Identifying the Source of Stolen Nuclear Materials
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Alfred O. C. Nier
CHEMICAL HERITAGE FOUNDATION ALFRED O. C. NIER Transcript of Interviews Conducted by Michael A. Grayson and Thomas Krick at University of Minnesota Minneapolis, Minnesota on 7, 8, 9, and 10 April 1989 (With Subsequent Corrections and Additions) ACKNOWLEDGMENT This oral history is one in a series initiated by the Chemical Heritage Foundation on behalf of the American Society for Mass Spectrometry. The series documents the personal perspectives of individuals related to the advancement of mass spectrometric instrumentation, and records the human dimensions of the growth of mass spectrometry in academic, industrial, and governmental laboratories during the twentieth century. This project is made possible through the generous support of the American Society for Mass Spectrometry Upon Alfred O.C. Nier’s death in 1994, this oral history was designated Free Access. Please note: Users citing this interview for purposes of publication are obliged under the terms of the Chemical Heritage Foundation Oral History Program to credit CHF using the format below: Alfred O.C. Nier, interview by Michael A. Grayson and Thomas Krick at the University of Minnesota, Minneapolis, Minnesota, 7-10 April 1989 (Philadelphia: Chemical Heritage Foundation, Oral History Transcript # 0112). Chemical Heritage Foundation Oral History Program 315 Chestnut Street Philadelphia, Pennsylvania 19106 The Chemical Heritage Foundation (CHF) serves the community of the chemical and molecular sciences, and the wider public, by treasuring the past, educating the present, and inspiring the future. CHF maintains a world-class collection of materials that document the history and heritage of the chemical and molecular sciences, technologies, and industries; encourages research in CHF collections; and carries out a program of outreach and interpretation in order to advance an understanding of the role of the chemical and molecular sciences, technologies, and industries in shaping society. -
Character List
Character List - Bomb Use this chart to help you keep track of the hundreds of names of physicists, freedom fighters, government officials, and others involved in the making of the atomic bomb. Scientists Political/Military Leaders Spies Robert Oppenheimer - Winston Churchill -- Prime Klaus Fuchs - physicist in designed atomic bomb. He was Minister of England Manhattan Project who gave accused of spying. secrets to Russia Franklin D. Roosevelt -- Albert Einstein - convinced President of the United States Harry Gold - spy and Courier U.S. government that they for Russia KGB. Narrator of the needed to research fission. Harry Truman -- President of story the United States Enrico Fermi - created first Ruth Werner - Russian spy chain reaction Joseph Stalin -- dictator of the Tell Hall -- physicist in Soviet Union Igor Korchatov -- Russian Manhattan Project who gave physicist in charge of designing Adolf Hitler -- dictator of secrets to Russia bomb Germany Haakon Chevalier - friend who Werner Reisenberg -- Leslie Groves -- Military approached Oppenheimer about German physicist in charge of leader of the Manhattan Project spying for Russia. He was designing bomb watched by the FBI, but he was not charged. Otto Hahn -- German physicist who discovered fission Other scientists involved in the Manhattan Project: Aage Niels Bohr George Kistiakowsky Joseph W. Kennedy Richard Feynman Arthur C. Wahl Frank Oppenheimer Joseph Rotblat Robert Bacher Arthur H. Compton Hans Bethe Karl T. Compton Robert Serber Charles Critchfield Harold Agnew Kenneth Bainbridge Robert Wilson Charles Thomas Harold Urey Leo James Rainwater Rudolf Pelerls Crawford Greenewalt Harold DeWolf Smyth Leo Szilard Samuel K. Allison Cyril S. Smith Herbert L. Anderson Luis Alvarez Samuel Goudsmit Edward Norris Isidor I. -
Trinity Transcript
THE NATIONAL ACADEMIES Committee on International Security and Arms Control 60th Anniversary of Trinity: First Manmade Nuclear Explosion, July 16, 1945 PUBLIC SYMPOSIUM July 14, 2005 National Academy of Sciences Auditorium 2100 C Street, NW Washington, DC Proceedings By: CASET Associates, Ltd. 10201 Lee Highway, Suite 180 Fairfax, VA 22030 (703) 352-0091 CONTENTS PAGE Introductory Remarks Welcome: Ralph Cicerone, President, The National Academies (NAS) 1 Introduction: Raymond Jeanloz, Chair, Committee on International Security and Arms Control (CISAC) 3 Roundtable Discussion by Trinity Veterans Introduction: Wolfgang Panofsky, Chair 5 Individual Statements by Trinity Veterans: Harold Agnew 10 Hugh Bradner 13 Robert Christy 16 Val Fitch 20 Don Hornig 24 Lawrence Johnston 29 Arnold Kramish 31 Louis Rosen 35 Maurice Shapiro 38 Rubby Sherr 41 Harold Agnew (continued) 43 1 PROCEEDINGS 8:45 AM DR. JEANLOZ: My name is Raymond Jeanloz, and I am the Chair of the Committee on International Security and Arms Control that organized this morning’s symposium, recognizing the 60th anniversary of Trinity, the first manmade nuclear explosion. I will be the moderator for today’s event, and primarily will try to stay out of the way because we have many truly distinguished and notable speakers. In order to allow them the maximum amount of time, I will only give brief introductions and ask that you please turn to the biographical information that has been provided to you. To start with, it is my special honor to introduce Ralph Cicerone, the President of the National Academy of Sciences, who will open our meeting with introductory remarks. He is a distinguished researcher and scientific leader, recently serving as Chancellor of the University of California at Irvine, and his work in the area of climate change and pollution has had an important impact on policy. -
George Gamow and Barbara Gamow Papers
George Gamow and Barbara Gamow Papers A Finding Aid to the Collection in the Library of Congress Manuscript Division, Library of Congress Washington, D.C. 2016 Revised 2016 December Contact information: http://hdl.loc.gov/loc.mss/mss.contact Additional search options available at: http://hdl.loc.gov/loc.mss/eadmss.ms010191 LC Online Catalog record: http://lccn.loc.gov/mm79021899 Prepared by Grover Batts, Carolyn Craig, and Paul Ledvina with the assistance of Thelma Queen Revised by Manuscript Division Staff Collection Summary Title: George Gamow and Barbara Gamow Papers Span Dates: 1915-1975 Bulk Dates: (bulk 1950-1975) ID No.: MSS21899 Creator: Gamow, George, 1904-1968 Creator: Gamow, Barbara, 1905-1976 Extent: 8,000 items ; 31 containers plus 1 oversize ; 13 linear feet Language: Collection material in English Location: Manuscript Division, Library of Congress, Washington, D.C. Summary: George Gamow, physicist, astronomer, and author. Barbara Gamow, editor and translator. Correspondence, drafts of speeches, articles, and books, and other papers relating principally to George Gamow's career as an astronomer, physicist, and popularizer of science and to Barbara Gamow's personal and literary associations. Selected Search Terms The following terms have been used to index the description of this collection in the Library's online catalog. They are grouped by name of person or organization, by subject or location, and by occupation and listed alphabetically therein. People Alpher, Ralph--Correspondence. Bedford, Sybille, 1911-2006--Correspondence. Brakhage, Stan--Correspondence. Brosche, P. (Peter)--Correspondence. Broughton, James, 1913-1999--Correspondence. Cockcroft, John, Sir, 1897-1967--Correspondence. Covici, Pascal, 1885-1964--Correspondence. Critchfield, Charles Louis, 1910- --Correspondence. -
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. -
María Goeppert Mayer: De Gotinga a Premio Nobel De Física
José Manuel Sánchez Ron José Manuel Sánchez Ron María Goeppert Mayer: de Gotinga a Premio María Goeppert Mayer: Nobel de Física de Gotinga a Premio María Goeppert Mayer (1906-1972) fue una de las cuatro José Manuel Sánchez Ron se Nobel de Física mujeres que, hasta la fecha, han obtenido el Premio Nobel licenció en Física en la Universidad de Física: Marie Curie (1903), María Goeppert Mayer Complutense de Madrid y doctoró en la Universidad de Londres. (1963), Donna Strickland (2018) y Andrea Ghez (2020). Desde 2019 es catedrático emérito Insertando su biografía y contribuciones en el contexto de de Historia de la Ciencia en la los mundos científico y nacional en los que vivió (Alemania Universidad Autónoma de Madrid, y Estados Unidos), el catedrático emérito de Historia de la donde antes de obtener esa cátedra en 1994 fue profesor titular Ciencia en la Universidad Autónoma de Madrid y miembro de Física Teórica. Es autor de de la Real Academia Española, José Manuel Sánchez Ron, numerosas e influyentes obras de reconstruye en este libro los avatares de su carrera, que la historia de la ciencia internacional llevó de la Universidad de Gotinga a la de California en San y española. En 2015 recibió el Diego, pasando por Johns Hopkins, Columbia y Chicago. Premio Nacional de Ensayo por El mundo después de la revolución. Dotada especialmente para la física teórica, sin embargo las La física de la segunda mitad del “circunstancias” de su vida no le permitieron desarrollar un siglo xx, el primer Premio Nacional programa de investigación con cierta coherencia y continuidad. -
Science and New Mexico Los Alamos Los Alamos Scientific Laboratory
National Historic Landmark #7c America At Work: Science and Invention STATE: Form 10-300 UNITED STATES DEPARTMENT OF THE INTERIOR (Rev. 6-72) NATIONAL PARK SERVICE New Mexico COUNTY: NATIONAL REGISTER OF HISTORIC PLACES Los Alamos INVENTORY - NOMINATION FORM FOR NPS USE ONLY ENTRY DATE (Type all entries complete applicable sections) COMMON: Los Alamos Scientific Laboratory AND/OR HISTORIC: Los Alamos Scientific Laboratory STREET AND NUMBER: State Route 4 CITY OR TOWN: CONGRESSIONAL DISTRICT: Los Alamos COUNTY: New Mexico 35 Los Alamos 28 CATEGORY ACCESSIBLE OWNERSHIP STATUS (Check One) TO THE PUBLIC 5Q District Q Building Public Acquisition: ftH Occupied Yes: Restricted Q Site Q Structure L~D Private || In Process [I Unoccupied Unrestricted D Object Both [ | Being Considered I | Preservation work in progress No PRESENT USE (Check One or More as Appropriate) I I Agricultural [~| Government D Pork L~| Transportation I | Comments | | Commercial [~l Industrial [X] Private Residence Q Other (Specify) I I Educational C3 Military I I Religious I I Entertainment ffl Museum [ | Scientific OWNER'S NAME: Also County of Los Alamos by- Atomic Energy Commission and Private land transfer from the AEG STREET AND NUMBER: CITY OR TOWN: CODF Los Alamos New Mexico 35 COURTHOUSE, REGISTRY OF DEEDS, ETC: County Clerk STREET AND NUMBER: County Administrative Building CITY OR TOWN: Los Alamos New Mexico 35 TITLE OF SURVEY: National Survey of Historic Sites and Buildings DATE OF SURVEY: 1965 Federal State Q County Local DEPOSITORY FOR SURVEY RECORDS: Historic -
The Grip of Gravity the Quest to Understand the Laws of Motion and Gravitation Gravity Is the Most Enigmatic of All Known Forces of Nature
The Grip of Gravity The Quest to Understand the Laws of Motion and Gravitation Gravity is the most enigmatic of all known forces of nature. It controls everything, from ocean tides to the expansion of the Universe. The search for the laws of motion and gravitation started over two thousand years ago. The reader is taken on an exciting journey through the subsequent centuries, identifying the blind alleys, profound insights and flashes of inspiration that have punctuated this search. Despite the fantastic progress that has been made, the true nature of gravity is still a mystery and the book attempts to show how the current developments in string theory (perhaps the ‘Theory of Everything’) may lead to a new and radical interpretation of gravity. This book describes the fundamental concepts and developments, and the experiments, both performed and planned, to increase our understanding of gravity and the natural phenomena in which gravity is the principal player. prabhakar gondhalekar is an astrophysicist with major research interest in the interstellar medium and active galactic nuclei. He was formerly head of the Space Astronomy Group at the Rutherford Appleton Laboratory. prabhakar gondhalekar The Grip of Gravity The Quest to Understand the Laws of Motion and Gravitation CAMBRIDGE UNIVERSITY PRESS Cambridge, New York, Melbourne, Madrid, Cape Town, Singapore, São Paulo Cambridge University Press The Edinburgh Building, Cambridge CB2 2RU, UK Published in the United States of America by Cambridge University Press, New York www.cambridge.org Information on this title: www.cambridge.org/9780521803168 © Cambridge University Press 2001 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. -
Designing the Bomb
designing the bomb The world’s first man-made atomic explosion take place efficiently and at the right time. A verit- took place only 28 months after the arrival of the able mountain of difficulties stood in the way. first scientific contingent at Los Alamos. Few greater No one knew how much fissionable material had tributes to human ingenuity have ever been written. to be put together to support an explosive chain The theoretical basis for nuclear weapons was reaction, but it was known that the reaction could already understood, in its outlines, when the Lab- not occur if the amount were insufficient. The oratory was established. Many of the engineering burning of conventional explosives is a chain reac- problems were foreseen in a general way, but much tion of a different kind; a tiny quantity of TNT remained to be done. The following summary of burns as readily as a larger amount. Fission chains weapon theory (all of it known in early 1943) will serve to suggest the enormous difficulty of the task cannot occur in the saline way, because the neutrons that lay ahead. on which they depend must remain within the fuel The nucleus of an atom of uranium-235 contains until they encounter fissionable nuclei. If the sur- 92 protons and 143 neutrons. When this nucleus face area of the fuel mass is large compared to the absorbs an additional neutron, it becomes unstable volume (i.e., if the fuel mass is too small or too and usually divides approximately in half. The two much flattened out), then the neutron escape area fragments become nuclei of two lighter elements, is too large compared to the neutron source volume, having a total mass somewhat less than the mass of and too many neutrons will find their way out with- the original uranium nucleus plus the additional out causing fission. -
Character List
Character List - Bomb Use this chart to help you keep track of the hundreds of names of physicists, freedom fighters, government officials, and others involved in the making of the atomic bomb. Scientists Political/Military Leaders Spies Robert Oppenheimer - Winston Churchill -- Prime Klaus Fuchs - physicist in designed atomic bomb. He was Minister of England Manhattan Project who gave accused of spying. secrets to Russia Franklin D. Roosevelt -- Albert Einstein - convinced President of the United States Harry Gold - spy and Courier U.S. government that they for Russia KGB. Narrator of the needed to research fission. Harry Truman -- President of story the United States Enrico Fermi - created first Ruth Werner - Russian spy chain reaction Joseph Stalin -- dictator of the Tell Hall -- physicist in Soviet Union Igor Korchatov -- Russian Manhattan Project who gave physicist in charge of designing Adolf Hitler -- dictator of secrets to Russia bomb Germany Haakon Chevalier - friend who Werner Reisenberg -- Leslie Groves -- Military approached Oppenheimer about German physicist in charge of leader of the Manhattan Project spying for Russia. He was designing bomb watched by the FBI, but he was not charged. Otto Hahn -- German physicist who discovered fission Other scientists involved in the Manhattan Project: Aage Niels Bohr George Kistiakowsky Joseph W. Kennedy Richard Feynman Arthur C. Wahl Frank Oppenheimer Joseph Rotblat Robert Bacher Arthur H. Compton Hans Bethe Karl T. Compton Robert Serber Charles Critchfield Harold Agnew Kenneth Bainbridge Robert Wilson Charles Thomas Harold Urey Leo James Rainwater Rudolf Pelerls Crawford Greenewalt Harold DeWolf Smyth Leo Szilard Samuel K. Allison Cyril S. Smith Herbert L. Anderson Luis Alvarez Samuel Goudsmit Edward Norris Isidor I. -
Los Alamos Scientific Laboratory
National Historic Landmark #7c America At Work: Science and Invention Form 10-300 UNITED STATES DEPARTMENT OF THE INTERIOR STATE: (Rev. 6-72) NATIONAL PARK SERVICE New Mexico COUNTY: NATIONAL REGISTER OF HISTORIC PLACES Los Alamos INVENTORY - NOMINATION FORM FOR NPS USE ONLY ENTRY DATE (Type all entries complete applicable sections) Los Alamos Scientific Laboratory AND/OR HISTORIC: Los Alamos Scientific Laboratory STREET AND NUMBER: State Route 4 CITY OR TOWN: CONGRESSIONAL DISTRICT: Los Alamos STATE COUN T Y: New Mexico 35 Los Alamos 28 CATEGORY ACCESSIBLE OWNERSH.P STATUS (Check One) TO THE PUBLIC K] District Q Building D Public Public Acquisition: Occupied Yes: ,. , Py Restricted D Site Q Structure D Private Q In Process Unoccupied LJ & Both Q Being Considered i in . [~1 Unrestricted D Object r j Preservation work V PA) MO in progress l— ' PRESENT USE (Check One or More as Appropriate) 1 1 Agricultural Q Government | | Park O Transportation CD Comments O Commercial O Industrie! [X| Private Residence D Other (Specify) PI Educational CD Mi itary | | Religious I | Entertainment El Museum Q] Scientific OWNER'S NAME: Also County of Los Alamos by Atomic Energy Commission and Private land transfer from the AEG STREET AND NUMBER: CITY OR TOWN: CODF Los Alamos New Mexico 35 COURTHOUSE, REGISTRY OF DEEDS, ETC: County Clerk STREET AND NUMBER: County Administrative Building CITY OR TOWN: CODE Los Alamos New Mexico 35 TITLE OF SURVEY: National Survey of Historic Sites and Buildings DATE OF SURVEY: 1965 f£] Federal State Q County Q Local DEPOSITORY -
Nucleosynthesis and Energy Production in Stars: Bethe's Crowning Achievement
GENERAL I ARTICLE Nucleosynthesis and Energy Production in Stars: Bethe's Crowning Achievement Indranil Mazumdar On the 6th of March this year, the seemingly immortal Prof. Hans Bethe passed away, at the ripe age of ninety eight. His mighty mathemat ical prowess, coupled with his amazing virtuos ity in applying the tools of theoretical physics, helped him make original contributions to an as tonishingly large number of topics in theoreti cal and applied physics. In this age of hyper specialization and super computers, Bethe steer Indranil Mazumdar is reader in nuclear physics ed his path through the myriad problems at the at the Tata Institute of frontiers of physics and kept on calculating num Fundamental Research. bers on his trusted slide rule. In this article we His primary research will discuss one of his great contributions that activities are in nuclear fetched him utmost satisfaction, in addition to structure studies, especially experimental the Nobel Prize. studies of the decay of giant dipole resonances Introduction from hot rotating nuclei The lllooniess night sky, studded with twinkling stars and related instrumenta- tion. His theoretical has captivated and inspired the human mind from the activities involve beginning of civilization. The quest to understand stars investigations of light has come a long way from the time of early philosophers neutron rich drip line halo and star watchers. Today we understand that the study nuclei using nuclear three of the structure and evolution of the stars is essential to body techniques. He loves cricket, poetry, clouds, answer a large number of questions about the universe, rivers and rain.