN COURIER VOLUME 43 NUMBER 1 JANUARY/FEBRUARY 2003 Bright prospects for Tevatron Run II JLAB Virginia laboratory delivers terahertz light p6 ^^^J Modular and expandable power supplies WÊ H Communications via TCP/IP içert. n_.___910S.CAEN '^^^*aBOKS^^^^ • ÊÊÊ WÊÊÊSêSê É TÏSjj à OPC Server to ease integration in DCS J Directly interfaced to JCOP Framework p " j^pj ^ ^^^^ Wa9neticFie,dand^ ^^HTJHj^^^^^^^^^^^^^^^^^^^^^^E' ' tfHl far IM Éfefi-*il * CAEN: your largest choice of HV & LV )^ H MULTICHANNEL POWER SUPPLIES CONTENTS Covering current developments in high- energy physics and related fields worldwide CERN Courier (ISSN 0304-288X) is distributed to member state governments, institutes and laboratories affiliated with CERN, and to their personnel. It is published monthly, except for January and August, in English and French editions. The views expressed are CERN not necessarily those of the CERN management. Editors James Gillies and Christine Sutton CERN, 1211 Geneva 23, Switzerland Email [email protected] Fax+41 (22) 782 1906 Web cerncourier.com COURIER Advisory Board R Landua (Chairman), F Close, E Lillest0l, VOLUME 43 NUMBER 1 JANUARY/FEBRUARY 2003 H Hoffmann, C Johnson, K Potter, P Sphicas Laboratory correspondents: Argonne National Laboratory (US): D Ayres Brookhaven, National Laboratory (US): PYamin Cornell University (US): D G Cassel DESY Laboratory (Germany): Ilka Flegel, P Waloschek Fermi National Accelerator Laboratory (US): Judy Jackson GSI Darmstadt (Germany): G Siegert INFN
    [Show full text]
  • Hadron Collider Physics
    KEK-PH Lectures and Workshops Hadron Collider Physics Zhen Liu University of Maryland 08/05/2020 Part I: Basics Part II: Advanced Topics Focus Collider Physics is a vast topic, one of the most systematically explored areas in particle physics, concerning many observational aspects in the microscopic world • Focus on important hadron collider concepts and representative examples • Details can be studied later when encounter References: Focus on basic pictures Barger & Philips, Collider Physics Pros: help build intuition Tao Han, TASI lecture, hep-ph/0508097 Tilman Plehn, TASI lecture, 0910.4182 Pros: easy to understand Maxim Perelstein, TASI lecture, 1002.0274 Cons: devils in the details Particle Data Group (PDG) and lots of good lectures (with details) from CTEQ summer schools Zhen Liu Hadron Collider Physics (lecture) KEK 2020 2 Part I: Basics The Large Hadron Collider Lyndon R Evans DOI:10.1098/rsta.2011.0453 Path to discovery 1995 1969 1974 1969 1979 1969 1800-1900 1977 2012 2000 1975 1983 1983 1937 1962 Electric field to accelerate 1897 1956 charged particles Synchrotron radiation 4 Zhen Liu Hadron Collider Physics (lecture) KEK 2020 4 Zhen Liu Hadron Collider Physics (lecture) KEK 2020 5 Why study (hadron) colliders (now)? • Leading tool in probing microscopic structure of nature • history of discovery • Currently running LHC • Great path forward • Precision QFT including strong dynamics and weakly coupled theories • Application to other physics probes • Set-up the basic knowledge to build other subfield of elementary particle physics Zhen Liu Hadron Collider Physics (lecture) KEK 2020 6 Basics: Experiment & Theory Zhen Liu Hadron Collider Physics (lecture) KEK 2020 7 Basics: How to make measurements? Zhen Liu Hadron Collider Physics (lecture) KEK 2020 8 Part I: Basics Basic Parameters Basics: Smashing Protons & Quick Estimates Proton Size ( ) Proton-Proton cross section ( ) Particle Physicists use the unit “Barn”2 1 = 100 The American idiom "couldn't hit the broad side of a barn" refers to someone whose aim is very bad.
    [Show full text]
  • Tevatron Accelerator Physics and Operation Highlights A
    FERMILAB-CONF-11-129-APC TEVATRON ACCELERATOR PHYSICS AND OPERATION HIGHLIGHTS A. Valishev for the Tevatron group, FNAL, Batavia, IL 60510, U.S.A. Abstract Table 1: Integrated luminosity performance by fiscal year. The performance of the Tevatron collider demonstrated FY07 FY08 FY09 FY10 continuous growth over the course of Run II, with the peak luminosity reaching 4×1032 cm-2 s-1, and the weekly Total integral (fb-1) 1.3 1.8 1.9 2.47 -1 integration rate exceeding 70 pb . This report presents a review of the most important advances that contributed to Until the middle of calendar year 2009, the luminosity this performance improvement, including beam dynamics growth was dominated by improvements of the antiproton modeling, precision optics measurements and stability production rate [2], which remains stable since. control, implementation of collimation during low-beta Performance improvements over the last two years squeeze. Algorithms employed for optimization of the became possible because of implementation of a few luminosity integration are presented and the lessons operational changes, described in the following section. learned from high-luminosity operation are discussed. Studies of novel accelerator physics concepts at the Tevatron are described, such as the collimation techniques using crystal collimator and hollow electron beam, and compensation of beam-beam effects. COLLIDER RUN II PERFORMANCE Tevatron collider Run II with proton-antiproton collisions at the center of mass energy of 1.96 TeV started in March 2001. Since then, 10.5 fb-1 of integrated luminosity has been delivered to CDF and D0 experiments (Fig. 1). All major technical upgrades of the accelerator complex were completed by 2007 [1].
    [Show full text]
  • MIT at the Large Hadron Collider—Illuminating the High-Energy Frontier
    Mit at the large hadron collider—Illuminating the high-energy frontier 40 ) roland | klute mit physics annual 2010 gunther roland and Markus Klute ver the last few decades, teams of physicists and engineers O all over the globe have worked on the components for one of the most complex machines ever built: the Large Hadron Collider (LHC) at the CERN laboratory in Geneva, Switzerland. Collaborations of thousands of scientists have assembled the giant particle detectors used to examine collisions of protons and nuclei at energies never before achieved in a labo- ratory. After initial tests proved successful in late 2009, the LHC physics program was launched in March 2010. Now the race is on to fulfill the LHC’s paradoxical mission: to complete the Stan- dard Model of particle physics by detecting its last missing piece, the Higgs boson, and to discover the building blocks of a more complete theory of nature to finally replace the Standard Model. The MIT team working on the Compact Muon Solenoid (CMS) experiment at the LHC stands at the forefront of this new era of particle and nuclear physics. The High Energy Frontier Our current understanding of the fundamental interactions of nature is encap- sulated in the Standard Model of particle physics. In this theory, the multitude of subatomic particles is explained in terms of just two kinds of basic building blocks: quarks, which form protons and neutrons, and leptons, including the electron and its heavier cousins. From the three basic interactions described by the Standard Model—the strong, electroweak and gravitational forces—arise much of our understanding of the world around us, from the formation of matter in the early universe, to the energy production in the Sun, and the stability of atoms and mit physics annual 2010 roland | klute ( 41 figure 1 A photograph of the interior, central molecules.
    [Show full text]
  • 01Ii Beam Line
    STA N FO RD LIN EA R A C C ELERA TO R C EN TER Fall 2001, Vol. 31, No. 3 CONTENTS A PERIODICAL OF PARTICLE PHYSICS FALL 2001 VOL. 31, NUMBER 3 Guest Editor MICHAEL RIORDAN Editors RENE DONALDSON, BILL KIRK Contributing Editors GORDON FRASER JUDY JACKSON, AKIHIRO MAKI MICHAEL RIORDAN, PEDRO WALOSCHEK Editorial Advisory Board PATRICIA BURCHAT, DAVID BURKE LANCE DIXON, EDWARD HARTOUNI ABRAHAM SEIDEN, GEORGE SMOOT HERMAN WINICK Illustrations TERRY ANDERSON Distribution CRYSTAL TILGHMAN The Beam Line is published quarterly by the Stanford Linear Accelerator Center, Box 4349, Stanford, CA 94309. Telephone: (650) 926-2585. EMAIL: [email protected] FAX: (650) 926-4500 Issues of the Beam Line are accessible electroni- cally on the World Wide Web at http://www.slac. stanford.edu/pubs/beamline. SLAC is operated by Stanford University under contract with the U.S. Department of Energy. The opinions of the authors do not necessarily reflect the policies of the Stanford Linear Accelerator Center. Cover: The Sudbury Neutrino Observatory detects neutrinos from the sun. This interior view from beneath the detector shows the acrylic vessel containing 1000 tons of heavy water, surrounded by photomultiplier tubes. (Courtesy SNO Collaboration) Printed on recycled paper 2 FOREWORD 32 THE ENIGMATIC WORLD David O. Caldwell OF NEUTRINOS Trying to discern the patterns of neutrino masses and mixing. FEATURES Boris Kayser 42 THE K2K NEUTRINO 4 PAULI’S GHOST EXPERIMENT A seventy-year saga of the conception The world’s first long-baseline and discovery of neutrinos. neutrino experiment is beginning Michael Riordan to produce results. Koichiro Nishikawa & Jeffrey Wilkes 15 MINING SUNSHINE The first results from the Sudbury 50 WHATEVER HAPPENED Neutrino Observatory reveal TO HOT DARK MATTER? the “missing” solar neutrinos.
    [Show full text]
  • Fermi National Accelerator Laboratory 132 Nsec Bunch Spacing in The
    Fermi National Accelerator Laboratory FERMILAR-TM-1920 132 nsec Bunch Spacing in the Tevatron Proton-Antiproton Collider S. D. Holmes et al. Fermi National Accelerator Laboratory P.O. Box 500, Batavia, Illinois 60510 December 1994 0 Operated by Universities Research Association Inc. under Contract No. DE-ACOZ-76CH030W with the United States Department of Energy Disclaimer This report was prepared as an account of work sponsored by an agency of the United States Government. Neither the United States Government nor any agency thereof 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 infn’nge privately owned rights. Reference herein to any specific commercial product, 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 any agency thereof The views and opinions of authors expressed herein do not necessarily state or reflect those of the United States Government or any agency thereof 132 nsec Bunch Spacing in the Tevatron Proton-Antiproton Collider SD. Holmes, J. Holt, J.A. Johnstone, J. Marriner, M. Martens, D. McGinnis Fermi National Accelerator Laboratory December 23, 1994 Abstract Following completion of the Fermilah Main Injector it is expected that the Tevatron proton-antiproton collider will be operating at a luminosity in excess of 5x1031 cm-%ec-1 with 36 proton and antiproton bunches spaced at 396 nsec. At this luminosity, each of the experimental detectors will see approximately 1.3 interactions per crossing.
    [Show full text]
  • HEPAP Looks Into the Future
    Volume 20 Friday, August 29, 1997 Number 17 f INSIDE HEPAP Looks into 2 HEPAP: Voice of the Community the Future 5 Profiles in HEPAP subpanel meets at Fermilab to chart the future of Particle Physics: high-energy physics in the U.S. Dave McGinnis by Donald Sena and Sharon Butler, Office of Public Affairs 6 Barns of Fermilab Charged with recommending how best to In a letter to HEPAP, Martha Krebs, position the U.S. particle physics community Director of the U.S. Department of Energy’s for new facilities beyond CERN’s Large Office of Energy Research, directed the Hadron Collider, a subpanel of the High- subpanel to “recommend a scenario for an Energy Physics Advisory Panel met at Fermilab optimal and balanced U.S. high-energy physics August 14-16 to hear presentations on such program over the next decade,” with “new topics as the research agenda for Fermilab’s facilities to address physics opportunities Run II, the complicated upgrades to the CDF beyond the LHC.” She asked the subpanel and DZero detectors and research on future to consider a future course in light of three accelerators. continued on page 3 Photo by Reidar Hahn Dixon Bogert, deputy project manager for the Main Injector, leads a tour for HEPAP subpanel members and DOE officials. HEPAP: Voice of the Community by Donald Sena and Sharon Butler, Office of Public Affairs The High-Energy Physics Advisory In 1983, for example, a HEPAP According to Fermilab physicist Cathy Panel traces its history to the 1960s, subpanel recommended terminating Newman-Holmes, outgoing member of when
    [Show full text]