CMB-S4 Workshop SLAC Feb 2017

Total Page:16

File Type:pdf, Size:1020Kb

CMB-S4 Workshop SLAC Feb 2017 Cosmology with CMB-S4 Workshop DOE/NSF Project Experience Key Ingredients to Success SLAC National Accelerator Laboratory February 27, 2017 Jim Yeck Outline • Personal Experience • DOE Office of Science (SC) Experience - Projects after the Superconducting Super Collider - DOE SC management perspectives • NSF Large Project Experience - IceCube - Large Hadron Collider Experiments • Satisfying Needs of Project Stakeholders • Next Steps 2 My projects Cost/Circa Infrastructure Project Purpose for CD-3 Funding Role Compact Ignition Tokamak (CIT) at Fusion Energy $330M DOE Acting Project Princeton Plasma Physics Lab Science 1988 DOE Manager Relativistic Heavy Ion Collider $600M DOE Project (RHIC) at Brookhaven Lab (BNL) Nuclear Physics 1991 DOE + NSF + Int Manager US Large Hadron Collider (USLHC) High Energy $530M DOE/NSF Project In-kind delivered to CERN Physics 1998 DOE & NSF Director IceCube Neutrino Observatory at Particle $300M U of Wisconsin -– South Pole Astrophysics 2005 NSF + Int Project Director National Synchrotron Light $900M BNL - Deputy Source II at BNL Photon Source 2008 DOE + Other Project Director Deep Underground Science and Physics, Biology, $750M U of Cal – Associate Engineering Laboratory (DUSEL) and Engineering 2010 NSF + Private Project Director European Spallation Source (ESS) $2,500M ESS ERIC – Director in Sweden Neutron Source 2014 European States General & CEO 3 Key Ingredients to success Facility is a priority of the science community! Strong funding agency commitments and host role Project leaders viewed as enabling success of others Establish realistic goals – “Experience over hope” Credibility through openness and transparency Collective ownership of problems and solutions Populate organization with critical experience Success requires energy and enthusiasm! Project leaders who prioritize on schedule performance and exhibit behaviour that is consistent with a “project culture” are likely to be successful! 4 Projects evaluated against the ingredients #1 #2 #3 #4 #5 #6 #7 & #8 Leaders Priority of Strong Agency Enable the Experience Openness Collective Experience, Science Commitment Success of Over and Trans- Owner- Energy & Project Community & Host Role Others Hope parency ship Enthusiasm Outcome CIT ✖ RHIC ✔ USLHC ✔ IceCube ✔ NSLS II ✔ DUSEL ✖ ? ESS ? 5 DOE Office of Science Project Performance After SSC # of Initial Completed # Cost % Success # Schedule % Success Baseline Final TPC % Cost SITE Projects Success by Cost Success by Schedule TPC ($M) ($M) Increase Argonne National Laboratory 5 5 100% 3 60% $59.5 $59.5 0% Brookhaven National Laboratory 14 14 100% 14 100% $1,223.8 $1,221.3 0% Fermi National Laboratory 11 10 91% 10 91% $1,069.2 $1,095.7 2% Jefferson National Accelerator Facility 2 2 100% 2 100% $84.1 $84.1 0% Lawrence Berkeley National Laboratory 15 14 93% 13 87% $460.2 $462.8 1% Oak Ridge National Laboratory* 13 13 100% 13 100% $1,702.3 $1,772.8 4% Pacific Northwest National Laboratory 3 3 100% 3 100% $15,241.5 $15,241.5 0% Princeton Plasma Physics Laboratory** 4 3 75% 3 75% $235.7 $236.1 0% Sandia National Laboratory (NNSA 1 1 100% 1 100% $75.8 $75.8 0% Operated) Stanford Linear Accelerator Center 9 7 78% 8 89% $692.8 $735.6 6% TOTAL SC PROJECTS* 77 72 94% 70 91% $20,844.9 $20,985.0 1% • Failure of SSC resulted in major changes • Current performance is excellent and SC has high credibility Dan Lehman, PLI Jan 2017 6 Some Unique Features of SC Projects • SC Laboratories are Not-for-Profit M&O contracts • Projects are typically ‘build to cost’ with a goal of maximizing science capability • Project designs consider future upgrades—programs and projects take a long view • Mostly non-nuclear projects • Laboratory’s viability/future is dependent of the success of new advanced facilities or projects to perform state-of-the-art R&D and to attract the best and brightest • Highly technical HQ Program personnel (with extensive laboratory experience) allows evaluation of feasibility and complexity of proposed technical approaches by the labs. Dan Lehman, PLI Jan 2017 7 Successful Projects – Dan Lehman (DOE retired) Primary Factors for Successful Project Completion • Clear Ownership, Accountability, and Responsibilities • Effective Front-End Planning • Appropriate Project Contingencies • Sufficient and Stable Funding • Regular Independent Oversight Dan Lehman, PLI Jan 2017 8 Pat Dehmer, DOE PLI 01/17 9 DOE Office of Science – 2003 priorities vs 2013 status • Some priorities become projects later (and earlier) than originally planned • Project scope is often different than earliest proposals • Not all priorities are realized Pat Dehmer, DOE PLI 01/1710 NSF Large Project Experience • NSF is not a “mission” agency like DOE and NASA • Major Research Equipment and Facilities Construction (MREFC) Program funds NSF large projects - Many successful MREFC projects but some problems - A few early off-ramps, e.g., RSVP, DUSEL • Increased expectations and requirements for projects - Stronger emphasis on front end planning - No cost overrun philosophy embraced • NSF experienced and successful in delivering projects that enable scientific collaborations 11 The IceCube Collaboration includes > 300 researchers from 47 institutes in 12 countries. IceCube is one of the NSF’s large facilities (LIGO, LSST, … 2 dozen others). The Operations and Management of the facility is handled by WIPAC at UW- Madison University of Wisconsin – Madison International Oversight and Finance Group R. Blank, Chancellor National Science M. Mailick, Vice Chancellor for Research and Foundation Science Advisory Committee Graduate Education (VCRGE) B. Barish, Caltech, Chair Software & Computing Advisory Panel WIPAC Education & Outreach Advisory Panel M. Ernst, Brookhaven, Chair Wisconsin IceCube Particle IceCube Neutrino Observatory Collaboration Board Astrophysics Center (WIPAC) Spokesperson & Executive Committee Chair, K. Hanson, Executive Director F. Halzen, Principal Investigator O. Botner (Uppsala) K. Gislason, HR, Busnss&Admin K. Hanson, Director of Operations Deputy Spokesperson, T. DeYoung (MSU) S. Bravo Gallart / M. Madsen, A. Karle, Associate Director for Science & Instrumentation Publication Com. Chair, D. Grant (Alberta) Speakers Com. Chair, E. Resconi (Munich) Communications J. Madsen, Associate Director for Education & Outreach N. Irland, Business IT Support Beyond Deep Core Upgrades Coordinators, D. Grant (Alberta) & D. Cowen (Penn State) Maintenance & Operations Coordination Committee Chair, P. Desiati Resource Coordinator, C. Vakhnina Research & Physics Software Coordination, A. Olivas Analysis Detector M&O – J. Kelley, UW Manager South Pole Logistics/R&D Support – J. Haugen (UW) Analysis Coordinator – Run Coordination, M. Kauer (UW) E. Blaufuss (Maryland) DAQ, D. Glowacki (UW) Computing & Data Management – G. Merino,UW Manager Supernova DAQ, V. Baum / B. Eberhardt (Mainz) Operations Coord. & Cybersecurity, S. Barnet (UW) Working Groups: Processing & Filtering, E. Blaufuss (Maryland) South Pole System & Test System, R. Auer (UW) Muons IceTop Operations, S. Tilav (Delaware) Data Transfer Systems, P. Meade (UW) Cascades & Taus IceCube Live, M. Frère (UW) Data Storage Systems, I. Saunders (UW) Cosmic-Ray Calibration, D. Williams (Alabama) / K. Mase (Chiba) Data Management, J. Bellinger (UW) Point Source High Throughput Computing, V. Brik (UW) EHE and Diffuse Neutrinos TFT Coordination – A. Hallgren (Uppsala) Networking and Facilities, P. Wisniewski (UW) Gamma-ray Burst Data Archive at DESY, K. Leffhalm (DESY) Beyond the Standard Model Data Processing Coordination Supernova P. Desiati, UW Manager Data Processing, J. Oertlin (UW) Simulation Production – Low-Energy / Neutrino Osc. Offline Processing Software (2013), C. Kopper (Alberta) & Production Coordinator, J.C. Diaz-Velez (UW) N. Wandkowsky (UW) Simulation Programs, A. Olivas (Maryland) IceTray Framework/Development, D. LaDieu (Maryland) Collaboration Simulation Production Centers: Database Development Systems, G. Kohnen (Mons) Belgium: IIHE-Brussels, UGent-Ghent; Canada: WestGrid(Alberta) Germany: DESY, Aachen, Dortmund, Wuppertal, Mainz, Bochum Sweden: SWEGRID; US: UW (npx3, GLOW, CHTC, GZK), UMD, UDEL, LBNL/NERSC, UCI, PSU, SUBR(LONI) April 11, 2016 The birth of ATLAS March 1992 – Summer 1992 Merging of EAGLE and ASCOT September 1992: Decision on the name 1st round 2nd round ATLAS 31 ATLAS 40 ALICE 12 ALICE 13 ACE 5 ALEX 5 LHD 0 October 1992 ATLAS LoI submitted to the LHCC Official birth of the ATLAS Collaboration ThyssenKrupp, 8-11-2010 ATLAS Project at CERN's LHC 14 Peter Jenni (CERN) The ATLAS organization has been defined in a lean document (less than 10 pages) in 1994, approved by the Collaboration Board (CB) and the RRB (Funding Agencies) Some key elements: - Each Institution has one vote (independent on the the number of people and the resources) in the CB - The CB meets 3-4 a year, and has an elected Chair ATLAS Management 2004-2009 - The CB elects the Spokesperson (SP, the ‘CEO’) of the Collaboration, by ballot, renewable with a 2/3 majority (initially renewable 3-year terms of office, now 2-year and only once renewable) - Based on explicit consultation, the SP proposes the other management positions, to be endorsed by ballot by the CB (CERN Director General has to agree on Technical and Resources Coordinators) - Sub-system Project Leaders (PLs) elected by the Institutes forming a sub-system, the SP has a right to ‘influence constructively’ this process - The SP finally propose the PLs to the CB for endorsement (by ballot) to form the Executive Board (EB)
Recommended publications
  • 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.
    [Show full text]
  • Subnuclear Physics: Past, Present and Future
    Subnuclear Physics: Past, Present and Future International Symposium 30 October - 2 November 2011 – The purpose of the Symposium is to discuss the origin, the status and the future of the new frontier of Physics, the Subnuclear World, whose first two hints were discovered in the middle of the last century: the so-called “Strange Particles” and the “Resonance #++”. It took more than two decades to understand the real meaning of these two great discoveries: the existence of the Subnuclear World with regularities, spontaneously plus directly broken Symmetries, and totally unexpected phenomena including the existence of a new fundamental force of Nature, called Quantum ChromoDynamics. In order to reach this new frontier of our knowledge, new Laboratories were established all over the world, in Europe, in USA and in the former Soviet Union, with thousands of physicists, engineers and specialists in the most advanced technologies, engaged in the implementation of new experiments of ever increasing complexity. At present the most advanced Laboratory in the world is CERN where experiments are being performed with the Large Hadron Collider (LHC), the most powerful collider in the world, which is able to reach the highest energies possible in this satellite of the Sun, called Earth. Understanding the laws governing the Space-time intervals in the range of 10-17 cm and 10-23 sec will allow our form of living matter endowed with Reason to open new horizons in our knowledge. Antonino Zichichi Participants Prof. Werner Arber H.E. Msgr. Marcelo Sánchez Sorondo Prof. Guido Altarelli Prof. Ignatios Antoniadis Prof. Robert Aymar Prof. Rinaldo Baldini Ferroli Prof.
    [Show full text]
  • CURRICULUM VITAE – Paul D. Grannis April 6, 2021 DATE of BIRTH: June 26, 1938 EDUCATION
    CURRICULUM VITAE { Paul D. Grannis July 15, 2021 EDUCATION: B. Eng. Phys., with Distinction, Cornell University (1961) Ph.D. University of California, Berkeley (1965) Thesis: Measurement of the Polarization Parameter in Proton-Proton Scattering from 1.7 to 6.1 BeV Advisor, Owen Chamberlain EMPLOYMENT: Research Professor of Physics, State Univ. of New York at Stony Brook, 2007 { Distinguished Professor Emeritus, State Univ. of New York at Stony Brook, 2007 { Chair, Department of Physics and Astronomy, Stony Brook, 2002 { 2005 Distinguished Professor of Physics, State Univ. of New York at Stony Brook, 1997 { 2006 Professor of Physics, Stony Brook, 1975 { 1997 Associate Professor of Physics, Stony Brook, 1969 { 1975 Assistant Professor of Physics, Stony Brook, 1966 { 1969 Research Associate, Lawrence Radiation Laboratory, 1965 { 1966 1 AWARDS: Danforth Foundation Fellow, 1961 { 1965 Alfred P. Sloan Foundation Fellow, 1969 { 1971 Fellow, American Physical Society Fellow, American Association for the Advancement of Science Exceptional Teaching Award, Stony Brook, 1992 Exceptional Service Award, U.S. Department of Energy, 1997 John S. Guggenheim Fellowship, 2000 { 2001 American Physical Society W.K.H. Panofsky Prize, 2001 Honorary Doctor of Science, Ohio University, 2009 W. V. Houston Memorial Lectureship, Rice University 2012 Foreign member, Russian Academy of Science, 2016 Co-winner with the members of the DØ Collaboration, European Physical Society High Energy Particle Physics Prize, 2019 2 OTHER ACTIVITIES: Visiting Scientist, Rutherford
    [Show full text]
  • CERN Inaugurates LHC Cyrogenics
    FACES AND PLACES SYMPOSIUM CERN inaugurates LHC cyrogenics Inauguration and ribbon-cutting ceremony of LHC cryogenics by CERN officials: from left, Giorgio Passardi, leader of cryogenics for experiments group; Philippe Lebrun, head of the accelerator Members of the CERN cryogenic groups in front of the Globe of technology department; Giorgio Brianti, founder of the LHC Science and Innovation, where the symposium took place. (Globe project; Lyn Evans, LHC project leader and Laurent Tavian, leader conception T Buchi, Charpente Concept and H Dessimoz, Group H.) of the cryogenics for accelerators group. The beginning of June saw the start of a coils operating at 1.9 K. Besides enhancing Tennessee. Although the commissioning new phase at the LHC project, with the the performance of the niobium-titanium work is far from finished, the cyrogenics inauguration of LHC cryogenics. This was superconductor, this temperature regime groups at CERN felt that after 10 years of marked with a symposium in the Globe makes use of the excellent heat-transfer construction it was now a good time to of Science and Innovation attended by properties of helium in its superfluid state. celebrate, organizing the Symposium for the 178 representatives of the research The design for the LHC cryogenics had to Inauguration of LHC Cryogenics that took institutes involved and industrial partners. incorporate both newly ordered and reused place on 31 May-1 June at CERN's Globe of It also coincided with the stable low- refrigeration plant from LEP operating Science and Innovation. After an inaugural temperature operation of the cryogenic plant at 4.5 K – together with a second stage address by CERN’s director-general, for sector 7–8, the first sector to be cooled operating at 1.9 K – in a system that could Robert Aymar, the programme included down (CERN Courier May 2007 p5).
    [Show full text]
  • CERN Courier – Digital Edition Welcome to the Digital Edition of the November 2018 Issue of CERN Courier
    I NTERNATIONAL J OURNAL OF H IGH -E NERGY P HYSICS CERNCOURIER WELCOME V OLUME 5 8 N UMBER 9 N OVEMBER 2 0 1 8 CERN Courier – digital edition Welcome to the digital edition of the November 2018 issue of CERN Courier. Physics through Explaining the strong interaction was one of the great challenges facing theoretical physicists in the 1960s. Though the correct solution, quantum photography chromodynamics, would not turn up until early the next decade, previous attempts had at least two major unintended consequences. One is electroweak theory, elucidated by Steven Weinberg in 1967 when he realised that the massless rho meson of his proposed SU(2)xSU(2) gauge theory was the photon of electromagnetism. Another, unleashed in July 1968 by Gabriele Veneziano, is string theory. Veneziano, a 26-year-old visitor in the CERN theory division at the time, was trying “hopelessly” to copy the successful model of quantum electrodynamics to the strong force when he came across the idea – via a formula called the Euler beta function – that hadrons could be described in terms of strings. Though not immediately appreciated, his 1968 paper marked the beginning of string theory, which, as Veneziano describes 50 years later, continues to beguile physicists. This issue of CERN Courier also explores an equally beguiling idea, quantum computing, in addition to a PET scanner for clinical and fundamental-physics applications, the internationally renowned Beamline for Schools competition, and the growing links between high-power lasers (the subject of the 2018 Nobel Prize in Physics) and particle physics. To sign up to the new-issue alert, please visit: cerncourier.com/cws/sign-up.
    [Show full text]
  • The Discovery of the Higgs Boson at the LHC
    Chapter 6 The Discovery of the Higgs Boson at the LHC Peter Jenni and Tejinder S. Virdee 6.1 Introduction and the Standard Model The standard model of particle physics (SM) is a theory that is based upon principles of great beauty and simplicity. The theory comprises the building blocks of visible matter, the fundamental fermions: quarks and leptons, and the fundamental bosons that mediate three of the four fundamental interactions; photons for electromag- netism, the W and Z bosons for the weak interaction and gluons for the strong interaction (Fig. 6.1). The SM provides a very successful description of the visible universe and has been verified in many experiments to a very high precision. It has an enormous range of applicability and validity. So far no significant deviations have been observed experimentally. The possibility of installing a proton-proton accelerator in the LEP tunnel, after the e+e− programme, was being discussed in the 1980’s. At the time there were many profound open questions in particle physics, and several are still present. In simple terms these are: what is the origin of mass i.e. how do fundamental particles acquire mass, and why do they have the masses that they have? Why is there more matter than anti-matter? What is dark matter? What is the path towards unification of all forces? Do we live in a world with more space-time dimensions than the familiar four? The LHC [1, 2] was conceived to address or shed light on these questions. P. Jenni CERN, Geneva, Switzerland Albert-Ludwigs University Freiburg, Freiburg im Breisgau, Germany T.
    [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]
  • Die Entdeckung Des Higgs-Teilchens Am CERN
    Die Entdeckung des Higgs-Teilchens am CERN Prof. Karl Jakobs Physikalisches Institut Universität Freiburg From the editorial: “The top Breakthrough of the Year – the discovery of the Higgs boson – was an unusually easy choice, representing both a triumph of the human intellect and the culmination of decades of work by many thousands of physicists and engineers.” Nobel-Preis für Physik 2013: François Englert und Peter Higgs “ … for the theoretical discovery of a mechanism that contributes to our understanding of the origin of mass of sub-atomic particles, and which recently was confirmed through the discovery of the predicted fundamental particle, by the ATLAS and CMS experiments at CERN’s Large Hadron Collider.” EPS Prize 2013: The 2013 High Energy and Particle Physics Prize, for an outstanding contribution to High Energy Physics, is awarded to the ATLAS and CMS collaborations, “for the discovery of a Higgs boson, as predicted by the Brout-Englert-Higgs mechanism”, and to Michel Della Negra, Peter Jenni, and Tejinder Virdee, “for their pioneering and outstanding leadership rôles in the making of the ATLAS and CMS experiments”. Physik-Journal Februar 2015: “.. Obwohl in diesen großen Kollaborationen eine große Zahl von Forschern mitarbeitet, ist es möglich, einzelne Forscherpersönlichkeiten herauszuheben, deren Ideen und Arbeit für den Erfolg des Experiments von besonderer Bedeutung waren. Zu diesen gehört neben den Sprechern der Experimente Karl Jakobs.” The Standard Model of Particle Physics γ mW ≈ 80.4 GeV mZ ≈ 91.2 GeV (i) Matter particles: quarks and leptons (spin ½, fermions) (ii) Four fundamental forces: described by quantum field theories (except gravitation) à massless spin-1 gauge bosons (iii) The Higgs field à scalar field, spin-0 Higgs boson The Brout-Englert-Higgs Mechanism F.
    [Show full text]
  • 2014André Lagarrigue Prize
    2014 André Lagarrigue Prize The international jury1 of the André Lagarrigue prize, meeting under the chairmanship of Jacques Martino, director of IN2P3, has awarded the 2014 prize to Michel Della Negra, physicist emeritus of the CERN Physics Department, presently CMS emeritus at Imperial College, London. The award, established in 2005 under the aegis of the French Physical Society, pays tribute to Professor André Lagarrigue, director of the Laboratory of Linear Accelerator (LAL, Orsay) from 1969 to 1975, who had a major role in the discovery of neutral weak interactions with the Gargamelle bubble chamber at CERN, thus establishing the validity of the electroweak theory. The award, co-funded by the CEA, CERN, Ecole Polytechnique, IN2P3-CNRS, LAL and Université Paris-Sud, is awarded every two years. Born leader, with deep understanding of physics, in direct André Lagarrigue’s lineage, Michel Della Negra has shown outstanding qualities as a builder of experimental devices of great complexity. He is one of the major players in two fundamental discoveries: the W and Z bosons, carriers of the weak interaction with the UA1 SppS, and the Higgs boson with CMS at the LHC. Born in 1942, a graduate of the Ecole Polytechnique, Paris, he begins his career at the Laboratory of Nuclear Physics of the College de France. He defends his thesis in 1967 on the study of proton-antiproton annihilations at rest, using bubble chamber photographs. He is recruited by the CNRS in 1968. During a postdoctoral stay at SLAC (1970-1972), he joins the first deep inelastic scattering experiment using a 17 GeV muon beam interacting on the protons of a rapid cycling bubble chamber, and he is given the responsibility of the muon system.
    [Show full text]
  • Team Science and Individual Recognition
    Individual Recognition in Large Collaborations Archana SHARMA CERN CH1211 Geneva Switzerland ALBA Synchrotron Barcelona - July 19-20, 2018 Group Leader Research Post Doc Assistant Staff Student Staff Staff Student Staff Pierre Curie Assistant Petit Marie Curie Hans Geiger and Ernest Rutherford th th 19 and 20 Century A HEP Group in 70s ALBA Synchrotron Barcelona - July 19-20, 2018 2 30-50 physicists from 10-15 Participating Institutions UA1 & UA2 1980’s 5-8 countries. Natural evolution of Individual Recognition Important component of career and job security 3 1990’s 300-550 physicists from 20-30 participating Institutions in 15-20 countries DELPHI L3 ALEPH OPAL 1990’s 300-550 physicists from 20-30 participating Institutions in 15-20 countries. DELPHI L3 Need for Large Collaborations an important component of scientific progress But are we diluting Individual Recognition ? ALEPH OPAL 2000’s LHC Experiments Up to 5500 physicists from 150-200 participating 2010’s Institutions from 40-50 countries. 2000’s LHC Experiments Leadership emanating from previous generation experiments 2010’s Caveats in Individual Recognition? Large collaborations are successful ! • Clear definitions, agreements on roles • Open communication within teams • Recognition and respect • Addressing problems cooperatively as they occur. • Group goals are placed above personal satisfaction and/or recognition. • Absolute willingness to forgiving for mistakes • Challenges? ALBA Synchrotron Barcelona - July 19-20, 2018 • Particularly for young budding 8 careers ? Guido Tonelli SCARF Autonomy – is “the perception of exerting control over one’s environment; a sensation of having choices.” Providing multiple choices is preferable NA1, NA7, CDF, ALEPH CMS Spokesperson Top: CERN NA close to the UA1 target (1977) First silicon and germanium µStrip active targets for the study of charmed particles.
    [Show full text]
  • Historical Milestones for the ATLAS Experiment
    Symposium 25 Years of LHC Experimental Programme CERN, 15th December 2017 Historical Milestones for Peter Jenni, CERN and the ATLAS Experiment Albert-Ludwigs-Universität Freiburg The plan is to comment a bit on: - History of the LHC experiment studies in general - Some early milestones leading to ATLAS as it is now - Some milestones of the ATLAS construction (pictures…) - Costs and funding, growth of the Collaboration - Note: Physics will be covered by Valerio Dao - And in all cases, these are only examples Drawing by Sergio Cittolin After the 1979 LEP White Book (ECFA-LEP WG chaired by A Zichichi) which mentioned the possibility of a far future LHC, and discoveries of the W and Z bosons by UA1 and UA2 in the early 1980s … 1984 For the community it all started with the CERN - ECFA Workshop in Lausanne on the feasibility of a hadron collider in the future LEP tunnel 1986 LAA R&D on new detector technologies started, later followed by the DRDC 1987 La Thuile Workshop Many LHC colleagues were already involved in this WS set up by Carlo Rubbia as part of the Long Range Planning Committee 25y LHC Exp. Prog. 15-12-2017 ATLAS History 3 Peter Jenni (CERN and Freiburg) Arguing after the mid-1980s of being ambitious and design a general purpose detector … 25y LHC Exp. Prog. 15-12-2017 ATLAS History 4 Peter Jenni (CERN and Freiburg) From an early talk about the LHC, must have been around 1986/7 … 25y LHC Exp. Prog. 15-12-2017 ATLAS History 5 Peter Jenni (CERN and Freiburg) 1989 ECFA Study Week in Barcelona for LHC instrumentation (forming of first proto-Collaboration) 1990 Large Hadron Collider Workshop Aachen (CERN - ECFA) 1992 CERN – ECFA meeting ‘Towards the LHC Experimental Programme’ in Evian 25y LHC Exp.
    [Show full text]
  • 'Vague, but Exciting'
    I n t e r n at I o n a l Jo u r n a l o f HI g H -en e r g y PH y s I c s CERN COURIERV o l u m e 49 nu m b e r 4 ma y 2009 ‘Vague, but exciting’ ACCELERATORS COSMIC RAYS COLLABORATIONS FFAGs enter the era of PAMELA finds a ATLAS makes a smooth applications p5 positron excess p12 changeover at the top p31 CCMay09Cover.indd 1 14/4/09 09:44:43 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 for January and August. The views expressed are not necessarily those of the CERN management. Editor Christine Sutton Editorial assistant Carolyn Lee CERN CERN, 1211 Geneva 23, Switzerland E-mail [email protected] Fax +41 (0) 22 785 0247 Web cerncourier.com Advisory board James Gillies, Rolf Landua and Maximilian Metzger COURIERo l u m e u m b e r a y Laboratory correspondents: V 49 N 4 m 2009 Argonne National Laboratory (US) Cosmas Zachos Brookhaven National Laboratory (US) P Yamin Cornell University (US) D G Cassel DESY Laboratory (Germany) Ilka Flegel, Ute Wilhelmsen EMFCSC (Italy) Anna Cavallini Enrico Fermi Centre (Italy) Guido Piragino Fermi National Accelerator Laboratory (US) Judy Jackson Forschungszentrum Jülich (Germany) Markus Buescher GSI Darmstadt (Germany) I Peter IHEP, Beijing (China) Tongzhou Xu IHEP, Serpukhov (Russia) Yu Ryabov INFN (Italy) Romeo Bassoli Jefferson Laboratory (US) Steven Corneliussen JINR Dubna (Russia) B Starchenko KEK National Laboratory (Japan) Youhei Morita Lawrence Berkeley Laboratory (US) Spencer Klein Seeing beam once again p6 Dirac was right about antimatter p15 A new side to Peter Higgs p36 Los Alamos National Laboratory (US) C Hoffmann NIKHEF Laboratory (Netherlands) Paul de Jong Novosibirsk Institute (Russia) S Eidelman News 5 NCSL (US) Geoff Koch Orsay Laboratory (France) Anne-Marie Lutz FFAGs enter the applications era.
    [Show full text]