20180801 Crucial Non-Thermal Ignition of HB11
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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. -
Progress Towards Polar-Drive Ignition for the NIF
Home Search Collections Journals About Contact us My IOPscience Progress towards polar-drive ignition for the NIF This content has been downloaded from IOPscience. Please scroll down to see the full text. 2013 Nucl. Fusion 53 113021 (http://iopscience.iop.org/0029-5515/53/11/113021) View the table of contents for this issue, or go to the journal homepage for more Download details: IP Address: 198.125.179.18 This content was downloaded on 06/11/2013 at 22:08 Please note that terms and conditions apply. IOP PUBLISHING and INTERNATIONAL ATOMIC ENERGY AGENCY NUCLEAR FUSION Nucl. Fusion 53 (2013) 113021 (5pp) doi:10.1088/0029-5515/53/11/113021 Progress towards polar-drive ignition for the NIF R.L. McCrory1,a, R. Betti1,a, T.R. Boehly1, D.T. Casey2, T.J.B. Collins1, R.S. Craxton1, J.A. Delettrez1, D.H. Edgell1, R. Epstein1, J.A. Frenje2, D.H. Froula1, M. Gatu-Johnson2, V.Yu. Glebov1, V.N. Goncharov1, D.R. Harding1, M. Hohenberger1, S.X. Hu1, I.V. Igumenshchev1, T.J. Kessler1, J.P. Knauer1, C.K. Li2, J.A. Marozas1, F.J. Marshall1, P.W. McKenty1, D.D. Meyerhofer1,a, D.T. Michel1, J.F. Myatt1, P.M. Nilson1, S.J. Padalino3, R.D. Petrasso2, P.B. Radha1, S.P. Regan1, T.C. Sangster1, F.H. Seguin´ 2, W. Seka1, R.W. Short1, A. Shvydky1, S. Skupsky1, J.M. Soures1, C. Stoeckl1, W. Theobald1, B. Yaakobi1 and J.D. Zuegel1 1 Laboratory for Laser Energetics, University of Rochester, 250 East River Road, Rochester, NY 14623-1299, USA 2 Plasma Science Fusion Center, 173 Albany Street, Massachusetts Institute of Technology, Cambridge MA 02139, USA 3 Department of Physics, State University of New York at Geneseo, 1 College Circle, Geneseo NY 14454, USA E-mail: [email protected] Received 31 December 2012, accepted for publication 4 September 2013 Published 27 September 2013 Online at stacks.iop.org/NF/53/113021 Abstract The University of Rochester’s Laboratory for Laser Energetics (LLE) performs direct-drive inertial confinement fusion (ICF) research. -
Controlled Nuclear Fusion
Controlled Nuclear Fusion HANNAH SILVER, SPENCER LUKE, PETER TING, ADAM BARRETT, TORY TILTON, GABE KARP, TIMOTHY BERWIND Nuclear Fusion Thermonuclear fusion is the process by which nuclei of low atomic weight such as hydrogen combine to form nuclei of higher atomic weight such as helium. two isotopes of hydrogen, deuterium (composed of a hydrogen nucleus containing one neutrons and one proton) and tritium (a hydrogen nucleus containing two neutrons and one proton), provide the most energetically favorable fusion reactants. in the fusion process, some of the mass of the original nuclei is lost and transformed to energy in the form of high-energy particles. energy from fusion reactions is the most basic form of energy in the universe; our sun and all other stars produce energy through thermonuclear fusion reactions. Nuclear Fusion Overview Two nuclei fuse together to form one larger nucleus Fusion occurs in the sun, supernovae explosion, and right after the big bang Occurs in the stars Initially, research failed Nuclear weapon research renewed interest The Science of Nuclear Fusion Fusion in stars is mostly of hydrogen (H1 & H2) Electrically charged hydrogen atoms repel each other. The heat from stars speeds up hydrogen atoms Nuclei move so fast, they push through the repulsive electric force Reaction creates radiant & thermal energy Controlled Fusion uses two main elements Deuterium is found in sea water and can be extracted using sea water Tritium can be made from lithium When the thermal energy output exceeds input, the equation is self-sustaining and called a thermonuclear reaction 1929 1939 1954 1976 1988 1993 2003 Prediction Quantitativ ZETA JET Project Japanese Princeton ITER using e=mc2, e theory Tokomak Generates that energy explaining 10 from fusion is fusion. -
Can 250+ Fusions Per Muon Be Achieved?
CAN 250+ FUSIONS PER MUON BE ACHIEVED? CONF-870448—1 Steven E. Jones DE87 010472 Brigham Young University Dept. of Physics and Astronomy Provo, UT 84602 U.S.A. INTRODUCTION Nuclear fusion of hydrogen isotopes can be induced by negative muons (u) in reactions such as: y- + d + t + o + n -s- u- (1) t J N This reaction is analagous to the nuclear fusion reaction achieved in stars in which hydrogen isotopes (such as deuterium, d, and tritium, t) at very high temperatures first penetrate the Coulomb repulsive barrier and then fuse together to produce an alpha particle (a) and a neutron (n), releasing energy which reaches the earth as light and heat. Life in the universe depends on fusion energy. In the case of reaction (1), the muon in general reappears after inducing fusion so that the reaction can be repeated many (N) times. Thus, the muon may serve as an effective catalyst for nuclear fusion. Muon- catalyzed fusion is unique in that it proceeds rapidly in deuterium-tritium mixtures at relatively cold temperatures, e.g. room temperature. The need for plasma temperatures to initiate fusion is overcome by the presence of the nuon. In analogy to an ordinary hydrogen molecule, the nuon binds together the deuteron and triton in a very small molecule. Since the muonic mass is so large, the dtp molecule is tiny, so small that the deuteron and triton are induced to fuse together in about a picosecond - one millionth of the nuon lifetime. We could speak here of nuonlc confinement, in lieu of the gravitational confinement found in stars, or MASTER DISTRIBUTION OF THIS BBCUMENT IS UNLIMITED magnetic or inertial confinement of hot plasmas favored in earth-bound attempts at imitating stellar fusion. -
Thermonuclear AB-Reactors for Aerospace
1 Article Micro Thermonuclear Reactor after Ct 9 18 06 AIAA-2006-8104 Micro -Thermonuclear AB-Reactors for Aerospace* Alexander Bolonkin C&R, 1310 Avenue R, #F-6, Brooklyn, NY 11229, USA T/F 718-339-4563, [email protected], [email protected], http://Bolonkin.narod.ru Abstract About fifty years ago, scientists conducted R&D of a thermonuclear reactor that promises a true revolution in the energy industry and, especially, in aerospace. Using such a reactor, aircraft could undertake flights of very long distance and for extended periods and that, of course, decreases a significant cost of aerial transportation, allowing the saving of ever-more expensive imported oil-based fuels. (As of mid-2006, the USA’s DoD has a program to make aircraft fuel from domestic natural gas sources.) The temperature and pressure required for any particular fuel to fuse is known as the Lawson criterion L. Lawson criterion relates to plasma production temperature, plasma density and time. The thermonuclear reaction is realised when L > 1014. There are two main methods of nuclear fusion: inertial confinement fusion (ICF) and magnetic confinement fusion (MCF). Existing thermonuclear reactors are very complex, expensive, large, and heavy. They cannot achieve the Lawson criterion. The author offers several innovations that he first suggested publicly early in 1983 for the AB multi- reflex engine, space propulsion, getting energy from plasma, etc. (see: A. Bolonkin, Non-Rocket Space Launch and Flight, Elsevier, London, 2006, Chapters 12, 3A). It is the micro-thermonuclear AB- Reactors. That is new micro-thermonuclear reactor with very small fuel pellet that uses plasma confinement generated by multi-reflection of laser beam or its own magnetic field. -
Inis: Terminology Charts
IAEA-INIS-13A(Rev.0) XA0400071 INIS: TERMINOLOGY CHARTS agree INTERNATIONAL ATOMIC ENERGY AGENCY, VIENNA, AUGUST 1970 INISs TERMINOLOGY CHARTS TABLE OF CONTENTS FOREWORD ... ......... *.* 1 PREFACE 2 INTRODUCTION ... .... *a ... oo 3 LIST OF SUBJECT FIELDS REPRESENTED BY THE CHARTS ........ 5 GENERAL DESCRIPTOR INDEX ................ 9*999.9o.ooo .... 7 FOREWORD This document is one in a series of publications known as the INIS Reference Series. It is to be used in conjunction with the indexing manual 1) and the thesaurus 2) for the preparation of INIS input by national and regional centrea. The thesaurus and terminology charts in their first edition (Rev.0) were produced as the result of an agreement between the International Atomic Energy Agency (IAEA) and the European Atomic Energy Community (Euratom). Except for minor changesq the terminology and the interrela- tionships btween rms are those of the December 1969 edition of the Euratom Thesaurus 3) In all matters of subject indexing and ontrol, the IAEA followed the recommendations of Euratom for these charts. Credit and responsibility for the present version of these charts must go to Euratom. Suggestions for improvement from all interested parties. particularly those that are contributing to or utilizing the INIS magnetic-tape services are welcomed. These should be addressed to: The Thesaurus Speoialist/INIS Section Division of Scientific and Tohnioal Information International Atomic Energy Agency P.O. Box 590 A-1011 Vienna, Austria International Atomic Energy Agency Division of Sientific and Technical Information INIS Section June 1970 1) IAEA-INIS-12 (INIS: Manual for Indexing) 2) IAEA-INIS-13 (INIS: Thesaurus) 3) EURATOM Thesaurusq, Euratom Nuclear Documentation System. -
The Stellarator Program J. L, Johnson, Plasma Physics Laboratory, Princeton University, Princeton, New Jersey
The Stellarator Program J. L, Johnson, Plasma Physics Laboratory, Princeton University, Princeton, New Jersey, U.S.A. (On loan from Westlnghouse Research and Development Center) G. Grieger, Max Planck Institut fur Plasmaphyslk, Garching bel Mun<:hen, West Germany D. J. Lees, U.K.A.E.A. Culham Laboratory, Abingdon, Oxfordshire, England M. S. Rablnovich, P. N. Lebedev Physics Institute, U.S.3.R. Academy of Sciences, Moscow, U.S.S.R. J. L. Shohet, Torsatron-Stellarator Laboratory, University of Wisconsin, Madison, Wisconsin, U.S.A. and X. Uo, Plasma Physics Laboratory Kyoto University, Gokasho, Uj', Japan Abstract The woHlwide development of stellnrator research is reviewed briefly and informally. I OISCLAIWCH _— . vi'Tli^liW r.'r -?- A stellarator is a closed steady-state toroidal device for cer.flning a hot plasma In a magnetic field where the rotational transform Is produced externally, from torsion or colls outside the plasma. This concept was one of the first approaches proposed for obtaining a controlled thsrtnonuclear device. It was suggested and developed at Princeton in the 1950*s. Worldwide efforts were undertaken in the 1960's. The United States stellarator commitment became very small In the 19/0's, but recent progress, especially at Carchlng ;ind Kyoto, loeethar with «ome new insights for attacking hotii theoretics] Issues and engineering concerns have led to a renewed optimism and interest a:; we enter the lQRO's. The stellarator concept was borr In 1951. Legend has it that Lyman Spiczer, Professor of Astronomy at Princeton, read reports of a successful demonstration of controlled thermonuclear fusion by R. -
1 Looking Back at Half a Century of Fusion Research Association Euratom-CEA, Centre De
Looking Back at Half a Century of Fusion Research P. STOTT Association Euratom-CEA, Centre de Cadarache, 13108 Saint Paul lez Durance, France. This article gives a short overview of the origins of nuclear fusion and of its development as a potential source of terrestrial energy. 1 Introduction A hundred years ago, at the dawn of the twentieth century, physicists did not understand the source of the Sun‘s energy. Although classical physics had made major advances during the nineteenth century and many people thought that there was little of the physical sciences left to be discovered, they could not explain how the Sun could continue to radiate energy, apparently indefinitely. The law of energy conservation required that there must be an internal energy source equal to that radiated from the Sun‘s surface but the only substantial sources of energy known at that time were wood or coal. The mass of the Sun and the rate at which it radiated energy were known and it was easy to show that if the Sun had started off as a solid lump of coal it would have burnt out in a few thousand years. It was clear that this was much too shortœœthe Sun had to be older than the Earth and, although there was much controversy about the age of the Earth, it was clear that it had to be older than a few thousand years. The realization that the source of energy in the Sun and stars is due to nuclear fusion followed three main steps in the development of science. -
Highlights in Early Stellarator Research at Princeton
J. Plasma Fusion Res. SERIES, Vol.1 (1998) 3-8 Highlights in Early Stellarator Research at Princeton STIX Thomas H. Department of Astrophysical Sciences, Princeton University, Princeton, NJ 08540, USA (Received: 30 September 1997/Accepted: 22 October 1997) Abstract This paper presents an overview of the work on Stellarators in Princeton during the first fifteen years. Particular emphasis is given to the pioneering contributions of the late Lyman Spitzer, Jr. The concepts discussed will include equilibrium, stability, ohmic and radiofrequency plasma heating, plasma purity, and the problems associated with creating a full-scale fusion power plant. Brief descriptions are given of the early Princeton Stellarators: Model A, Model B, Model B-2, Model B-3, Models 8-64 and 8-65, and Model C, and also of the postulated fusion power plant, Model D. Keywords: Spitzer, Kruskal, stellarator, rotational transform, Bohm diffusion, ohmic heating, magnetic pumping, ion cyclotron resonance heating (ICRH), magnetic island, tokamak On March 31 of this year, at the age of 82, Lyman stellarator was brought to the headquarters of the U.S. Spitzer, Jr., a true pioneer in the fields of astrophysics Atomic Energy Commission in Washington where it re- and plasma physics, died. I wish to dedicate this presen- ceived a favorable reception. Spitzer chose the name tation to his memory. "Project Matterhorn" for the project which was to be Forty-six years ago, in early 1951, Spitzer, then sited in the Princeton area, on the newly acquired For- chair of the Department of Astronomy at Princeton restal tract, and funding began on July 1 of that year University, together with Princeton physicist John 121- Wheeler, had been thinking about the physics of ther- Spitzer's earliest stellarator papers comprise a truly monoclear processes. -
Tomographic Inversion of Wendelstein 7-X Stellarator Plasmas
45th EPS Conference on Plasma Physics P4.1056 Tomographic inversion of Wendelstein 7-X stellarator plasmas C. Brandt1, H. Thomsen1, T. Andreeva, N. Lauf1, U. Neuner1, K. Rahbarnia1, J. Schilling1, T. Broszat1, R. Laube1 and the Wendelstein 7-X Team 1 Max-Planck-Institute for Plasma Physics, Greifswald, Germany In the operational phase OP1.2a (Aug-Dec 2017) of the Wendelstein 7-X (W7-X) stellarator experiment the soft X-ray tomography diagnostic (XMCTS: soft X-ray multi camera tomogra- phy system) has been commissioned. Soft X-ray tomography systems are powerful diagnostics for high temperature plasmas measuring spatiotemporal X-ray emissivity profiles. The XMCTS consists of 20 poloidally arranged pinhole cameras at one toroidal location observing a triangu- lar shaped up-down symmetric plasma cross section. X-ray radiation is mainly emitted in the hot plasma core (electron temperatures > 1keV). In the pinhole cameras the plasma radiation is filtered by a beryllium foil of 12:5 mm thickness being transmissible for X-ray radiation above 1keV. Taking into account the detector silicon thickness of 100 mm the detectable energy range is limited to approximately 1 − 10keV. With 18 available cameras in OP1.2a the soft X-ray emissivity has been recorded along 324 lines-of-sight with a time resolution of 0:5 ms. The presentation concentrates on the preparation and first results of the tomographic inver- sion. For correct calculation of the tomograms, both, the knowledge of the exact geometry of the lines-of-sight and the sensitivity of each photodiode are of crucial importance. The as-built coordinates of the cameras have been measured after the in-vessel installation. -
Fusion Ignition Via a Magnetically-Assisted Fast Ignition Approach
Fusion ignition via a magnetically-assisted fast ignition approach W.-M. Wang1,3*, P. Gibbon2,4†, Z.-M. Sheng3,5,6‡, Y. T. Li1,3, and J. Zhang3,6 1Beijing National Laboratory for Condensed Matter Physics, Institute of Physics, CAS, Beijing 100190, China 2Forschungszentrum Jülich GmbH, Institute for Advanced Simulation, Jülich Supercomputing Centre, D-52425 Jülich, Germany 3Collaborative Innovation Center of IFSA, Shanghai Jiao Tong University, Shanghai 200240, China 4Centre for Mathematical Plasma Astrophysics, Katholieke Universiteit Leuven, 3000 Leuven, Belgium 5SUPA, Department of Physics, University of Strathclyde, Glasgow G4 0NG, United Kingdom 6Key Laboratory for Laser Plasmas (MoE) and Department of Physics and Astronomy, Shanghai Jiao Tong University, Shanghai 200240, China * E-mail: [email protected] † E-mail: [email protected] ‡ E-mail: [email protected] 1 Significant progress has been made towards laser-driven fusion ignition via different schemes, including direct and indirect central ignition, fast ignition, shock ignition, and impact ignition schemes. However, to reach ignition conditions, there are still various technical and physical challenges to be solved for all these schemes. Here, our multi-dimensional integrated simulation shows that the fast-ignition conditions could be achieved when two 2.8 petawatt heating laser pulses counter-propagate along a 3.5 kilotesla external magnetic field. Within a period of 5 picoseconds, the laser pulses heat a nuclear fuel to reach the ignition conditions. Furthermore, we present the parameter windows of lasers and magnetic fields required for ignition for experimental test. To achieve controlled nuclear fusion energy, the central ignition concept of inertial confinement fusion (ICF) was proposed in 1970s [1-4]. -
USAD Science Resource Guide • 2016–2017 • Revised Page The
sure that nuclei are energetic enough to fuse. As we have seen, hydrogen fusion in the Sun requires temperatures of at least ten million kelvin. Temperatures of this mag- nitude are difficult to achieve and maintain in a labora- tory or power plant. Achieving a single fusion reaction is not enough, how- ever; a fusion reactor, like a fission reactor, must be self- sustaining. Fusion ignition refers to the point at which a fusion reaction becomes self-sustaining. That is, the energy released by the fusion reactions continues to heat the fuel, and the external energy that was used to heat the fuel can be turned off—much like lighting a piece of pa- per with a match. Although it has not yet been achieved, reaching fusion ignition is considered an important first step toward harnessing fusion energy. The deuterium-tritium target pellet at the Fusion reactors require not only extremely high tem- peratures, but also a sufficiently high density of nuclei National Ignition Facility. to ensure that fusion reactions will occur with a great enough frequency. When atoms are heated past their 2H + 2H 3H + 1n ionization energy, their electrons are no longer bound to 1 1 2 0 (Q=3.27 MeV) the nucleus. A collection of superheated atoms forms a cloud of positively charged nuclei and negatively charged 2H + 2 H 3 H + 1 H 1 1 1 1 (Q=4.03 MeV) electrons called a plasma. Two parameters for describing the characteristics of a plasma are the plasma ion den- τ 2H + 3H 4He + 1n sity, n, and the plasma confinement time, .