Nuclear Fission Studies with the IGISOL Method and JYFLTRAP
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Development of an On-Line Fuel Failure Monitoring System For
DEVELOPMENT OF AN ON-LINE FUEL FAILURE MONITORING SYSTEM FOR CANDU REACTORS DEVELOPPEMENT D'UN SYSTEME DE SURVEILLANCE EN LIGNE POUR DES RUPTURES DE GAINES DES REACTEURS CANDU A Thesis Submitted to the Division of Graduate Studies of the Royal Military College of Canada by Stephen Jason Livingstone, BSc, MSc Sub-Lieutenant In Partial Fulfillment of the Requirements for the Degree of Doctor of Philosophy March 2012 ©This thesis may be used within the Department of National Defence but copyright for open publication remains the property of the author. Library and Archives Bibliotheque et Canada Archives Canada Published Heritage Direction du Branch Patrimoine de I'edition 395 Wellington Street 395, rue Wellington Ottawa ON K1A0N4 Ottawa ON K1A 0N4 Canada Canada Your file Votre reference ISBN: 978-0-494-83407-7 Our file Notre reference ISBN: 978-0-494-83407-7 NOTICE: AVIS: The author has granted a non L'auteur a accorde une licence non exclusive exclusive license allowing Library and permettant a la Bibliotheque et Archives Archives Canada to reproduce, Canada de reproduire, publier, archiver, publish, archive, preserve, conserve, sauvegarder, conserver, transmettre au public communicate to the public by par telecommunication ou par Plnternet, preter, telecommunication or on the Internet, distribuer et vendre des theses partout dans le loan, distrbute and sell theses monde, a des fins commerciales ou autres, sur worldwide, for commercial or non support microforme, papier, electronique et/ou commercial purposes, in microform, autres formats. paper, electronic and/or any other formats. The author retains copyright L'auteur conserve la propriete du droit d'auteur ownership and moral rights in this et des droits moraux qui protege cette these. -
小型飛翔体/海外 [Format 2] Technical Catalog Category
小型飛翔体/海外 [Format 2] Technical Catalog Category Airborne contamination sensor Title Depth Evaluation of Entrained Products (DEEP) Proposed by Create Technologies Ltd & Costain Group PLC 1.DEEP is a sensor analysis software for analysing contamination. DEEP can distinguish between surface contamination and internal / absorbed contamination. The software measures contamination depth by analysing distortions in the gamma spectrum. The method can be applied to data gathered using any spectrometer. Because DEEP provides a means of discriminating surface contamination from other radiation sources, DEEP can be used to provide an estimate of surface contamination without physical sampling. DEEP is a real-time method which enables the user to generate a large number of rapid contamination assessments- this data is complementary to physical samples, providing a sound basis for extrapolation from point samples. It also helps identify anomalies enabling targeted sampling startegies. DEEP is compatible with small airborne spectrometer/ processor combinations, such as that proposed by the ARM-U project – please refer to the ARM-U proposal for more details of the air vehicle. Figure 1: DEEP system core components are small, light, low power and can be integrated via USB, serial or Ethernet interfaces. 小型飛翔体/海外 Figure 2: DEEP prototype software 2.Past experience (plants in Japan, overseas plant, applications in other industries, etc) Create technologies is a specialist R&D firm with a focus on imaging and sensing in the nuclear industry. Createc has developed and delivered several novel nuclear technologies, including the N-Visage gamma camera system. Costainis a leading UK construction and civil engineering firm with almost 150 years of history. -
CME Search Before Isobar Collisions and Blind Analysis from STAR
CME Search Before Isobar Collisions and Blind Analysis From STAR Prithwish Tribedy for the STAR collaboration The 36th Winter Workshop on Nuclear Dynamics 1-7th March, 2020, Puerto Vallarta, Mexico In part supported by Introduction Solenoidal Tracker at RHIC (STAR) RHIC has collided multiple ion species; year 2018 was dedicated to search for effects driven by strong electromagnetic fields by STAR Isobars: Ru+Ru, Zr+Zr @ 200GeV (2018) Low energy: Au+Au 27 GeV (2018) Large systems : U+U, Au+Au @ 200 GeV P.Tribedy, WWND 2 The Chiral Magnetic Effect (Cartoon Picture) Quarks Quarks randomly aligned oriented along B antiquarks I II III IV More More right left handed handed quarks quarks J || B J || -B CME converts chiral imbalance to observable electric current P.Tribedy, WWND 2020 3 New Theory Guidance : Complexity Of An Event Magnetic field map Pb+Pb @ 2.76 TeV Axial charge profile b=11.4 fm, Npart=56 Pb+Pb 2.76 TeV, b=11.4 fm, dN5/dxT [a.u.] 0.3 6 uR>uL 0.2 4 uR<uL 0.1 2 0 0 y [fm] -2 -0.1 -4 -0.2 -6 -0.3 -6 -4 -2 0 2 4 6 x [fm] Based on: Chatterjee, Tribedy, Phys. Rev. C 92, Based on: Lappi, Schlichting, Phys. Rev. D 97, 011902 (2015) 034034 (2018) Going beyond cartoon picture: 1) Fluctuations dominate e-by-e physics, 2) B-field & domain size of axial-charge change with √s P.Tribedy, WWND 2020 4 New Theory Guidance : Complexity Of An Event Pb+Pb @ 2.76 TeV Magnetic field b=11.4 fm, N Axial charge profile Pb+Pb 2.76 TeV, b=11.4 fm, dN5/dxT [a.u.] 0.3 6 u 0.2 4 u 0.1 2 0 0 y [fm] -2 -0.1 -4 -0.2 -6 -0.3 -6 -4 -2 0 2 4 6 x [fm] Based on: Chatterjee, -
Search for Isobar Nuclei in Mass Distributions of Heavy Fission Fragments of 235U Nuclei by Thermal Neutrons
International Conference “Nuclear Science and its Application”, Samarkand, Uzbekistan, September 25-28, 2012 SEARCH FOR ISOBAR NUCLEI IN MASS DISTRIBUTIONS OF HEAVY FISSION FRAGMENTS OF 235U NUCLEI BY THERMAL NEUTRONS Abdullaeva G.A., Koblik Yu.N., Nebesniy A.F., Pikul V.P. Institute of Nuclear Physics, Tashkent, Uzbekistan To search for isobar nuclei in mass distributions of 235U nuclei heavy fission fragments (FF) caused by thermal neutrons we used experimental data from [1]. In [1] experimental data of yields for each value of mass number in FF mass numbers range from A=125 to A=155 a.m.u. depending on effective charge state z* are published. In figure 1 such experimental dependence of FF yields Yi (Ai) =f(z*) and processing of this dependence by Gauss distribution with an error to one σ for each z* is presented. The basic difficulty consisted in correct transition from measured z* to charges of heavy fragments at the moment of nuclear fission. For this purpose we used the modified expression from [2] in the form of: k * α k1 i i ii VzV1zz 0 . Here zi* and zi - the measured effective charge of the i-th ion with mass number Ai and a charge of corresponding fragment, Vi - velocity of ion, Vo - average velocity of electrons interacting with fragment in the target matter and influencing to formation of an effective charge of the ion. Velocity Vi was defined with use of measured value Ek for each fragment. Velocity Vo can 8 changes in limits from Vo = 2.2×10 cm/s - electron velocity in the first orbit of hydrogen atom to 3.6×108 cm/s [2], constants: α =0.45 and k =0.6 are taken as from [2]. -
Models of the Atomic Nucleus
Models of the Atomic Nucleus Second Edition Norman D. Cook Models of the Atomic Nucleus Unification Through a Lattice of Nucleons Second Edition 123 Prof. Norman D. Cook Kansai University Dept. Informatics 569 Takatsuki, Osaka Japan [email protected] Additional material to this book can be downloaded from http://extras.springer.com. ISBN 978-3-642-14736-4 e-ISBN 978-3-642-14737-1 DOI 10.1007/978-3-642-14737-1 Springer Heidelberg Dordrecht London New York Library of Congress Control Number: 2010936431 © Springer-Verlag Berlin Heidelberg 2006, 2010 This work is subject to copyright. All rights are reserved, whether the whole or part of the material is concerned, specifically the rights of translation, reprinting, reuse of illustrations, recitation, broadcasting, reproduction on microfilm or in any other way, and storage in data banks. Duplication of this publication or parts thereof is permitted only under the provisions of the German Copyright Law of September 9, 1965, in its current version, and permission for use must always be obtained from Springer. Violations are liable to prosecution under the German Copyright Law. The use of general descriptive names, registered names, trademarks, etc. in this publication does not imply, even in the absence of a specific statement, that such names are exempt from the relevant protective laws and regulations and therefore free for general use. Cover design: WMXDesign GmbH, Heidelberg Printed on acid-free paper Springer is part of Springer Science+Business Media (www.springer.com) Preface to the Second Edition Already by the 1970s, some theorists had declared that nuclear structure physics was a “closed chapter” in science, but since then it has repeatedly been found necessary to re-open this closed chapter to address old problems and to explain new phenom- ena. -
Study of Macromolecule-Mineral Interactions on Nuclear Related Materials
Study of macromolecule-mineral interactions on nuclear related materials by Lygia Eleftheriou Submitted in partial fulfillment of the requirements for the degree of Doctor of Philosophy Supervised by: Prof John Harding Dr Maria Romero-González The University of Sheffield Faculty of Engineering Department of Materials Science and Engineering September 2016 Declaration The work described within this thesis has been completed under the supervision of Prof J. Harding and Dr M. Romero-González at the University of Sheffield between September 2012 and September 2016. This thesis along with the work described here has been completed by the author with some exceptions indicated clearly at the relevant chapters. These include: (1) the construction of ceria models for the computational work that was completed by Dr Colin Freeman and Dr Shaun Hall (described in chapter 5), (2) the purification of peptidoglycan completed by Dr Stephane Mesnage (described in chapter 4) and (3) the electron microscopy analysis completed by Dr Mohamed Merroun (described in chapter 2). Lygia Eleftheriou September 2016 Acknowledgements I would like to express my sincere gratitude to my supervisors Dr Maria Romero González and Prof John Harding for all their support during the past four years. This work would not have been possible without their endless encouragement, guidance and advice. I would also like to thank Dr Colin Freeman, Dr Shaun Hall and Riccardo Innocenti Malini for all the hours they spent trying to make things work and all their help with the computational part of this project. In addition, I would like to thank Dr Simon Thorpe, Dr Stephane Mesnage and Mr Robert Hanson for their help with the analytical methods of this project. -
Arxiv:1901.01410V3 [Astro-Ph.HE] 1 Feb 2021 Mental Information Is Available, and One Has to Rely Strongly on Theoretical Predictions for Nuclear Properties
Origin of the heaviest elements: The rapid neutron-capture process John J. Cowan∗ HLD Department of Physics and Astronomy, University of Oklahoma, 440 W. Brooks St., Norman, OK 73019, USA Christopher Snedeny Department of Astronomy, University of Texas, 2515 Speedway, Austin, TX 78712-1205, USA James E. Lawlerz Physics Department, University of Wisconsin-Madison, 1150 University Avenue, Madison, WI 53706-1390, USA Ani Aprahamianx and Michael Wiescher{ Department of Physics and Joint Institute for Nuclear Astrophysics, University of Notre Dame, 225 Nieuwland Science Hall, Notre Dame, IN 46556, USA Karlheinz Langanke∗∗ GSI Helmholtzzentrum f¨urSchwerionenforschung, Planckstraße 1, 64291 Darmstadt, Germany and Institut f¨urKernphysik (Theoriezentrum), Fachbereich Physik, Technische Universit¨atDarmstadt, Schlossgartenstraße 2, 64298 Darmstadt, Germany Gabriel Mart´ınez-Pinedoyy GSI Helmholtzzentrum f¨urSchwerionenforschung, Planckstraße 1, 64291 Darmstadt, Germany; Institut f¨urKernphysik (Theoriezentrum), Fachbereich Physik, Technische Universit¨atDarmstadt, Schlossgartenstraße 2, 64298 Darmstadt, Germany; and Helmholtz Forschungsakademie Hessen f¨urFAIR, GSI Helmholtzzentrum f¨urSchwerionenforschung, Planckstraße 1, 64291 Darmstadt, Germany Friedrich-Karl Thielemannzz Department of Physics, University of Basel, Klingelbergstrasse 82, 4056 Basel, Switzerland and GSI Helmholtzzentrum f¨urSchwerionenforschung, Planckstraße 1, 64291 Darmstadt, Germany (Dated: February 2, 2021) The production of about half of the heavy elements found in nature is assigned to a spe- cific astrophysical nucleosynthesis process: the rapid neutron capture process (r-process). Although this idea has been postulated more than six decades ago, the full understand- ing faces two types of uncertainties/open questions: (a) The nucleosynthesis path in the nuclear chart runs close to the neutron-drip line, where presently only limited experi- arXiv:1901.01410v3 [astro-ph.HE] 1 Feb 2021 mental information is available, and one has to rely strongly on theoretical predictions for nuclear properties. -
Appendix: Key Concepts and Vocabulary for Nuclear Energy
Appendix: Key Concepts and Vocabulary for Nuclear Energy The likelihood of fission depends on, among other Power Plant things, the energy of the incoming neutron. Some In most power plants around the world, heat, usually nuclei can undergo fission even when hit by a low- produced in the form of steam, is converted to energy neutron. Such elements are called fissile. electricity. The heat could come through the burning The most important fissile nuclides are the uranium of coal or natural gas, in the case of fossil-fueled isotopes, uranium-235 and uranium-233, and the power plants, or the fission of uranium or plutonium plutonium isotope, plutonium-239. Isotopes are nuclei. The rate of electrical power production in variants of the same chemical element that have these power plants is usually measured in megawatts the same number of protons and electrons, but or millions of watts, and a typical large coal or nuclear differ in the number of neutrons. Of these, only power plant today produces electricity at a rate of uranium-235 is found in nature, and it is found about 1,000 megawatts. A much smaller physical only in very low concentrations. Uranium in nature unit, the kilowatt, is a thousand watts, and large contains 0.7 percent uranium-235 and 99.3 percent household appliances use electricity at a rate of a few uranium-238. This more abundant variety is an kilowatts when they are running. The reader will have important example of a nucleus that can be split only heard about the “kilowatt-hour,” which is the amount by a high-energy neutron. -
Physics 111 Fall 2007 Radioactive Decay Problems Solutions
Physics 111 Fall 2007 Radioactive Decay Problems Solutions 3 1. The 1 H isotope of hydrogen, which is called tritium (because it contains three nucleons), has a half-life of 12.33 yr. It can be used to measure the age of objects up to about 100 yr. It is produced in the upper atmosphere by cosmic rays and brought to Earth by rain. As an application, determine approximately the age of a bottle of wine 3 1 whose 1 H radiation is about 10 that present in new wine. Because the tritium in water is being replenished, we assume that the amount is constant until the wine is made, and then it decays. We find the number of half-lives from N n = 1 ; N ()2 0 n 0.10 = 1 , or n log 2 = log 10 , which gives n = 3.32. ()2 () Thus the time is t = nT = 3.32 12.33 yr = 41 yr. 1 ()() 2 2. Strontium-90 is produced as a nuclear fission product of uranium in both reactors and atomic bombs. Look at its location in the periodic table to see what other elements it might be similar to chemically, and tell why you think it might be dangerous to ingest. It has too many neutrons, and it decays with a half-life of about 29 yr. How 90 long will we have to wait for the amount of 38 Sr on the Earth’s surface to reach 1% of its current level, assuming no new material is scattered about? Write down the decay reaction, including the daughter nucleus. -
Perspective the Radioactivity of Atmospheric Krypton in 1949–1950
Proc. Natl. Acad. Sci. USA Vol. 94, pp. 7807–7810, July 1997 Perspective The radioactivity of atmospheric krypton in 1949–1950 Anthony Turkevich*, Lester Winsberg†, Howard Flotow‡, and Richard M. Adams§ Argonne National Laboratory, 9700 S. Cass Avenue, Argonne, IL 60439 Contributed by Anthony Turkevich, April 10, 1997 ABSTRACT The chemical element krypton, whose prin- Libby (in 1948; unpublished work) gave indications that these cipal source is the atmosphere, had a long-lived radioactive predictions were correct. The present report describes the content, in the mid-1940s, of less than 5 dpm per liter of technique that was used soon afterward to establish more krypton. In the late 1940s, this content had risen to values in precisely that atmospheric krypton in the late 1940s was much the range of 100 dpm per liter. It is now some hundred times more radioactive than it had been, and gives the results of some higher than the late 1940 values. This radioactivity is the early measurements of krypton samples isolated from the result of the dissolving of nuclear fuel for military and civilian atmosphere at that time.** purposes, and the release thereby of the fission product krypton-85 (half-life 5 10.71 years, fission yield 5 0.2%). The Measurement Technique present largest emitter of krypton-85 is the French reprocess- ing plant at Cap-de-la-Hague. The measurement technique that was used was influenced by those simultaneously being developed by Libby and Anderson It is generally known that the chemical element krypton, (9) to measure the radiocarbon content of samples of arche- isolated from the atmosphere in 1996, is radioactive. -
The Nucleus and Nuclear Instability
Lecture 2: The nucleus and nuclear instability Nuclei are described using the following nomenclature: A Z Element N Z is the atomic number, the number of protons: this defines the element. A is called the “mass number” A = N + Z. N is the number of neutrons (N = A - Z) Nuclide: A species of nucleus of a given Z and A. Isotope: Nuclides of an element (i.e. same Z) with different N. Isotone: Nuclides having the same N. Isobar: Nuclides having the same A. [A handy way to keep these straight is to note that isotope includes the letter “p” (same proton number), isotone the letter “n” (same neutron number), and isobar the letter “a” (same A).] Example: 206 82 Pb124 is an isotope of 208 82 Pb126 is an isotone of 207 83 Bi124 and an isobar of 206 84 Po122 1 Chart of the Nuclides Image removed. 90 natural elements 109 total elements All elements with Z > 42 are man-made Except for technicium Z=43 Promethium Z = 61 More than 800 nuclides are known (274 are stable) “stable” unable to transform into another configuration without the addition of outside energy. “unstable” = radioactive Images removed. [www2.bnl.gov/ton] 2 Nuclear Structure: Forces in the nucleus Coulomb Force Force between two point charges, q, separated by distance, r (Coulomb’s Law) k0 q1q2 F(N) = 9 2 -2 r 2 k0 = 8.98755 x 10 N m C (Boltzman constant) Potential energy (MeV) of one particle relative to the other k q q PE(MeV)= 0 1 2 r Strong Nuclear Force • Acts over short distances • ~ 10-15 m • can overcome Coulomb repulsion • acts on protons and neutrons Image removed. -
Status of Fission Product Yield Data for Thermal Reactors
Atomic Energy of Canada Limited STATUS OF FISSION PRODUCT YIELD DATA FOR THERMAL REACTORS by W.H. WALKER Chalk River Nuclear Laboratories Chalk River, Ontario February 1974 AECL-4704, tr - STATUS OF FISSION PRODUCT YIELD DATA FOR THERMAL REACTORS W.H. Walker Review Paper lla for the I.A.E.A. Panel on Fission Product Nuclear Data, held at Bologna, Italy, November 26 - 30, 1973. Chalk River Nuclear Laboratories Chalk River, Ontario February 1974 AECL-4704 STATUS OF FISSION PRODUCT YIELD DATA FOR THERMAL REACTORS by W.H. Walker ABSTRACT Methods of measuring fission product yields are discussed. Measured and evaluated chain yields from thermal neutron fission of 233U, 235U, 239Pu and 21flPu are reviewed and evaluated yields are compared in an appendix. Measured fractional and direct yields of interest in reactor cal- culations are discussed and compiled in an appendix. The few data on cumulative yields from fission by low energy epithermal neutrons are noted and their significance in reactor calculations estimated. Chalk River Nuclear Laboratories Chalk River, Ontario February 1974 AECL-4704 Connaissances actuelles, en matière de rendement des produits de fission, pour les réacteurs thermiques par W.H. Walker Résumé Les méthodes permettant de mesurer le rendement des produits de fission font l'objet de commentaires. Des rendements en chaîne ayant été mesurés et évalués à partir 2 3 3 235 239 de la fission, par neutrons thermiques, de U, U, Pu 241 et Pu sont passés en revue et les rendements évalués font l'objet d'une comparaison dans une annexe. Les rende- ments mesurés, directs ou fractionnels, qui présentent un intérêt pour les calculs de réacteur font l'objet de commen- taires et ils sent compilés dans une annexe.