DOCSLIB.ORG

Wiktor Peryt 1944–2013 William (Bill) J Willis 1932–2012

Total Page：16

File Type：pdf, Size：1020Kb

Download full-text PDF Read full-text
Wiktor Peryt 1944–2013 William (Bill) J Willis 1932–2012 Document1 8/8/06 10:44 Page 1 CERN Courier May 2013 Faces & Places A WARDS Engineering prize honours internet and Web pioneers Five engineers whose work, beginning in the 1970s, led to the internet and the World Wide Web have together won the inaugural Queen Elizabeth Prize for Engineering. Robert Kahn, Vinton Cerf, Louis Pouzin, Tim Berners-Lee and Marc Andreessen were announced on 18 March as the winners at the Royal Academy of Engineering in London. Kahn, Cerf and Pouzin receive the award for their contributions to the protocols that make up the fundamental architecture of the internet. French computer scientist Pouzin invented the datagram and designed an early packet communications network known as CYCLADES in the early 1970s. His work was broadly used by Americans Kahn and Cerf in the development of TCP/ IP. Berners-Lee created the World Wide Web at CERN in 1989 and American Marc Andreessen wrote the Mosaic browser that is credited with popularizing the Web. By sharing their work freely and without restriction these pioneers allowed the Tim Berners-Lee is reunited with the historic NeXT computer at CERN during celebrations Visit us at internet and the Web to be adopted rapidly for the 20th anniversary of the web in 2009 (CERN Courier May 2009 p24). He used this around the world and to grow organically computer to develop and run the fi rst Web server, multimedia browser and Web editor. Booth 605 thanks to open and universal standards. Measuring magnetic Additionally, they have served as technical 330 petabytes of data a year – enough to for a ground-breaking innovation in and political stewards of the internet and the transfer every character ever written in every engineering that have benefi ted humanity. New Photomultiplier HV Base field transients? web over the past 30 years as it has grown book ever published 20 times over. It is administered by the Royal Academy of Using photomultipliers is now even easier with a new from its experimental phase to hosting The Queen Elizabeth Prize for Engineering. range of compact, low noise, HV Bases from The Fast Digital Integrator FDI2056 is the world’s 50 billion pages of information today. Today Engineering is a £1 million global The winners are due to come to London in ET Enterprises. fastest and most sensitive voltage integrator. a third of the world’s population uses the engineering prize designed to reward June for the formal presentation of the prize at Incorporating socket, voltage divider and HV - Photo: Scott Maxwell www.agence-arca.com internet and it is estimated to carry around and celebrate the individuals responsible Buckingham Palace by Queen Elizabeth II. supply, they are suitable for use with a wide range of photomultipliers operating in analogue, For the first time it is possible to measure fast, low-level pulse counting or photon counting modes. magnetic field disturbances such as eddy currents in a switched magnet. range of input voltage (5V to 15V) . output voltage adjustable from 100V to 2000V A complete and upgradable . very low power solution for your most exacting . high stability magnetic measurements. Visit our new website for further information. ET Enterprises is now your single source for ‘Electron Tubes’ and ADIT photomultipliers, including many Photonis replacements. Now it’s possible! Designed at the CERN Use our new interactive website to search our complete range of products or follow the contact links to discuss your application. Recipients of the Fundamental Physics project and the CMS and ATLAS Hawking also received a special prize, while ET Enterprises Limited, Riverside Way, Uxbridge, UB8 2YF, UK Prize Foundation’s special prize in experiments from the time that the LHC was quantum-fi eld theorist Alexander Polyakov Phone: +44 (0)1895 200880 fundamental physics, announced in approved by the CERN Council in 1994. received the 2013 Fundamental Physics Fax: +44 (0)1895 270873 [email protected] December (CERN Courier January/ Here Guido Tonelli shares the stage with Prize for his work in fi eld theory and string www.et-enterprises.com February 2013 p36), accepted their awards (left to right): Lyn Evans, Michel Della theory. The event was hosted by the actor ADIT Electron Tubes, 300 Crane Street, at a ceremony in Geneva on 20 March. The Negra, Tejinder Virdee, Peter Jenni, Joe Morgan Freeman, who took the opportunity Sweetwater, Texas 79556, USA Phone: (325) 235 1418 Pantone 286 Pantone 032 prize was shared by leaders of the LHC Incandela and Fabiola Gianotti. Stephen to visit CERN and the LHC tunnel (right). Fax: (325) 235 2872 [email protected] www.electrontubes.com catch the light www.metrolab.com Magnetic precision has a name 41 ANNONCE 2.indd 1 09/03/10 14:33 CERNCOURIER www. V OLUME 5 3 N UMBER 4 M AY 2 0 1 3 CERN Courier May 2013 CERN Courier May 2013 Faces & Places Faces & Places S YMPOSIUM I NAUGURATION 5000 m above sea level. The assembly of Ceremony marks ALMA’s antennas was recently completed, Imperial College celebrates Kibble’s 80th birthday with the last batch of seven out of the fi nal total of 66 antennas currently being tested Tom Kibble, one of the founding fathers a Higgs boson. At the end of the talk, there completion of before entering into service. The telescope of the Standard Model, turned 80 last was a standing ovation for Kibble that lasted has already provided unprecedented views December. To celebrate this milestone and several minutes. ALMA telescope of the cosmos using only a portion of its full Kibble’s extraordinary contributions to In the evening, Nobel laureate Steven array (CERN Courier November 2011 p13). theoretical physics, a one-day symposium Weinberg gave a stunning keynote The ALMA array consists of 54 antennas was held on 13 March at Imperial College, presentation to a capacity audience of 700. In the vast Atacama Desert of the Chilean with 12-m dishes and 12 smaller 7-m dishes, London. With no visual props, he talked eruditely Andes, an offi cial ceremony marked which work together as a single telescope. Kibble has made seminal contributions to on symmetry breaking and its role in the inauguration of the Atacama Large The signals from the individual antennas the understanding of the mass-generating elementary particle physics. He emphasized Millimeter/submillimeter Array (ALMA) are brought together and processed by the mechanism for elementary particles via the role played by the three 1964 papers by (CERN Courier October 2007 p23). More “ALMA correlator” supercomputer. The symmetry breaking. Indeed, his profound Robert Brout, François Englert, Peter Higgs, than 500 people attended the 13 March 66 antennas can be arranged in different papers of 1964 and 1967 provided key Tom Kibble, centre, with from left to right, Gerald Guralnik, Carl Hagen and Kibble event, which signalled the completion of all confi gurations, where the maximum foundations for the Standard Model and Jim Virdee, John Hassard, Tariq Ali, Peter himself. He also emphasized the signifi cant major systems of the giant telescope and the distance between each one can vary from inspired the search for the Higgs boson. He Dornan, John Pendry and Jordan Nash. impact of Kibble’s sole-authored 1967 formal transition from a construction project 150 m to 16 km. has also made signifi cant contributions to the (Images: Meilin Sancho, Imperial College.) paper that, among other things, explains the into an observatory. ALMA is a partnership between scientifi c study of the dynamics of symmetry-breaking mechanism whereby the W and Z boson get A select group, including guest of honour organizations and funding bodies in near phase transitions with diverse mass while the photon remains massless. Sebastián Piñera, the President of Chile, had Europe, North America and East Asia, in applications including to structure formation At the banquet, the UK Minister of the opportunity to visit the telescope, located co-operation with the Republic of Chile. in the universe and vortices in helium-3. Science, David Willetts, praised Kibble’s The symposium profi led these and other contributions to fundamental knowledge aspects of Kibble’s long scientifi c career. The and the important ongoing role of Imperial two themes that resonated throughout the College and the UK more generally. Ed day were Kibble’s extraordinary scientifi c Copeland of the University of Nottingham achievements coupled with his humility. and Kibble’s most prolifi c collaborator, The tenor of the meeting was set in the profi led Kibble’s scientifi c leadership, morning by Neil Turok, director of the vision and generosity. Robert Kibble Perimeter Institute for Theoretical Physics, recollected that while his father was doing who described Kibble as “our guru and Weinberg gave the keynote presentation. his amazing work, family life continued as example”. He discussed Kibble’s pioneering normal – although holiday destinations did work on how topological defects might to be seen in the universe, although many strangely seem to coincide with venues for have formed in the early universe during physicists remain hopeful. physics conferences. Frank Close of Oxford symmetry-breaking phase transitions as the The afternoon’s events were concluded University concluded the banquet speeches universe expanded and cooled. Wojciech by Jim Virdee of Imperial College and the by summarizing the signifi cance of Kibble’s Zurek of Los Alamos National Laboratory CMS experiment, who summarized the contributions to the Standard Model, again Guests at the inauguration included the president of Chile, Sebastián Piñera, seen here continued with this theme, surveying epic quest of fi nding the Higgs boson at highlighting how his 1967 paper inspired (second from left) on an ALMA transporter with representatives from the European analogous processes within the context of the LHC.
Load more

Recommended publications
  • 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]
  • CONTENTS Group Membership, January 2002 2
    CONTENTS Group Membership, January 2002 2 APPENDIX 1: Report on Activities 2000-2002 & Proposed Programme 2002-2006 4 1OPAL 4 2H1 7 3 ATLAS 11 4 BABAR 19 5DØ 24 6 e-Science 29 7 Geant4 32 8 Blue Sky and applied R&D 33 9 Computing 36 10 Activities in Support of Public Understanding of Science 38 11 Collaborations and contacts with Industry 41 12 Other Research Related Activities by Group Members 41 13 Staff Management and Implementation of Concordat 41 APPENDIX 2: Request for Funds 1. Support staff 43 2. Travel 55 3. Consumables 56 4. Equipment 58 APPENDIX 3: Publications 61 1 Group Membership, May 2002 Academic Staff Dr John Allison Senior Lecturer Professor Roger Barlow Professor Dr Ian Duerdoth Senior Lecturer Dr Mike Ibbotson Reader Dr George Lafferty Reader Dr Fred Loebinger Senior Lecturer Professor Robin Marshall Professor, Group Leader Dr Terry Wyatt Reader Dr A N Other (from Sept 2002) Lecturer Fellows Dr Brian Cox PPARC Advanced Fellow Dr Graham Wilson (leave of absence for 2 yrs) PPARC Advanced Fellow James Weatherall PPARC Fellow PPARC funded Research Associates∗ Dr Nick Malden Dr Joleen Pater Dr Michiel Sanders Dr Ben Waugh Dr Jenny Williams PPARC funded Responsive Research Associate Dr Liang Han PPARC funded e-Science Research Associates Steve Dallison core e-Science Sergey Dolgobrodov core e-Science Gareth Fairey EU/PPARC DataGrid Alessandra Forti GridPP Andrew McNab EU/PPARC DataGrid PPARC funded Support Staff∗ Phil Dunn (replacement) Technician Andrew Elvin Technician Dr Joe Foster Physicist Programmer Julian Freestone
    [Show full text]
  • Fabiola Gianotti
    Fabiola Gianotti Date of Birth 29 October 1960 Place Rome, Italy Nomination 18 August 2020 Field Physics Title Director-General of the European Laboratory for Particle Physics, CERN, Geneva Most important awards, prizes and academies Honorary Professor, University of Edinburgh; Corresponding or foreign associate member of the Italian Academy of Sciences (Lincei), the National Academy of Sciences of the United States, the French Academy of Sciences, the Royal Society London, the Royal Academy of Sciences and Arts of Barcelona, the Royal Irish Academy and the Russian Academy of Sciences. Honorary doctoral degrees from: University of Uppsala (2012); Ecole Polytechnique Federale de Lausanne (2013); McGill University, Montreal (2014); University of Oslo (2014); University of Edinburgh (2015); University of Roma Tor Vergata (2017); University of Chicago (2018); University Federico II, Naples (2018); Université de Paris Sud, Orsay (2018); Université Savoie Mont Blanc, Annecy (2018); Weizmann Institute, Israel (2018); Imperial College, London (2019). National honours: Cavaliere di Gran Croce dell'Ordine al Merito della Repubblica, awarded by the Italian President Giorgio Napolitano (2014). Special Breakthrough Prize in Fundamental Physics (shared, 2013); Enrico Fermi Prize of the Italian Physical Society (shared, 2013); Medal of Honour of the Niels Bohr Institute, Copenhagen (2013); Wilhelm Exner Medal, Vienna (2017); Tate Medal of the American Institute of Physics for International Leadership (2019). Summary of scientific research Fabiola Gianotti is a particle physicist working at high-energy accelerators. In her scientific career, she has made significant contributions to several experiments at CERN, including UA2 at the proton-antiproton collider (SpbarpS), ALEPH at the Large Electron-Positron collider (LEP) and ATLAS at the Large Hadron Collider (LHC).
    [Show full text]
  • Particle Physics – It Matters a Forward Look at UK Research Into the Building Blocks of the Universe and Its Impact on Society
    Particle physics – it matters A forward look at UK research into the building blocks of the Universe and its impact on society In partnership with CONTENTS 3 Foreword 4 Advancing human progress through basic knowledge 5 Why does it matter? 6 New frontiers in basic science 6 The experiments 8 How particle physics benefi ts society 8 Particle physics and healthcare 10 Communications 10 Manufacturing and business 11 Global challenges 12 Helping industry 13 Underpinning the knowledge-based economy 14 Particle physics in the UK 15 Further information 2 Foreword Particle physics – it matters Foreword This report summarises the science questions confronting particle-physics research in the next 20 years, what advances in technology are being pursued and the cross-disciplinary benefi ts to be accrued. It is predominantly an interest in curiosity-driven science, of which particle physics is a major part, that often attracts students to study physics and which drives the technological innovation; neither can proceed in isolation. WHAT IS PARTICLE PHYSICS? Particle physics seeks to understand the evolution of the Universe in the fi rst fraction of a second after its birth in the Big Bang in terms of a small number of fundamental particles and forces. The processes involved ultimately resulted in the creation of atoms and the complex molecules that led to our existence. The intellectual curiosity embodied in particle physics is also at the foundation of philosophy, art and other scientifi c disciplines which, together, have shaped the modern world. Without such innate curiosity, the modern world would not exist. The study of particle physics challenges our preconceptions, inspires and seeks to move human knowledge forward at a basic level – wherever that may lead.
    [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]
  • Calorimetry for Particle Physics
    REVIEWS OF MODERN PHYSICS, VOLUME 75, OCTOBER 2003 Calorimetry for particle physics Christian W. Fabjan and Fabiola Gianotti CERN, 1211 Geneva 23, Switzerland (Published 15 October 2003) Calorimetry has become a well-understood, powerful, and versatile measurement method. Besides perfecting this technique to match increasingly demanding operation at high-energy particle accelerators, physicists are developing low-temperature calorimeters to extend detection down to ever lower energies, and atmospheric and deep-sea calorimeters to scrutinize the universe up to the highest energies. The authors summarize the state of the art, with emphasis on the physics of the detectors and innovative technologies. CONTENTS VI. Citius, Altius, Fortius 1280 A. Introduction 1280 B. Atmospheric calorimeters 1280 I. Introduction 1243 1. Setting the energy scale 1283 II. Electromagnetic Calorimetry 1244 2. Energy resolution 1283 A. Physics of the electromagnetic cascade 1244 C. Deep-water calorimeters 1283 B. Energy resolution of electromagnetic VII. Conclusions 1284 calorimeters 1246 Acknowledgments 1284 1. Stochastic term 1247 References 1284 2. Noise term 1247 3. Constant term 1247 4. Additional contributions 1248 C. Main techniques and examples of facilities 1249 I. INTRODUCTION 1. Homogeneous calorimeters 1249 a. Semiconductor calorimeters 1249 Calorimetry is an ubiquitous detection principle in b. Cherenkov calorimeters 1250 particle physics. Originally invented for the study of c. Scintillation calorimeters 1251 cosmic-ray phenomena, this method was developed and d. Noble-liquid calorimeters 1254 perfected for accelerator-based particle physics experi- 2. Sampling calorimeters 1256 mentation primarily in order to measure the energy of a. Scintillation sampling calorimeters 1257 electrons, photons, and hadrons. Calorimeters are b. Gas sampling calorimeters 1257 blocks of instrumented material in which particles to be c.
    [Show full text]
  • ANTIMATTER a Review of Its Role in the Universe and Its Applications
    A review of its role in the ANTIMATTER universe and its applications THE DISCOVERY OF NATURE’S SYMMETRIES ntimatter plays an intrinsic role in our Aunderstanding of the subatomic world THE UNIVERSE THROUGH THE LOOKING-GLASS C.D. Anderson, Anderson, Emilio VisualSegrè Archives C.D. The beginning of the 20th century or vice versa, it absorbed or emitted saw a cascade of brilliant insights into quanta of electromagnetic radiation the nature of matter and energy. The of definite energy, giving rise to a first was Max Planck’s realisation that characteristic spectrum of bright or energy (in the form of electromagnetic dark lines at specific wavelengths. radiation i.e. light) had discrete values The Austrian physicist, Erwin – it was quantised. The second was Schrödinger laid down a more precise that energy and mass were equivalent, mathematical formulation of this as described by Einstein’s special behaviour based on wave theory and theory of relativity and his iconic probability – quantum mechanics. The first image of a positron track found in cosmic rays equation, E = mc2, where c is the The Schrödinger wave equation could speed of light in a vacuum; the theory predict the spectrum of the simplest or positron; when an electron also predicted that objects behave atom, hydrogen, which consists of met a positron, they would annihilate somewhat differently when moving a single electron orbiting a positive according to Einstein’s equation, proton. However, the spectrum generating two gamma rays in the featured additional lines that were not process. The concept of antimatter explained. In 1928, the British physicist was born.
    [Show full text]
  • Department of Physics Review
    The Blackett Laboratory Department of Physics Review Faculty of Natural Sciences 2008/09 Contents Preface from the Head of Department 2 Undergraduate Teaching 54 Academic Staff group photograph 9 Postgraduate Studies 59 General Departmental Information 10 PhD degrees awarded (by research group) 61 Research Groups 11 Research Grants Grants obtained by research group 64 Astrophysics 12 Technical Development, Intellectual Property 69 and Commercial Interactions (by research group) Condensed Matter Theory 17 Academic Staff 72 Experimental Solid State 20 Administrative and Support Staff 76 High Energy Physics 25 Optics - Laser Consortium 30 Optics - Photonics 33 Optics - Quantum Optics and Laser Science 41 Plasma Physics 38 Space and Atmospheric Physics 45 Theoretical Physics 49 Front cover: Laser probing images of jet propagating in ambient plasma and a density map from a 3D simulation of a nested, stainless steel, wire array experiment - see Plamsa Physics group page 38. 1 Preface from the Heads of Department During 2008 much of the headline were invited by, Ian Pearson MP, the within the IOP Juno code of practice grabbing news focused on ‘big science’ Minister of State for Science and (available to download at with serious financial problems at the Innovation, to initiate a broad ranging www.ioppublishing.com/activity/diver Science and Technology Facilities review of physics research under sity/Gender/Juno_code_of_practice/ Council (STFC) (we note that some the chairmanship of Professor Bill page_31619.html). As noted in the 40% of the Department’s research Wakeham (Vice-Chancellor of IOP document, “The code … sets expenditure is STFC derived) and Southampton University). The stated out practical ideas for actions that the start-up of the Large Hadron purpose of the review was to examine departments can take to address the Collider at CERN.
    [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]
  • PARTICLE PHYSICS 2013ª Highlights and Annual Report 2 | Contents Contentsª
    ª PARTICLE PHYSICS Deutsches Elektronen-Synchrotron A Research Centre of the Helmholtz Association PARTICLE PHYSICS 2013 2013ª The Helmholtz Association is a community grand challenges faced by society, science and of 18 scientific-technical and biological- industry. Helmholtz Centres perform top-class Highlights medical research centres. These centres have research in strategic programmes in six core been commissioned with pursuing long-term fields: Energy, Earth and Environment, Health, and Annual Report research goals on behalf of the state and Key Technologies, Structure of Matter, Aero- society. The Association strives to gain insights nautics, Space and Transport. and knowledge so that it can help to preserve and improve the foundations of human life. It does this by identifying and working on the www.helmholtz.de Accelerators | Photon Science | Particle Physics Deutsches Elektronen-Synchrotron A Research Centre of the Helmholtz Association Imprint Publishing and contact Editing Deutsches Elektronen-Synchrotron DESY Ilka Flegel, Manfred Fleischer, Michael Medinnis, A Research Centre of the Helmholtz Association Thomas Schörner-Sadenius Hamburg location: Layout Notkestr. 85, 22607 Hamburg, Germany Diana Schröder Tel.: +49 40 8998-0, Fax: +49 40 8998-3282 Production [email protected] Monika Illenseer Zeuthen location: Printing Platanenallee 6, 15738 Zeuthen, Germany Druckerei Heigener Europrint, Hamburg Tel.: +49 33762 7-70, Fax: +49 33762 7-7413 [email protected] Editorial deadline 28 February 2014 www.desy.de ISBN 978-3-935702-87-4 Editorial note doi: 10.3204/DESY_AR_ET2013 The authors of the individual scientific contributions published in this report are fully responsible for the contents. Cover A possible design of CTA, the Cherenkov Telescope Array.
    [Show full text]
  • Language and Materiality Ethnographic and Theoretical Explorations
    Language and Materiality Ethnographic and Theoretical Explorations Edited by Jillian R. Cavanaugh CUNY, New York Shalini Shankar Northwestern University University Printing House, Cambridge CB2 8BS, United Kingdom One Liberty Plaza, 20th Floor, New York, NY 10006, USA 477 Williamstown Road, Port Melbourne, VIC 3207, Australia 4843/24, 2nd Floor, Ansari Road, Daryaganj, Delhi - 110002, India 79 Anson Road, #06-04/06, Singapore 079906 Cambridge University Press is part of the University of Cambridge. It furthers the University’s mission by disseminating knowledge in the pursuit of education, learning, and research at the highest international levels of excellence. www.cambridge.org Information on this title: www.cambridge.org/9781107180949 DOI: 10.1017/9781316848418 C Cambridge University Press 2017 This publication is in copyright. Subject to statutory exception and to the provisions of relevant collective licensing agreements, no reproduction of any part may take place without the written permission of Cambridge University Press. First published 2017 Printed in <country> by <printer> A catalogue record for this publication is available from the British Library. Library of Congress Cataloging-in-Publication Data ISBN 978-1-107-18094-9 Hardback Cambridge University Press has no responsibility for the persistence or accuracy of URLs for external or third-party internet websites referred to in this publication and does not guarantee that any content on such websites is, or will remain, accurate or appropriate. 4 Fontroversy! Or, How to Care about the Shape of Language Keith M. Murphy Introduction On July 4, 2012, standing in the well of a packed lecture hall on the cam- pus of the European Organization for Nuclear Research (CERN), just outside Geneva, particle physicist Joseph Incandela looked up at the hall’s projection screen and, with only a hint of nerves in his voice, uttered the following pro- nouncement: “If we combine the ZZ and gamma-gamma, this is what we get.
    [Show full text]
  • Neutrino Physics Was Certainly Major.'Xxii
    Neutrino FRANK CLOSE OXFORD UNIVERSITY PRESS OXFORD UNIVERSITY PRESS Great Clarendon Street, Oxford ox2 6dp Oxford University Press is a department of the University of Oxford. It furthers the University's objective of excellence in research, scholarship, and education by publishing worldwide in Oxford New York Auckland Cape Town Dar es Salaam Hong Kong Karachi Kuala Lumpur Madrid Melbourne Mexico City Nairobi New Delhi Shanghai Taipei Toronto With offices in Argentina Austria Brazil Chile Czech Republic France Greece Guatemala Hungary Italy Japan Poland Portugal Singapore South Korea Switzerland Thailand Turkey Ukraine Vietnam Oxford is a registered trade mark of Oxford University Press in the UK and in certain other countries Published in the United States by Oxford University Press Inc., New York ©Frank Close 2010 The moral rights of the author have been asserted Database right Oxford University Press (maker) First published 2010 All rights reserved. No part of this publication may be reproduced, stored in a retrieval system, or transmitted, in any form or by any means, without the prior permission in writing of Oxford University Press, or as expressly permitted by law, or under terms agreed with the appropriate reprographics rights organization. Enquiries concerning reproduction outside the scope of the above should be sent to the Rights Department, Oxford University Press, at the address above You must not circulate this book in any other binding or cover and you must impose the same condition on any acquirer British Library Cataloguing in Publication Data Data available Library of Congress Cataloging in Publication Data Library of Congress Control Number 2010930302 Typeset by SPI Publisher Services, Pondicherry, India Printed in Great Britain on acid-free paper by Clays Ltd, St Ives ISBN 978-0-19-957459-9 Contents Ray Davis Foreword 1.
    [Show full text]