Release of 108Mag from Irradiated PWR Control Rod Absorbers Under Deep Repository Conditions
Total Page:16
File Type:pdf, Size:1020Kb
Load more
Recommended publications
-
Chemistry 2100 In-Class Test 1(A)
NAME:____________________________ Student Number:______________________ Fall 2019 Chemistry 1000 Midterm #1B ____/ 65 marks INSTRUCTIONS: 1) Please read over the test carefully before beginning. You should have 5 pages of questions and a formula/periodic table sheet. 2) If your work is not legible, it will be given a mark of zero. 3) Marks will be deducted for incorrect information added to an otherwise correct answer. 4) Marks will be deducted for improper use of significant figures and for missing or incorrect units. 5) Show your work for all calculations. Answers without supporting calculations will not be given full credit. 6) You may use a calculator. 7) You have 90 minutes to complete this test. Confidentiality Agreement: I agree not to discuss (or in any other way divulge) the contents of this test until after 8:00pm Mountain Time on Thursday, October 10th, 2019. I understand that breaking this agreement would constitute academic misconduct, a serious offense with serious consequences. The minimum punishment would be a mark of 0/65 on this exam and removal of the “overwrite midterm mark with final exam mark” option for my grade in this course; the maximum punishment would include expulsion from this university. Signature: ___________________________ Date: _____________________________ Course: CHEM 1000 (General Chemistry I) Semester: Fall 2019 The University of Lethbridge Question Breakdown Spelling matters! Q1 / 4 Fluorine = F Fluorene = C13H10 Q2 / 4 Q3 / 6 Q4 / 4 Q5 / 6 Flourine = Q6 / 3 Q7 / 2 Q8 / 10 Q9 / 10 Q10 / 3 Q11 / 8 Q12 / 5 Total / 65 NAME:____________________________ Student Number:______________________ 1. Complete the following table. -
Study of Advanced Lwr Cores for Effective Use of Plutonium and Mox Physics Experiments
STUDY OF ADVANCED LWR CORES FOR EFFECTIVE USE OF PLUTONIUM AND MOX PHYSICS EXPERIMENTS T. YAMAMOTO, H. MATSU-URA*, M. UEJI, H. OTA XA9953266 Nuclear Power Engineering Corporation, Toranomon, Minato-ku, Tokyo T. KANAGAWA Mitsubishi Heavy Industries, Ltd, Nishi-ku, Yokohama K. SAKURADA Toshiba Corporation, Isogo-ku, Yokohama H.MARUYAMA Hitachi, Ltd, Hitachi-shi Japan Abstract Advanced technologies of full MOX cores have been studied to obtain higher Pu consumption based on the advanced light water reactors (APWRs and ABWRs). For this aim, basic core designs of high moderation lattice (H/HM ~5) have been studied with reduced fuel diameters in fuel assemblies for APWRs and those of high moderation lattice (H/HM ~6) with addition of extra water rods in fuel assemblies for ABWRs. The analysis of equilibrium cores shows that nuclear and thermal hydraulic parameters satisfy the design criteria and the Pu consumption rate increases about 20 %. An experimental program has been carried out to obtain the core parameters of high moderation MOX cores in the EOLE critical facility at the Cadarache Centre as a joint study of NUPEC, CEA and CEA's industrial partners. The experiments include a uranium homogeneous core, two MOX homogeneous cores of different moderation and a PWR assembly mock up core of MOX fuel with high moderation. The program was started from 1996 and will be completed in 2000. 1. INTRODUCTION In Japan, the MOX fuel demonstration programs have been performed successfully and reload size use of MOX fuel has been prepared. The recycling of plutonium in light water reactors is expected to continue in several decades. -
Chapter 2 Atoms, Molecules and Ions
Chapter 2 Atoms, Molecules and Ions PRACTICING SKILLS Atoms:Their Composition and Structure 1. Fundamental Particles Protons Electrons Neutrons Electrical Charges +1 -1 0 Present in nucleus Yes No Yes Least Massive 1.007 u 0.00055 u 1.007 u 3. Isotopic symbol for: 27 (a) Mg (at. no. 12) with 15 neutrons : 27 12 Mg 48 (b) Ti (at. no. 22) with 26 neutrons : 48 22 Ti 62 (c) Zn (at. no. 30) with 32 neutrons : 62 30 Zn The mass number represents the SUM of the protons + neutrons in the nucleus of an atom. The atomic number represents the # of protons, so (atomic no. + # neutrons)=mass number 5. substance protons neutrons electrons (a) magnesium-24 12 12 12 (b) tin-119 50 69 50 (c) thorium-232 90 142 90 (d) carbon-13 6 7 6 (e) copper-63 29 34 29 (f) bismuth-205 83 122 83 Note that the number of protons and electrons are equal for any neutral atom. The number of protons is always equal to the atomic number. The mass number equals the sum of the numbers of protons and neutrons. Isotopes 7. Isotopes of cobalt (atomic number 27) with 30, 31, and 33 neutrons: 57 58 60 would have symbols of 27 Co , 27 Co , and 27 Co respectively. Chapter 2 Atoms, Molecules and Ions Isotope Abundance and Atomic Mass 9. Thallium has two stable isotopes 203 Tl and 205 Tl. The more abundant isotope is:___?___ The atomic weight of thallium is 204.4 u. The fact that this weight is closer to 205 than 203 indicates that the 205 isotope is the more abundant isotope. -
Understanding the Astrophysical Origin of Silver, Palladium and Other Neutron-Capture Elements
Understanding the astrophysical origin of silver, palladium and other neutron-capture elements Camilla Juul Hansen M¨unchen 2010 Understanding the astrophysical origin of silver, palladium and other neutron-capture elements Camilla Juul Hansen Dissertation an der Fakult¨at f¨ur Physik der Ludwig–Maximilians–Universit¨at M¨unchen vorgelegt von Camilla Juul Hansen aus Lillehammer, Norwegen M¨unchen, den 20/12/2010 Erstgutachter: Achim Weiss Zweitgutachter: Joseph Mohr Tag der m¨undlichen Pr¨ufung: 22 M¨arz 2011 Contents 1 Introduction 1 1.1 Evolutionoftheformationprocesses . ..... 2 1.2 Neutron-capture processes: The historical perspective............ 5 1.3 Features and description of the neutron-capture processes.......... 7 1.4 Whatisknownfromobservations? . .. 9 1.5 Why study palladium and silver? . .. 15 1.6 Abiggerpicture................................. 16 2 Data - Sample and Data Reduction 19 2.1 Compositionofthesample . 19 2.1.1 Samplebiases .............................. 21 2.2 Datareduction ................................. 22 2.2.1 Fromrawtoreducedspectra. 22 2.2.2 IRAF versus UVES pipeline . 25 2.3 Merging ..................................... 26 2.3.1 Radialvelocityshift .......................... 27 3 Stellar Parameters 29 3.1 Methods for determining stellar parameters . ........ 29 3.2 Temperature................................... 30 3.2.1 Comparingtemperaturescales . 32 3.3 Gravity ..................................... 34 3.4 Metallicity.................................... 35 3.5 Microturbulence velocity, ξ .......................... -
Detailed B Depletion in Control Rods Operating in a Nuclear Boiling
UPTEC K11 015 Examensarbete 30 hp Februari 2011 Detailed 10B depletion in control rods operating in a Nuclear Boiling Water Reactor John Johnsson Abstract Detailed 10B depletion in control rods operating in a Nuclear Boiling Water Reactor John Johnsson Teknisk- naturvetenskaplig fakultet UTH-enheten In a nuclear power plant, control rods play a central role to control the reactivity of the core. In an inspection campaign of three control rods (CR 99) operated in the Besöksadress: KKL reactor in Leibstadt, Switzerland, during 6 respectively 7 consecutive cycles, Ångströmlaboratoriet Lägerhyddsvägen 1 defects were detected in the top part of the control rods due to swelling caused by 10 Hus 4, Plan 0 depletion of the neutron-absorbing B isotope (Boron-10). In order to correlate these defects to control rod depletion, the 10B depletion has in this study been Postadress: calculated in detail for the absorber pins in the top node of the control rods. Box 536 751 21 Uppsala Today the core simulator PLOCA7 is used for predicting the behavior of the reactor Telefon: core, where the retrievable information from the standard control rod follow-up is 018 – 471 30 03 the average 10B depletion for clusters of 19 absorber holes i.e. one axial node. 10 Telefax: However, the local B depletion in an absorber pin may be significantly different 018 – 471 30 00 from the node average depletion that is re-ceived from POLCA7. To learn more, the 10B depletion has been simulated for each absorber hole in the uppermost node using Hemsida: the stochastic Monte Carlo 3D simulation code MCNP as well as an MCNP- based http://www.teknat.uu.se/student 2D-depletion code (McScram). -
Boiling Water Reactor Control Rod CR 82M-1
Nuclear Fuel Boiling Water Reactor Control Rod CR 82M-1 Background CR 82M-1 Design The boiling water reactor (BWR) control rod of The hafnium tip of the CR 82M-1 design protects today must meet high operational demands and at the control rod from absorber material swelling the same time contribute to decreased operational when operated in the shutdown mode; i.e., costs for the plant operator. withdrawn from the core. The flexible B4C inventory allows for either matched or high- Description reactivity worth control rods. As structural material, American Iron and Steel Institute 316L stainless The Westinghouse BWR control rod design steel is an irradiation-resistant steel, not readily consists of four stainless steel sheets welded sensitized to irradiation-assisted stress corrosion together to form a cruciform-shaped rod. Each cracking. With an extremely low-cobalt content sheet has horizontally drilled holes to contain the (< 0.02%) in the wing material, these control rods absorber materials (B4C powder and hafnium). can play a significant role in as-low-as-reasonably- This design allows significantly more B4C to be achievable efforts. The design, with horizontally contained in the rod compared to the original drilled absorber holes, limits the washout of control rods of most reactors. B4C in the event of an anomaly in a wing, thus maintaining full reactivity worth. Westinghouse CR 82M-1 control rod for all types of BWRs Westinghouse BWR control rod CR 82M-1 Benefits CR 82M-1 is an evolutionary design based on 45 years of control rod operation -
Accident-Tolerant Control Rod
NEA/NSC/DOC(2013)9 Accident-tolerant control rod Hirokazu Ohta, Takashi Sawabe, Takanari Ogata Central Research Institute of Electric Power Industry (CRIEPI), Japan Boron carbide (B4C) and hafnium (Hf) metal are used for the neutron absorber materials of control rods in BWRs, and silver-indium-cadmium (Ag-In-Cd) alloy is used in PWRs. These materials are clad with stainless steel. The eutectic point of B4C and iron (Fe) is about 1 150°C and the melting point of Ag-In-Cd alloy is about 800°C, which are lower than the temperature of zircaloy – steam reaction increases rapidly (~1 200°C). Accordingly, it is possible that the control rods melt and collapse before the reactor core is significantly damaged in the case of severe accidents. Since the neutron absorber would be separated from the fuels, there is a risk of re-criticality, when pure water or seawater is injected for emergency cooling. In order to ensure sub-criticality and extend options of emergency cooling in the course of severe accidents, a concept of accident-tolerant control rod (ACT) has been derived. ACT utilises a new absorber material having the following properties: • higher neutron absorption than current control rod; • higher melting or eutectic temperature than 1 200°C where rapid zircaloy oxidation occurs; • high miscibility with molten fuel materials. The candidate of a new absorber material for ATC includes gadolinia (Gd2O3), samaria (Sm2O3), europia (Eu2O3), dysprosia (Dy2O3), hafnia (HfO2). The melting point of these materials and the liquefaction temperature with Fe are higher than the rapid zircaloy oxidation temperature. -
Vitae CHRISTOPHER H. GAMMONS
vitae CHRISTOPHER H. GAMMONS Ph.D. Geochemistry and Mineralogy, The Pennsylvania State University, 1988 B.S. Geology (High Honors, Magna Cum Laude, Phi Beta Kappa), Bates College, 1980 Professional Geologist, State of Wyoming, 1999 to present Dept. of Geological Engineering phone (W): (406) 496-4763 Montana Tech of the University of Montana phone (H): (406) 782-3179 Butte, Montana, 59701 FAX: (406) 496-4133 [email protected] Geology-Related Employment 2003-present Professor, Montana Tech, Dept. of Geological Engineering 2013-2016 Head of the Dept. of Geological Engineering, Montana Tech 1999-2003 Associate Professor, Montana Tech, Dept. of Geological Engineering 1997-1999 Assistant Professor, Montana Tech, Dept. of Geological Engineering 1993-1996 4/93 to 12/96: Research Associate/Faculty Lecturer, McGill University 1992-1993 2/92 to 4/93: Postdoctoral Research Fellow, Swiss Fed. Inst. Tech. (ETH) 1988-1991 11/88 to 11/91: Postdoctoral Research Fellow, Monash University, Australia 1979-1982 4/79 to 8/79; 6/80 to 11/80; 4/81 to 9/82: Exploration Geologist, Anaconda Minerals Co. Teaching Experience Classes I have taught include (19 different subjects): Hydrogeochemistry, Acid Rock Drainage, Environmental Geology, Geochemical Modeling, Hydrogeology, Introductory Petrology, Mineralogy and Petrology, Earth and Life History, Astrobiology and Evolution of the Early Earth, Economic Geology, Hydrothermal Ore Deposits, Advanced Topics in Economic Geology, Geothermal Systems, Isotope Geochemistry, Physical Geology, Geology of Montana, Introduction to Geologic Field Mapping, Field Geology (3 week summer course) and Field Hydrogeology (3 week summer course). I enjoy teaching, and have always received excellent student evaluations. This is true for introductory service classes, as well as graduate or upper level undergraduate courses. -
Apr1400 Design Control Document Tier 2
APR1400 DESIGN CONTROL DOCUMENT TIER 2 CHAPTER 4 REACTOR APR1400-K-X-FS-14002-NP REVISION 0 DECEMBER 2014 2014 KOREA ELECTRIC POWER CORPORATION & KOREA HYDRO & NUCLEAR POWER CO., LTD All Rights Reserved This document was prepared for the design certification application to the U.S. Nuclear Regulatory Commission and contains technological information that constitutes intellectual property. Copying, using, or distributing the information in this document in whole or in part is permitted only by the U.S. Nuclear Regulatory Commission and its contractors for the purpose of reviewing design certification application materials. Other uses are strictly prohibited without the written permission of Korea Electric Power Corporation and Korea Hydro & Nuclear Power Co., Ltd. Rev. 0 APR1400 DCD TIER 2 CHAPTER 4 – REACTOR TABLE OF CONTENTS NUMBER TITLE PAGE CHAPTER 4 – REACTOR ............................................................................................ 4.1-1 4.1 Summary Description ......................................................................................... 4.1-1 4.1.1 Initial Core Design Description and Permissible Changes ..................... 4.1-2 4.1.2 Analytical Techniques ............................................................................ 4.1-2 4.1.3 Combined License Information .............................................................. 4.1-2 4.2 Fuel System Design ............................................................................................. 4.2-1 4.2.1 Design Bases ......................................................................................... -
Radioactive Half-Life
Radioactive Half-Life In this lab we will measure the radioactive half-lives of two isotopes of silver. Along the way we will measure the background radioactivity due to cosmic rays. We will learn how to estimate the risk associated with exposure to radiation. RADIATION SAFETY This experiment involves the use of various radioactive sources, including a neutron howitzer containing an intensely radioactive plutonium source. The principal hazard is the (remote) possibility of contamination with plutonium leaking from the sealed source. The following rules should be followed in this lab, as in any lab where radioactive materials are present: 1. No eating or drinking in the lab. 2. Wash your hands at the end of the lab. I. Theory Background Radiation Whether we like it or not, we are constantly being bombarded by ionizing radiation from a variety of sources. A major source is cosmic rays which originate in supernovae. These very energetic primary cosmic rays interact with nuclei in the upper atmosphere and produce showers of secondary cosmic rays, a few of which reach the surface of the earth. (The cosmic radiation is twice as intense in Denver as in San Francisco, due to the difference in altitude.) Other sources of background radioactivity are radioactive elements in the concrete of this building and radon gas diffusing up out of the ground. This background rate is very low. We will measure it. Radioactivity of Silver Atoms The nuclei of most elements will readily absorb neutrons. The addition of another neutron to a given nucleus changes it to a different nuclear species, or isotope. -
Performance Comparison of Different Absorbent Materials in BWR Control Rods
PHYSOR 2004 -The Physics of Fuel Cycles and Advanced Nuclear Systems: Global Developments Chicago, Illinois, April 25-29, 2004, on CD-ROM, American Nuclear Society, Lagrange Park, IL. (2004) Performance Comparison of Different Absorbent Materials in BWR Control Rods José L. Montes*1, Juan J. Ortiz1, Raul Perusquía1 and Robert T. Perry2 1Instituto Nacional de Investigaciones Nucleares, Carr. México-Toluca Km. 36.5., Ocoyoacac Edo. De México, México. 2Los Alamos National Laboratory, PO Box 1663, Los Alamos, NM 87545, USA Nowadays there is a trend of increasing the cycle length of commercial operation in nuclear reactors. This demands to control a greater quantity of reactivity excess in this type of cycles. In this work, a comparative study of the use of various absorbent materials in the control rods of a BWR is presented. The behavior of the different absorbent material used is accomplished only from the neutron point of view. The capability of each different material to control the reactor is analyzed by studying the required control rod density and the complexity to design the target control rod patterns (CRP). The system GACRP was used to generate the target control rods patterns for an 18 months equilibrium cycle. This system is based on genetic algorithms computational technique. The found results show that the behavior of the dysprosium is acceptable and very similar to the boron one. In average, both require around 4.3% of control rod density, while in Hf cases 5.1% is needed. Although the greatest impact of including different absorbent material is noted in cold condition, GACRP could obtain a CRP in any of the considered cases. -
Co-Production of Light and Heavy $ R $-Process Elements Via Fission
Draft version June 22, 2020 Typeset using LATEX twocolumn style in AASTeX62 Co-production of Light and Heavy r-process Elements via Fission Deposition Nicole Vassh,1 Matthew R. Mumpower,2, 3 Gail C. McLaughlin,4 Trevor M. Sprouse,5 and Rebecca Surman5, 3 1University of Notre Dame, Notre Dame, IN 46556, USA 2Theoretical Division, Los Alamos National Lab, Los Alamos, NM 87545, USA 3Joint Institute for Nuclear Astrophysics - Center for the Evolution of the Elements, USA 4North Carolina State University, Raleigh, NC 27695, USA 5University of Notre Dame, Notre Dame, Indiana 46556, USA ABSTRACT We apply for the first time fission yields determined across the chart of nuclides from the macroscopic- microscopic theory of the Finite Range Liquid Drop Model to simulations of rapid neutron capture (r-process) nucleosynthesis. With the fission rates and yields derived within the same theoretical framework utilized for other relevant nuclear data, our results represent an important step toward self- consistent applications of macroscopic-microscopic models in r-process calculations. The yields from this model are wide for nuclei with extreme neutron excess. We show that these wide distributions of neutron-rich nuclei, and particularly the asymmetric yields for key species that fission at late times in the r process, can contribute significantly to the abundances of the lighter heavy elements, specifically the light precious metals palladium and silver. Since these asymmetric yields correspondingly also deposit into the lanthanide region, we consider the possible evidence for co-production by comparing our nucleosynthesis results directly with the trends in the elemental ratios of metal-poor stars rich in r-process material.