EARLY ACCELERATORS and THEIR BUILDERS* Edwin M
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October 1986
C Fermi National Accelerator Laboratory Monthly Report October 1986 'Ht», i't:.t"tS?t M Fermi/ab Report is published monthly by the Fermi National Accelerator Laboratory Technical Publications Office, P.O. Box 500, MS 107, Batavia, IL, 60510 U.S.A. (312) 840-3278 Editors: R.A. Carrigan, Jr., F.T. Cole, R. Fenner, L. Voyvodic Contributing Editors: D. Beatty, M. Bodnarczuk, R. Craven, D. Green, L. McLerran, S. Pruss, R. Vidal Editorial Assistant: S. Winchester The presentation of material in Fermilab Report is not intended to substitute for nor preclude its publication in a professional journal, and references to articles herein should not be cited in such journals. Contributions, comments, and requests for copies should be addressed to the Fermilab Technical Publications Office. 86/8 Fermi National Accelerator Laboratory 0090.01 011 the cover: M. Stanley Livingston (May 25, 1905 - August 25, 1986) and Ernest 0. Lawrence beside one of the earliest cyclotrons ca. 1933. A remembrance of M.S. Livingston begins on page 21 of this issue. Operated by Universities Research Association, Inc., under contract with the United States Department of Energy Table of Contents Who's Who in the Upcoming Fixed-Target Run? Mark W. Bodnarczuk Saturday Morning Physics: a Report Card 17 Drasko Jovanovic, Barbara Grannis, and Marjorie Bardeen M. Stanley Livingston; 1905 - 1986 21 F.T. Cole Manuscripts, Notes, Lectures, and Colloquia Prepared or Presented from September 21 to October 20, 1986 23 Dates to Remember inside back cover Who's Who in the Upcoming Fixed-Target Physics Run? Mark W. Bodnarczuk Introduction The purpose of this article is to identify the 16 experiments and major test beam programs that will operate during the upcoming fixed-target run scheduled to begin in the middle of March 1987. -
Merle A. Tuve
NATIONAL ACADEMY OF SCIENCES M E R L E A N T O N Y T UVE 1901—1982 A Biographical Memoir by P H ILI P H . AbELSON Any opinions expressed in this memoir are those of the author(s) and do not necessarily reflect the views of the National Academy of Sciences. Biographical Memoir COPYRIGHT 1996 NATIONAL ACADEMIES PRESS WASHINGTON D.C. MERLE ANTONY TUVE June 27, 1901–May 20, 1982 BY PHILIP H. ABELSON ERLE ANTONY TUVE WAS a leading scientist of his times. MHe joined with Gregory Breit in the first use of pulsed radio waves in the measurement of layers in the ionosphere. Together with Lawrence R. Hafstad and Norman P. Heydenburg he made the first and definitive measurements of the proton-proton force at nuclear distances. During World War II he led in the development of the proximity fuze that stopped the buzz bomb attack on London, played a crucial part in the Battle of the Bulge, and enabled naval ships to ward off Japanese aircraft in the western Pacific. Following World War II he served for twenty years as director of the Carnegie Institution of Washington’s Department of Ter- restrial Magnetism, where, in addition to supporting a mul- tifaceted program of research, he personally made impor- tant contributions to experimental seismology, radio astronomy, and optical astronomy. Tuve was a dreamer and an achiever, but he was more than that. He was a man of conscience and ideals. Throughout his life he remained a scientist whose primary motivation was the search for knowledge but a person whose zeal was tempered by a regard for the aspirations of other humans. -
A Brief History and Review of Accelerators
A BRIEF HISTORY AND REVIEW OF ACCELERATORS P.J. Bryant CERN, Geneva, Switzerland ABSTRACT The history of accelerators is traced from three separate roots, through a rapid development to the present day. The well-known Livingston chart is used to illustrate how spectacular this development has been with, on average, an increase of one and a half orders of magnitude in energy per decade, since the early thirties. Several present-day accelerators are reviewed along with plans and hopes for the future. 1 . INTRODUCTION High-energy physics research has always been the driving force behind the development of particle accelerators. They started life in physics research laboratories in glass envelopes sealed with varnish and putty with shining electrodes and frequent discharges, but they have long since outgrown this environment to become large-scale facilities offering services to large communities. Although the particle physics community is still the main group, they have been joined by others of whom the synchrotron light users are the largest and fastest growing. There is also an increasing interest in radiation therapy in the medical world and industry has been a long-time user of ion implantation and many other applications. Consequently accelerators now constitute a field of activity in their own right with professional physicists and engineers dedicated to their study, construction and operation. This paper will describe the early history of accelerators, review the important milestones in their development up to the present day and take a preview of future plans and hopes. 2 . HISTORICAL ROOTS The early history of accelerators can be traced from three separate roots. -
The History and Impact of the CNO Cycles in Nuclear Astrophysics
Phys. Perspect. 20 (2018) 124–158 Ó 2018 Springer International Publishing AG, part of Springer Nature 1422-6944/18/010124-35 https://doi.org/10.1007/s00016-018-0216-0 Physics in Perspective The History and Impact of the CNO Cycles in Nuclear Astrophysics Michael Wiescher* The carbon cycle, or Bethe-Weizsa¨cker cycle, plays an important role in astrophysics as one of the most important energy sources for quiescent and explosive hydrogen burning in stars. This paper presents the intellectual and historical background of the idea of the correlation between stellar energy production and the synthesis of the chemical elements in stars on the example of this cycle. In particular, it addresses the contributions of Carl Friedrich von Weizsa¨cker and Hans Bethe, who provided the first predictions of the carbon cycle. Further, the experimental verification of the predicted process as it developed over the following decades is discussed, as well as the extension of the initial carbon cycle to the carbon- nitrogen-oxygen (CNO) multi-cycles and the hot CNO cycles. This development emerged from the detailed experimental studies of the associated nuclear reactions over more than seven decades. Finally, the impact of the experimental and theoretical results on our present understanding of hydrogen burning in different stellar environments is presented, as well as the impact on our understanding of the chemical evolution of our universe. Key words: Carl Friedrich von Weizsa¨cker; Hans Bethe; Carbon cycle; CNO cycle. Introduction The energy source of the sun and all other stars became a topic of great interests in the physics community in the second half of the nineteenth century. -
Nuclear Navy United States Atomic Energy Commission Historical Advisory Committee
Nuclear Navy United States Atomic Energy Commission Historical Advisory Committee Chairman, Alfred D. Chandler, Jr. Harvard University John T. Conway Consolidated Edison Company Lauchlin M. Currie Carmel, California A. Hunter Dupree Brown University Ernest R. May Harvard University Robert P. Multhauf Smithsonian Institution Nuclear Navy 1946-1962 Richard G. Hewlett and Francis Duncan The University of Chicago Press Chicago and London The University of Chicago Press Chicago 60637 The University of Chicago Press Ltd., London Published 1974 Printed in the United States of America International Standard Book Number: 0-226-33219-5 Library of Congress Catalog Card Number: 74-5726 RICHARD G. HEWLETT is chief historian of the U. S. Atomic Energy Commission. He is coauthor, with Oscar E. Anderson, Jr., of The New World, 1939-1946 and, with Francis Duncan, of Atomic Shield, 1947-1952. FRANCIS DUNCAN is assistant historian of the U.S. Atomic Energy Commission. He is the coauthor of Atomic Shield. [1974] VA Contents Illustrations vii Foreword ix Preface xi 1 2 3 4 Control The The The of the Idea Question of Structure Sea and the Leadership of Responsi- 1 Challenge 52 bility 15 88 5 6 7 8 Emerging Prototypes Toward Nuclear Patterns of and a Nuclear Power Technical Submarines Fleet Beyond Management 153 194 the Navy 121 225 9 10 11 12 Propulsion Building Fleet The for the the Nuclear Operation Measure Fleet Fleet and of Accom- 258 297 Maintenance plishment 340 377 Appendix 1: Table of Organization Abbreviations 404 393 Notes 405 Appendix 2: Construction of the Sources 453 Nuclear Navy 399 Index 461 Appendix 3: Financial Data 402 V Illustrations Charts 8. -
A Brief History and Review of Accelerators
A BRIEF HISTORY AND REVIEW OF ACCELERATORS P.J. Bryant CERN, Geneva, Switzerland ABSTRACT The history of accelerators is traced from three separate roots, through a rapid development to the present day. The well-known Livingston chart is used to illustrate how spectacular this development has been with, on average, an increase of one and a half orders of magnitude in energy per decade, since the early thirties. Several present-day accelerators are reviewed along with plans and hopes for the future. 1 . INTRODUCTION High-energy physics research has always been the driving force behind the development of particle accelerators. They started life in physics research laboratories in glass envelopes sealed with varnish and putty with shining electrodes and frequent discharges, but they have long since outgrown this environment to become large-scale facilities offering services to large communities. Although the particle physics community is still the main group, they have been joined by others of whom the synchrotron light users are the largest and fastest growing. There is also an increasing interest in radiation therapy in the medical world and industry has been a long-time user of ion implantation and many other applications. Consequently accelerators now constitute a field of activity in their own right with professional physicists and engineers dedicated to their study, construction and operation. This paper will describe the early history of accelerators, review the important milestones in their development up to the present day and take a preview of future plans and hopes. 2 . HISTORICAL ROOTS The early history of accelerators can be traced from three separate roots. -
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526 BULLETIN AMERICAN METEOROLOGICAL SOCIETY NEWS AND NOTES International Programs in Atmospheric Sciences A proposed global weather service and scientific study— the atmosphere and fluids in motion, and to estimate the incorporating meteorological satellites, unmanned obser- rate at which these advances may lead to progress in vational platforms, and devices not yet on the drawing weather forecasting and related services. Finally, ad- boards—is outlined in a report issued in April to the vances in physics and a better understanding of the world scientific community by the National Academy of atmospheric responses to energy inputs point toward pos- Sciences—National Research Council. sibilities of modification of large-scale weather processes The report calls for an unprecedented collaboration be- to meet human needs." tween scientific institutions and national governments in Looking to the future, the committee's report adds, atmospheric research, meteorological service, atmos- "Perhaps one of the most important achievements to be pheric surveiliance, and meteorological education "to looked for in the near future will come from development raise the effectiveness of the meteorological services on a of communication between observation platforms. Espe- world-wide basis." cially equipped communication satellites may be used to "The aims go further," the report continues, "from monitor signals from high-level balloons, aircraft, rock- prediction to modification or control." ets, etc., to scan the atmosphere for disastrous storms The collaboration would take place through the non- and other important phenomena, and report to ground governmental International Council of Scientific Unions stations. Such extension will result in a functional sys- and the World Meteorological Organization, a United tem zvhich combines the advantages of direct and indi- Nations body. -
Introduction to Accelerators: Evolution of Accelerators and Modern Day Applications
Lecture 1 Introduction to Accelerators: Evolution of Accelerators and Modern Day Applications Sarah Cousineau, Jeff Holmes, Yan Zhang USPAS January, 2011 What are accelerators used for? • Particle accelerators are devices that produce energetic beams of particles which are used for – Understanding the fundamental building blocks of nature and the forces that act upon them (nuclear and particle physics) – Understanding the structure and dynamics of materials and their properties (physics, chemistry, biology, medicine) – Medical treatment of tumors and cancers – Production of medical isotopes – Sterilization – Ion Implantation to modify the surface of materials • There is active, ongoing work to utilize particle accelerators for – Transmutation of nuclear waste – Generating power more safely in sub-critical nuclear reactors Accelerators by the Numbers World wide inventory of accelerators, in total 15,000. The data have been collected by W. Scarf and W. Wiesczycka (See U. Amaldi Europhysics News, June 31, 2000) Category Number Ion implanters and surface modifications 7,000 Accelerators in industry 1,500 Accelerators in non-nuclear research 1,000 Radiotherapy 5,000 Medical isotopes production 200 Hadron therapy 20 Synchrotron radiation sources 70 Nuclear and particle physics research 110 The most well known category of accelerators – particle physics research accelerators – is one of the smallest in number. The technology for other types of accelerators was born from these machines. Nuclear and Particle Physics • Much of what we know about -
Particle Accelerators and Discoveries in Elementary Particle Physics
2280 PARTICLE ACCELERATORS AND DISCOVERIES IN ELEMENTARY PARTICLE PHYSICS Lawrence W. Jones Randall Laboratory of Physics, University of Michigan Ann Arbor, Michigan 48109-1120 Abstract Some discoveries in elementary particle physics are recounted from personal and his- torical perspective with particular reference to their interaction with particle accelerators. The particular examples chosen include the C/J, the T, and the study of nucleon con- stituents with inelastic electron scattering. Precurser experiments are cited together with the better known discoveries. 2281 PARTICLE ACCELERATORS AND DISCOVERIES IN ELEMENTARY PARTICLE PHYSICS Lawrence W. Jones* Randall Laboratory of Physics, University of Michigan Ann Arbor, Michigan 48109-1120 Dr. Month asked me to prepare a talk on high energy physics discoveries and their relationship to particle accelerators. No particular time period was specified~ however, high energy physics as a field is less than forty years old. This historical subject was a challenge for me as there was clearly far too much to cover in a comprehensive manner in just one hour. Therefore, I was forced to pick and choose. I am not an historian of physics, and I have not made a systematic study of the recent history of particle physics. Rather I am a physicist who is now becoming old enough to have "been there" when some of these discoveries were made. I have used as one source for this talk the material contained in a report prepared for a larger document "Physics in the 1980's" edited by Dr. Brinkman. Martin Perl of Stanford has chaired a subpanel on elementary particle physics of that task force, on which I served. -
Nobel Laureates and Twentieth-Century Physics Mauro Dardo Index More Information
Cambridge University Press 0521540089 - Nobel Laureates and Twentieth-Century Physics Mauro Dardo Index More information Index Abrikosov, Alexei A., 474 American Physical Society, 395 Armstrong, Neil, 279 biographical notes on, 466 Amp`ere,Andr´e-Marie,19, 28 Arnold, Harold, 163 Nobel Prize (2003) to, 462 Anderson, Carl David, 58, 183, 184, 187, Arrhenius, Svante, 34, 69–70, 120, superconductivity, 464–465 194, 196, 226, 231–234, 275, 422, 126–139, 302 Academy of Sciences, French, 13, 43, 44, 470 Aston, Francis William, 82, 200 138, 139, 165, 316, 411, 413 biographical notes on, 195–197 mass spectrograph, 121–122 Academy of Sciences, Prussian, 104–105, muon, 195 astronomy, 329, 414 115, 122, 123, 128, 187 Nobel Prize (1936) to, 193 Astrophysical Journal, 351, 415 Academy of Sciences, Russian, 268, 284, positron, 183, 197 astrophysics, 279, 302, 319, 329, 414, 349, 447, 466–467 Anderson, Philip Warren, 328, 344–345, 458, 475 Academy of Sciences, Soviet Union, see 348, 356, 434, 472 asymptotic freedom, 406 Academy of Sciences, Russian biographical notes on, 345–346 AT&T, 6, 163, 278 Accademia dei Lincei, 348 challenge of reductionism by, 347–349 Atkinson, Robert, 303 accelerators, see particle accelerators condensed-matter physics, 346–347 atom, 17, 25, 26–27, 475 AGS (BNL), 272, 286, 313, 337, 363, 398 Nobel Prize (1977) to, 340–341 Bohr’s model of, 91 Alembert Le Rond Jean d’, 14 Anderson localisation, 344–347, 434 nuclear, 77, 80, 81, 90–91 Alferov, Zhores Ivanovich, 447, 474 Anderson model, 346 plum pudding model of, 81 biographical -
Smithsonian at the Poles Contributions to International Polar Year Science
A Selection from Smithsonian at the Poles Contributions to International Polar Year Science Igor Krupnik, Michael A. Lang, and Scott E. Miller Editors A Smithsonian Contribution to Knowledge WASHINGTON, D.C. 2009 This proceedings volume of the Smithsonian at the Poles symposium, sponsored by and convened at the Smithsonian Institution on 3–4 May 2007, is published as part of the International Polar Year 2007–2008, which is sponsored by the International Council for Science (ICSU) and the World Meteorological Organization (WMO). Published by Smithsonian Institution Scholarly Press P.O. Box 37012 MRC 957 Washington, D.C. 20013-7012 www.scholarlypress.si.edu Text and images in this publication may be protected by copyright and other restrictions or owned by individuals and entities other than, and in addition to, the Smithsonian Institution. Fair use of copyrighted material includes the use of protected materials for personal, educational, or noncommercial purposes. Users must cite author and source of content, must not alter or modify content, and must comply with all other terms or restrictions that may be applicable. Cover design: Piper F. Wallis Cover images: (top left) Wave-sculpted iceberg in Svalbard, Norway (Photo by Laurie M. Penland); (top right) Smithsonian Scientifi c Diving Offi cer Michael A. Lang prepares to exit from ice dive (Photo by Adam G. Marsh); (main) Kongsfjorden, Svalbard, Norway (Photo by Laurie M. Penland). Library of Congress Cataloging-in-Publication Data Smithsonian at the poles : contributions to International Polar Year science / Igor Krupnik, Michael A. Lang, and Scott E. Miller, editors. p. cm. ISBN 978-0-9788460-1-5 (pbk. -
M. Stanley Livingston
NATIONAL ACADEMY OF SCIENCES M I L T O N S T A N L E Y L IVIN G STON 1905—1986 A Biographical Memoir by E R N E S T D. COURANT Any opinions expressed in this memoir are those of the author(s) and do not necessarily reflect the views of the National Academy of Sciences. Biographical Memoir COPYRIGHT 1997 NATIONAL ACADEMIES PRESS WASHINGTON D.C. Courtesy of Brookhaven National Laboratory MILTON STANLEY LIVINGSTON May 25, 1905–August 25, 1986 BY ERNEST D. COURANT N JANUARY 9, 1932, in Berkeley, California, a magnetic Oresonance accelerator (cyclotron) built by M. Stanley Livingston accelerated protons to 1.22 MeV (million elec- tron volts), the first time that particles with energies ex- ceeding one million volts had been produced by man. Twenty years later, in May 1952, the Cosmotron at Brookhaven Na- tional Laboratory, whose construction Livingston had initi- ated, became the world’s first billion-volt (GeV) accelera- tor. By the time of his death in 1986 the world record had gone up by three more orders of magnitude to 900 GeV, thanks to an innovation by Livingston and others. Milton Stanley Livingston was born in Broadhead, Wis- consin, on May 25, 1905, the son of Milton McWhorter Livingston and his wife Sarah Jane, née Ten Eyck. His fa- ther was a divinity student who soon became minister of a local church. When Stanley was about five years old the family moved to southern California, where his father be- came a high school teacher and later principal, having found that a minister’s salary was inadequate to support a growing family.