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Nuclear Technology
Nuclear Technology Joseph A. Angelo, Jr. GREENWOOD PRESS NUCLEAR TECHNOLOGY Sourcebooks in Modern Technology Space Technology Joseph A. Angelo, Jr. Sourcebooks in Modern Technology Nuclear Technology Joseph A. Angelo, Jr. GREENWOOD PRESS Westport, Connecticut • London Library of Congress Cataloging-in-Publication Data Angelo, Joseph A. Nuclear technology / Joseph A. Angelo, Jr. p. cm.—(Sourcebooks in modern technology) Includes index. ISBN 1–57356–336–6 (alk. paper) 1. Nuclear engineering. I. Title. II. Series. TK9145.A55 2004 621.48—dc22 2004011238 British Library Cataloguing in Publication Data is available. Copyright © 2004 by Joseph A. Angelo, Jr. All rights reserved. No portion of this book may be reproduced, by any process or technique, without the express written consent of the publisher. Library of Congress Catalog Card Number: 2004011238 ISBN: 1–57356–336–6 First published in 2004 Greenwood Press, 88 Post Road West, Westport, CT 06881 An imprint of Greenwood Publishing Group, Inc. www.greenwood.com Printed in the United States of America The paper used in this book complies with the Permanent Paper Standard issued by the National Information Standards Organization (Z39.48–1984). 10987654321 To my wife, Joan—a wonderful companion and soul mate Contents Preface ix Chapter 1. History of Nuclear Technology and Science 1 Chapter 2. Chronology of Nuclear Technology 65 Chapter 3. Profiles of Nuclear Technology Pioneers, Visionaries, and Advocates 95 Chapter 4. How Nuclear Technology Works 155 Chapter 5. Impact 315 Chapter 6. Issues 375 Chapter 7. The Future of Nuclear Technology 443 Chapter 8. Glossary of Terms Used in Nuclear Technology 485 Chapter 9. Associations 539 Chapter 10. -
Richard G. Hewlett and Jack M. Holl. Atoms
ATOMS PEACE WAR Eisenhower and the Atomic Energy Commission Richard G. Hewlett and lack M. Roll With a Foreword by Richard S. Kirkendall and an Essay on Sources by Roger M. Anders University of California Press Berkeley Los Angeles London Published 1989 by the University of California Press Berkeley and Los Angeles, California University of California Press, Ltd. London, England Prepared by the Atomic Energy Commission; work made for hire. Library of Congress Cataloging-in-Publication Data Hewlett, Richard G. Atoms for peace and war, 1953-1961. (California studies in the history of science) Bibliography: p. Includes index. 1. Nuclear energy—United States—History. 2. U.S. Atomic Energy Commission—History. 3. Eisenhower, Dwight D. (Dwight David), 1890-1969. 4. United States—Politics and government-1953-1961. I. Holl, Jack M. II. Title. III. Series. QC792. 7. H48 1989 333.79'24'0973 88-29578 ISBN 0-520-06018-0 (alk. paper) Printed in the United States of America 1 2 3 4 5 6 7 8 9 CONTENTS List of Illustrations vii List of Figures and Tables ix Foreword by Richard S. Kirkendall xi Preface xix Acknowledgements xxvii 1. A Secret Mission 1 2. The Eisenhower Imprint 17 3. The President and the Bomb 34 4. The Oppenheimer Case 73 5. The Political Arena 113 6. Nuclear Weapons: A New Reality 144 7. Nuclear Power for the Marketplace 183 8. Atoms for Peace: Building American Policy 209 9. Pursuit of the Peaceful Atom 238 10. The Seeds of Anxiety 271 11. Safeguards, EURATOM, and the International Agency 305 12. -
2016-2017 Year Book Www
1 2016-2017 YEAR BOOK WWW. C A R N E G I E S C I E N C E . E D U Department of Embryology 3520 San Martin Dr. / Baltimore, MD 21218 410.246.3001 Geophysical Laboratory 5251 Broad Branch Rd., N.W. / Washington, DC 20015-1305 202.478.8900 Department of Global Ecology 260 Panama St. / Stanford, CA 94305-4101 650.462.1047 The Carnegie Observatories 813 Santa Barbara St. / Pasadena, CA 91101-1292 626.577.1122 Las Campanas Observatory Casilla 601 / La Serena, Chile Department of Plant Biology 260 Panama St. / Stanford, CA 94305-4101 650.325.1521 Department of Terrestrial Magnetism 5241 Broad Branch Rd., N.W. / Washington, DC 20015-1305 202.478.8820 Office of Administration 1530 P St., N.W. / Washington, DC 20005-1910 202.387.6400 2 0 1 6 - 2 0 1 7 Y E A R B O O K The President’s Report July 1, 2016 - June 30, 2017 C A R N E G I E I N S T I T U T I O N F O R S C I E N C E Former Presidents Daniel C. Gilman, 1902–1904 Robert S. Woodward, 1904–1920 John C. Merriam, 1921–1938 Vannevar Bush, 1939–1955 Caryl P. Haskins, 1956–1971 Philip H. Abelson, 1971–1978 James D. Ebert, 1978–1987 Edward E. David, Jr. (Acting President, 1987–1988) Maxine F. Singer, 1988–2002 Michael E. Gellert (Acting President, Jan.–April 2003) Richard A. Meserve, 2003–2014 Former Trustees Philip H. Abelson, 1978–2004 Patrick E. -
Ira Sprague Bowen Papers, 1940-1973
http://oac.cdlib.org/findaid/ark:/13030/tf2p300278 No online items Inventory of the Ira Sprague Bowen Papers, 1940-1973 Processed by Ronald S. Brashear; machine-readable finding aid created by Gabriela A. Montoya Manuscripts Department The Huntington Library 1151 Oxford Road San Marino, California 91108 Phone: (626) 405-2203 Fax: (626) 449-5720 Email: [email protected] URL: http://www.huntington.org/huntingtonlibrary.aspx?id=554 © 1998 The Huntington Library. All rights reserved. Observatories of the Carnegie Institution of Washington Collection Inventory of the Ira Sprague 1 Bowen Papers, 1940-1973 Observatories of the Carnegie Institution of Washington Collection Inventory of the Ira Sprague Bowen Paper, 1940-1973 The Huntington Library San Marino, California Contact Information Manuscripts Department The Huntington Library 1151 Oxford Road San Marino, California 91108 Phone: (626) 405-2203 Fax: (626) 449-5720 Email: [email protected] URL: http://www.huntington.org/huntingtonlibrary.aspx?id=554 Processed by: Ronald S. Brashear Encoded by: Gabriela A. Montoya © 1998 The Huntington Library. All rights reserved. Descriptive Summary Title: Ira Sprague Bowen Papers, Date (inclusive): 1940-1973 Creator: Bowen, Ira Sprague Extent: Approximately 29,000 pieces in 88 boxes Repository: The Huntington Library San Marino, California 91108 Language: English. Provenance Placed on permanent deposit in the Huntington Library by the Observatories of the Carnegie Institution of Washington Collection. This was done in 1989 as part of a letter of agreement (dated November 5, 1987) between the Huntington and the Carnegie Observatories. The papers have yet to be officially accessioned. Cataloging of the papers was completed in 1989 prior to their transfer to the Huntington. -
Volume LX I, I 9
CALIFORNIA INSTITUTE Of TECHNOLOGY E N GI N E E Volume LX I, N II1llber 3, I 9 9 8 IN THIS ISSUE • Prosecuting Science Simulating Molecules Observing Anniversaries London Bridge? The Manhattan skyline? No, it's an oil refinery. figuring out how to squeeze more gasoline rrom a barrel or crude is just one project a group or theoretical chemists at Caltech have taken on in a series or academic industrial collaborations. for more on this partner sh ip, see the story on page 20. Photo courtesy or Chevron Corporation. \ California Inst i tute of Technology 2 Random Wa l k 10 Scie ntific Fraud and Misconduct in American Po litica l Cu lture : Reflections on the Baltimore Case - by Dan ie l J. Kevles Excessive zeal on the part of legislators and the media hyped public suspicion of scientists' behavior. 20 " H ave Method , Wi ll T rave l" - by Douglas L. Smi t h Computational chemistry ventures into the Real World as Cal tech theorists tackle industrial problems. 30 Tw o A s tronomical Anniv ers aries : Palomar at 50 Still going strong , the hale and hearty Hale Telescope hits the half century mark. 36 ... and OVRO at 40 Radio astronomers parry, too. On t he Cover: The six IO.4·meter antennas (one 42 Boo ks - The Earth in Tf{rmoil by Kerr y Si eh a n d S i mon LeVay is hidden behind the others here) of the Owe ns 43 Faculty Fil e Valley Radio Observat ory millimeter· wave array can receive signals from up t o Engineering & Science (ISSN 0013-7812) is published Warren G. -
Solving the Discrete Logarithms in Quasi-Polynomial Time
Solving the discrete logarithms in quasi-polynomial time Ivo Kubjas 1 Introduction 1.1 Discrete logarithm The discrete logarithm problem is analogous to the problem of finding logarithm in finite groups. Definition 1 (Discrete logarithm). Discrete logarithm of h to the base g is x such that gx = h: We denote the discrete logarithm as logg(h) = x. The discrete logarithm has similar algebraic properties as for logarithm in reals. 0 0 Namely, logg(hh ) = logg(h) + logg(h ). The discrete logarithm problem is also randomly self-reducible. This means that there are no “difficult” problems. If there would be an element h in the group for which the logarithm is hard to solve, then it is possible to take 1 ≤ x? ≤ q, where q is the order ? of the group. Now, instead of finding the logarithm of h, we find the logarithm of hgx ? and subtract x? from the result. We know that if x? is chosen uniformly, then also gx is ? uniformly distributed in the group and hgx is uniformly distributed. Thus the difficult problem is reduced to solving the discrete logarithm for an average element in the group. Random self-reducibility allows for \easy" problems in the same group. 1.2 The difficulty of computing discrete logarithm Naturally, a question of why computing discrete logarithms is more difficult than comput- ing logarithms arises. For example, there exists a simple algorithm to compute logarithms in reals. Algorithm 1 (Finding logarithm). Let the base be b. We find the logarithm to the base 2 and convert the logarithm to required base in the final step. -
Samuel Goudsmit
NATIONAL ACADEMY OF SCIENCES SAMUEL ABRAHAM GOUDSMIT 1 9 0 2 — 1 9 7 8 A Biographical Memoir by BENJAMIN BEDERSON Any opinions expressed in this memoir are those of the author and do not necessarily reflect the views of the National Academy of Sciences. Biographical Memoir COPYRIGHT 2008 NATIONAL ACADEMY OF SCIENCES WASHINGTON, D.C. Photograph courtesy Brookhaven National Laboratory. SAMUEL ABRAHAM GOUDSMIT July 11, 1902–December 4, 1978 BY BENJAMIN BEDERSON AM GOUDSMIT LED A CAREER that touched many aspects of S20th-century physics and its impact on society. He started his professional life in Holland during the earliest days of quantum mechanics as a student of Paul Ehrenfest. In 1925 together with his fellow graduate student George Uhlenbeck he postulated that in addition to mass and charge the electron possessed a further intrinsic property, internal angular mo- mentum, that is, spin. This inspiration furnished the missing link that explained the existence of multiple spectroscopic lines in atomic spectra, resulting in the final triumph of the then struggling birth of quantum mechanics. In 1927 he and Uhlenbeck together moved to the United States where they continued their physics careers until death. In a rough way Goudsmit’s career can be divided into several separate parts: first in Holland, strictly as a theorist, where he achieved very early success, and then at the University of Michigan, where he worked in the thriving field of preci- sion spectroscopy, concerning himself with the influence of nuclear magnetism on atomic spectra. In 1944 he became the scientific leader of the Alsos Mission, whose aim was to determine the progress Germans had made in the development of nuclear weapons during World War II. -
Cosmic Background Explorer (COBE) and Beyond
From the Big Bang to the Nobel Prize: Cosmic Background Explorer (COBE) and Beyond Goddard Space Flight Center Lecture John Mather Nov. 21, 2006 Astronomical Search For Origins First Galaxies Big Bang Life Galaxies Evolve Planets Stars Looking Back in Time Measuring Distance This technique enables measurement of enormous distances Astronomer's Toolbox #2: Doppler Shift - Light Atoms emit light at discrete wavelengths that can be seen with a spectroscope This “line spectrum” identifies the atom and its velocity Galaxies attract each other, so the expansion should be slowing down -- Right?? To tell, we need to compare the velocity we measure on nearby galaxies to ones at very high redshift. In other words, we need to extend Hubble’s velocity vs distance plot to much greater distances. Nobel Prize Press Release The Royal Swedish Academy of Sciences has decided to award the Nobel Prize in Physics for 2006 jointly to John C. Mather, NASA Goddard Space Flight Center, Greenbelt, MD, USA, and George F. Smoot, University of California, Berkeley, CA, USA "for their discovery of the blackbody form and anisotropy of the cosmic microwave background radiation". The Power of Thought Georges Lemaitre & Albert Einstein George Gamow Robert Herman & Ralph Alpher Rashid Sunyaev Jim Peebles Power of Hardware - CMB Spectrum Paul Richards Mike Werner David Woody Frank Low Herb Gush Rai Weiss Brief COBE History • 1965, CMB announced - Penzias & Wilson; Dicke, Peebles, Roll, & Wilkinson • 1974, NASA AO for Explorers: ~ 150 proposals, including: – JPL anisotropy proposal (Gulkis, Janssen…) – Berkeley anisotropy proposal (Alvarez, Smoot…) – Goddard/MIT/Princeton COBE proposal (Hauser, Mather, Muehlner, Silverberg, Thaddeus, Weiss, Wilkinson) COBE History (2) • 1976, Mission Definition Science Team selected by HQ (Nancy Boggess, Program Scientist); PI’s chosen • ~ 1979, decision to build COBE in-house at GSFC • 1982, approval to construct for flight • 1986, Challenger explosion, start COBE redesign for Delta launch • 1989, Nov. -
History of the Numerical Methods of Pi
History of the Numerical Methods of Pi By Andy Yopp MAT3010 Spring 2003 Appalachian State University This project is composed of a worksheet, a time line, and a reference sheet. This material is intended for an audience consisting of undergraduate college students with a background and interest in the subject of numerical methods. This material is also largely recreational. Although there probably aren't any practical applications for computing pi in an undergraduate curriculum, that is precisely why this material aims to interest the student to pursue their own studies of mathematics and computing. The time line is a compilation of several other time lines of pi. It is explained at the bottom of the time line and further on the worksheet reference page. The worksheet is a take-home assignment. It requires that the student know how to construct a hexagon within and without a circle, use iterative algorithms, and code in C. Therefore, they will need a variety of materials and a significant amount of time. The most interesting part of the project was just how well the numerical methods of pi have evolved. Currently, there are iterative algorithms available that are more precise than a graphing calculator with only a single iteration of the algorithm. This is a far cry from the rough estimate of 3 used by the early Babylonians. It is also a different entity altogether than what the circle-squarers have devised. The history of pi and its numerical methods go hand-in-hand through shameful trickery and glorious achievements. It is through the evolution of these methods which I will try to inspire students to begin their own research. -
Stsci Newsletter: 1991 Volume 008 Issue 03
SPACE 'fEIFSCOPE SOENCE ...______._.INSTITUIE Operated for NASA by AURA November 1991 Vol. 8No. 3 HIGHLIGHTS OF THIS ISSUE: HSTSCIENCE HIGHLIGHTS WF/PC OBSERVATIONS OF THE STELLAR O NEW SCIENCE RESULTS ON M87, CRAB PULSAR CUSP IN M87 O COSTAR PROGRESSING WELL The photograph on the left shows one of a set of images of the central regions of the giant ellipti O ANSWERS TO YOUR QUESTIONS ABOUT HST DATA cal galaxy M87, obtained in June 1991 withHSI's Wide Field and Planetary Camera {WF/PC). 0 CYCLE 2 PEER REVIEW UNDERWAY Analysis of these images has revealed a stellar cusp in the core of M87, consistent with the pres ence of a massive black hole in its nucleus. A combined approach of image deconvolution and modelling has made it possible to investigate the starlight distribution in M87 down to a limiting radius of about 0'.'04 from the nucleus (or about 3 pc from the nucleus if the Virgo cluster is at 16 Mpc). The results show that the central struc ture of M87 can be described by three compo nents: a power-law starlight profile with an r·114 slope which continues unabated into the center, an unresolved central point source, and optical coun terparts of the jet knots identified by VLBI obser vations. In both the V- and /-band Planetary Camera images, the stellar cusp is consistent with the black-hole model proposed for M87 by Young et al. in 1978; in this model, there is a central mas sive object of about 3 x 109 Me. -
Cornell Gets a New Chair
PEOPLE APPOINTMENTS & AWARDS Cornell gets a new chair Two prominent accelerator physicists and Cornell alumni, Helen T Edwards and her husband, Donald A Edwards, have endowed a chair in accelerator physics at Cornell.The chair is named after Boyce D McDaniel, pro fessor emeritus at Cornell. The first holder of the new chair is David L Rubin, professor of physics and director of accelerator physics at Cornell.The donors David Rubin is the first incumbent of the new Boyce McDaniel Chair of Physics at Cornell, asked that the new professorship should be endowed by Helen and Donald Edwards. The chair is named after Boyce D McDaniel. Left awarded to a Cornell faculty member whose to right: Boyce McDaniel, Donald Edwards, David Rubin, Helen Edwards and Maury Tigner, discipline is particle-beam physics and who director of Cornell's Laboratory of Nuclear Studies. would teach both graduate and undergradu ate students in addition to doing research. McDaniel, a previous director of nuclear ingthe commissioning of the Main Ring at Helen Edwards is a 1957 graduate of science at Cornell, was Helen Edwards' thesis Fermilab and providing advice for numerous Cornell, where she also earned her PhD in adviser. Initially a graduate student at Cornell, accelerator projects throughout the US, in 1966. She works at Fermilab and at DESY in he left during the Second World War to join the addition to his notable contributions to the Germany. She played a prominent role in the Manhattan Project and returned to complete accelerator and elementary particle physics construction of Fermilab'sTevatron and has his PhD, joining the faculty in 1946. -
A Thin Diffuse Component of the Galactic Ridge X-Ray Emission and Heating of the Interstellar Medium Contributed by the Radiation of Galactic X-Ray Binaries
A&A 564, A107 (2014) Astronomy DOI: 10.1051/0004-6361/201323332 & c ESO 2014 Astrophysics A thin diffuse component of the Galactic ridge X-ray emission and heating of the interstellar medium contributed by the radiation of Galactic X-ray binaries Margherita Molaro1, Rishi Khatri1, and Rashid A. Sunyaev1,2 1 Max Planck Institut für Astrophysik, Karl-Schwarzschild-Str. 1, 85741 Garching, Germany e-mail: [email protected] 2 Space Research Institute, Russian Academy of Sciences, Profsoyuznaya 84/32, 117997 Moscow, Russia Received 23 December 2013 / Accepted 14 January 2014 ABSTRACT We predict athindiffuse component of the Galactic ridge X-ray emission (GRXE) arising from the scattering of the radiation of bright X-ray binaries (XBs) by the interstellar medium. This scattered component has the same scale height as that of the gaseous disk (∼80 pc) and is therefore thinner than the GRXE of stellar origin (scale height ∼130 pc). The morphology of the scattered component is furthermore expected to trace the clumpy molecular and HI clouds. We calculate this contribution to the GRXE from known Galactic XBs assuming that they are all persistent. The known XBs sample is incomplete, however, because it is flux limited and spans the lifetime of X-ray astronomy (∼50 years), which is very short compared with the characteristic time of 1000−10 000 years that would have contributed to the diffuse emission observed today due to time delays. We therefore also use a simulated sample of sources, to estimate the diffuse emission we should expect in an optimistic case assuming that the X-ray luminosity of our Galaxy is on average similar to that of other galaxies.