Analysis of Isotope Ratio of 232U/233U in Irradiated Thoria by Alpha Spectrometry

Total Page:16

File Type:pdf, Size:1020Kb

Analysis of Isotope Ratio of 232U/233U in Irradiated Thoria by Alpha Spectrometry ANALYSIS OF ISOTOPE RATIO OF 232U/233U IN IRRADIATED THORIA BY ALPHA SPECTROMETRY A.Dakshinamoorthy, P.V.Achuthan, D.S.Divakar, R.Kannan, U.Jambunathan, A.Ramanujam, P.B.Gurba*, R.K.Babber* Fuel Reprocessing Division Bhabha Atomic Research Centre Department of Atomic Energy, Trombay, Mumbai- 400 085. Abstract Indian nuclear program envisages the use of vast deposits of thorium in the country at the second stage for the production of 233U, a fissile material. Among the other isotopes produced, 232U content is of greater significance to fuel reprocessors as its daughter products contribute to high level of gamma dose during reprocessing. Alpha spectrometric method for the isotope ratio of 232U/233U in irradiated thoria has been successfully developed in our laboratory. The report describes the separation procedure followed using Tri-n-Octyl Phosphine Oxide (TOPO) for the purification of uranium from its daughter products and alpha spectrometric method followed for determining 232U content. Alpha spectrum evaluation is also explained in detail. Comparison of spectra from sources prepared prior and after separation forms the method for determining 228 Th activity in uranium. The method is simple and fast. Key words: Alpha spectrometry, Uranium, 232U, 233U, Thorium, 228Th, Reprocessing, Irradiated fuels * Power Reactor Fuel Reprocessing Plant, Bhabha Atomic Research Centre, Tarapur 1. INTRODUCTION India has adopted a three stage nuclear program1 wherein large amount of thorium available in the country will be utilised in the second stage for the production of 233U, which in turn will be used as fuel for the third stage. 232Th is converted to 233U by nuclear reaction in a reactor. In addition to 233U, other isotopes of uranium namely 232, 234, 235 and 236 are also produced. Determination of 232U content is important as it undergoes decay as per the decay chain shown in figure 1. Some of the daughter products are high energy gamma emitters and contributes significantly to the gamma dose during processing. Hence determination of 232U i.e. isotopic composition of uranium produced is one of the important parameters in 233U processing. Thermal ionisation mass spectrometry is normally followed for precise and accurate isotope ratio measurement of uranium2. Difficulty arises in the measurement of 232U content by mass spectrometry due to isobaric interference of 232Th, the major constituent in the sample. Hence alpha spectrometry has been followed in the present work for the determination of 232U present along with 233U in the sample. Alpha energies and branching intensities of uranium isotopes of interest and various daughter products of 232U decay chain are shown in table 1. It is evident that 232U and 228Th are having alpha energies closeby. 224Ra is also contributing to the 232U peak to the extent of 5%. Therefore, presence of these daughter products will interfere in the estimation of 232U by alpha spectrometry. Hence a separation of uranium from thorium is necessary prior to alpha spectrometry. An extractive spectrophotometric and radiometric method has already been reported from our laboratory3 for the determination of 233U. The radiometric method requires specific activity of uranium for finding the uranium concentration. Presence of small amount of 232U will drastically alter the specific activity of uranium. Our present work by alpha spectrometry will be useful in determining the specific activity of uranium in the sample. Separation procedure followed for removing the major constituent i.e. thorium is the same one reported earlier3. The separation steps involve complexing thorium with fluoride followed by solvent extraction using TOPO in xylene. Alpha spectrum of the source prepared from the TOPO extract was used for evaluation. The paper describes the procedure followed for separation of irradiated thorium sample and alpha spectrometric analysis carried out to find out the alpha activity ratio of 232U/233U. The atom ratio of 232/233 calculated from the activity ratio measured. 228Th is also estimated from the spectra obtained prior and after separation. 2. EXPERIMENTAL 2.1 Instruments 2.1.1 Alpha spectrometer Alpha spectrometer used consists of a vacuum chamber designed and fabricated in-house by Technical Physics & Prototype Engineering Division, Bhabha Atomic Research Centre, Trombay, connected to a rotary pump and fitted with pyrani gauge to measure the pressure in the chamber. A vacuum of better than 1x10-2 mbar is obtained in the chamber. A Silicon Surface Barrier detector of 300 mm2, with a resolution of 30 keV at 5.5 MeV is used. DC voltage of +100V is applied. The output of the detector is connected to a preamplifier, spectroscopy amplifier and PC based 8 K multichannel analyser (MCA) card Emacplus with MCA emulation software. 2.1.2 Sample preparation Irradiated thorium oxide pellet is dissolved in conc. HNO3 containing HF and aluminium nitrate. After dissolution it is made upto 25 ml. Suitable dilutions are made from the stock solution for further analyses. 2.1.3 Tri-n-octyl posphine oxide (TOPO) 0.05 M TOPO in xylene is prepared by dissolving 1.9338 g of TOPO, Fluka AG in 100 ml of xylene. 2.1.4. Sodium fluoride solution 4% NaF solution is prepared by dissolving 4 g of NaF (AR) in 100 ml of water and filtered. 2.1.5 2 M HNO3 By suitable dilution of AR grade conc. HNO3 . 2.1.6 Source material: 1” stainless steel disc of 0.3 mm thick having polished surface is used as backing material for preparing source to carry out alpha spectrometry work. 2.2 Procedure 2.2.1 Source preparation Suitable aliquot of the sample containing ~10 microgram of 233U along with milligram amount of thorium is conditioned to 2 M HNO3 and 2 ml of 4% fluoride solution is added and subjected to solvent extraction separation using 0.05 M TOPO as per the procedure reported3. 50 microlitre of the organic extract is placed on an SS disc, dried on a hot plate and fired in bunsen burner. A directly evaporated source is also prepared without separation by placing small volume of the sample solution (50 -100 microlitre) on an SS disc, drying & firing in a flame. 2.2.2 Spectrum analysis The source disc is placed in the vacuum chamber that has adjustable sample tray for counting. The distance between source and detector is maintained at 10 mm. The detector chamber is evacuated to a pressure of less than 4x10-2 mbar. Counting is continued till a minimum of 20,000 counts under region of interest (ROI) in the energy regions of 233U and 232U are accumulated. 2.2.3 Spectrum evaluation i) Correction for tail contribution: Difficulty arises in the determination of activity ratio of 232U/233U from the alpha spectrum because of tail contribution of higher energy peak to lower energy peak due to energy degradation of alpha particles before reaching the detector. Eventhough the problem is minimised under vacuum, it is not totally eliminated. Hence the tail contribution has to be corrected. A number of computer programs 4-9 have been developed for the correction of alpha activity ratio of 238Pu/ (239+240)Pu obtained from the evaluation of plutonium spectrum and a geometric progression (GP) decrease method has been followed successfully in our centre10. The method has been used earlier for the determination of 234U/238U alpha activity ratio measurements.11. The same GP correction method is adopted for evaluating 232U/233U activity ratio from the spectrum. Here the spectrum is divided into four regions A,B,C and D, where A is 232U region, B is 233U region and C & D are regions marked for evaluation of the correction required for tail contribution. Each region has same number of channels and number of channel between any two regions is the same. A The corrected ratio R1 = ------------------------- --------1 {B - AC/(B+AD/C)} 2.2.4 Correction for the presence of 234U : Presence of 234U in 233U sample will contribute to the peak of 233U as the alpha energy of 234U (4.77 MeV) and 233U ( 4.78, 4.82MeV) are close by and their half lives are comparable. Hence 233U peak has to be corrected for contribution from small amount of 234U.The correction is done as follows: Activity at 5.32 MeV N232 λ232 ------------------------ = --------------------------- = R1 --------- 2 Activity at 4.82 MeV N233 λ233 + N234 λ234 where Ni and λ i are the number of atoms and decay constants of isotope Activity ratio of 5.32 MeV/4.82 MeV after tail contribution is R1 . Dividing by N233 both denominator & numerator in equation 2, ( N232/N233) λ232 R1 = ----------------------------------- -------- 3 λ233 + (N234/N233 ) λ234 Rearranging 3 ( N232λ232) N234 λ234 R2 = ------------- = R1(1+ ------ x -----) --------- 4 (N233 λ233) N233 λ233 N234/N233 is available from mass spectrometric analysis, and λ234, λ233 are decay constants of 234 233 232 233 U and U available from literature. R2 is the alpha activity ratio of U to U. Isotope ratio of 232U/233U can be determined by rearranging the equation 4, N232/N233= R2 x λ233/λ232 ---------- 5 2.2.5 228Th determination Activity ratio of 228Th to 233U is determined from the spectrum of direct evaporated source. Two methods of evaluation are followed. Method 1 As it is seen from the spectrum of direct evoporated source in Figure 2, 228Th peak at 5.43 MeV is separated from 232U peak at 5.32 MeV. Hence it is possible to calculate the alpha activity and content of 228Th from the alpha spectrum of direct evaporated source. Five regions A’, A, B, C, D are marked where A’ is peak area of 228Th, A is peak area of 232U , B is peak area of 233U peak with minor contribution due to 234U and tail of U232 and C & D are regions on 233U tail contribution, marked for correction purpose as described already.
Recommended publications
  • 22.101 Applied Nuclear Physics (Fall 2006) Problem Set No. 1 Due: Sept
    22.101 Applied Nuclear Physics (Fall 2006) Problem Set No. 1 Due: Sept. 13, 2006 Problem 1 Before getting into the concepts of nuclear physics, every student should have some feeling for the numerical values of properties of nuclear radiations, such as energy and speed, wavelength, and frequency, etc. This involves some back of the envelope calculations using appropriate universal constants. (i) A thermal neutron in a nuclear reactor is a neutron with kinetic energy equal to kBT, where kB is the Boltzmann’s constant and T is the temperature of the reactor. Explain briefly the physical basis of this statement. Taking T to be the room temperature, 20C, calculate the energy of the thermal neutron (in units of ev), and then find its speed v (in cm/sec), the de Broglie wavelength λ (in A) and circular frequency ω (radian/sec). Compare these values with the energy, speed, and interatomic distance of atoms that make up the materials in the reactor. What is the point of comparing the neutron wavelength with typical atomic separations in a solid? (ii) Consider a 2 Kev x-ray, calculate the frequency and wavelength of this photon. What would be the point of comparing the x-ray wavelength with that of the thermal neutron? For an electron with wavelength equal to that of the thermal neutron, what energy would it have? 2 2 (iii) The classical radius of the electron, defined as e / mec , with e being the electron charge, me the electron rest mass, and c the speed of light, has the value of 2.818 x 10-13 cm.
    [Show full text]
  • Problem Set 3 Solutions
    22.01 Fall 2016, Problem Set 3 Solutions October 9, 2016 Complete all the assigned problems, and do make sure to show your intermediate work. 1 Activity and Half Lives 1. Given the half lives and modern-day abundances of the three natural isotopes of uranium, calculate the isotopic fractions of uranium when the Earth first formed 4.5 billion years ago. Today, uranium consists of 0.72% 235U, 99.2745% 238U, and 0.0055% 234U. However, it is clear that the half life of 234U (245,500 years) is so short compared to the lifetime of the Earth (4,500,000,000 years) that it would have all decayed away had there been some during the birth of the Earth. Therefore, we look a little closer, and find that 234U is an indirect decay product of 238U, by tracing it back from its parent nuclides on the KAERI table: α β− β− 238U −! 234T h −! 234P a −! 234U (1) Therefore we won’t consider there being any more 234U than would normally be in equi­ librium with the 238U around at the time. We set up the two remaining equations as follows: −t t ;235 −t t ;238 = 1=2 = 1=2 N235 = N0235 e N238 = N0238 e (2) Using the current isotopic abundances from above as N235 and N238 , the half lives from n 9 t 1 1 the KAERI Table of Nuclides t =2;235 = 703800000 y; t =2;238 = 4:468 · 10 y , and the lifetime of the earth in years (keeping everything in the same units), we arrive at the following expressions for N0235 and N0238 : N235 0:0072 N238 0:992745 N0235 =−t = 9 = 4:307N0238 =−t = 9 = 2:718 (3) =t1 ;235 −4:5·10 =7:038·108 =t1 ;238 −4:5·10 =4:468·109 e =2 e e =2 e Finally, taking the ratios of these two relative abundances gives us absolute abundances: 4:307 2:718 f235 = = 0:613 f238 = = 0:387 (4) 4:307 + 2:718 4:307 + 2:718 235U was 61.3% abundant, and 238U was 38.7% abundant.
    [Show full text]
  • Module01 Nuclear Physics and Reactor Theory
    Module I Nuclear physics and reactor theory International Atomic Energy Agency, May 2015 v1.0 Background In 1991, the General Conference (GC) in its resolution RES/552 requested the Director General to prepare 'a comprehensive proposal for education and training in both radiation protection and in nuclear safety' for consideration by the following GC in 1992. In 1992, the proposal was made by the Secretariat and after considering this proposal the General Conference requested the Director General to prepare a report on a possible programme of activities on education and training in radiological protection and nuclear safety in its resolution RES1584. In response to this request and as a first step, the Secretariat prepared a Standard Syllabus for the Post- graduate Educational Course in Radiation Protection. Subsequently, planning of specialised training courses and workshops in different areas of Standard Syllabus were also made. A similar approach was taken to develop basic professional training in nuclear safety. In January 1997, Programme Performance Assessment System (PPAS) recommended the preparation of a standard syllabus for nuclear safety based on Agency Safely Standard Series Documents and any other internationally accepted practices. A draft Standard Syllabus for Basic Professional Training Course in Nuclear Safety (BPTC) was prepared by a group of consultants in November 1997 and the syllabus was finalised in July 1998 in the second consultants meeting. The Basic Professional Training Course on Nuclear Safety was offered for the first time at the end of 1999, in English, in Saclay, France, in cooperation with Institut National des Sciences et Techniques Nucleaires/Commissariat a l'Energie Atomique (INSTN/CEA).
    [Show full text]
  • Phys586-Lec01-Radioa
    Introduction ¾A more general title for this course might be “Radiation Detector Physics” ¾Goals are to understand the physics, detection, and applications of ionizing radiation The emphasis for this course is on radiation detection and applications to radiological physics However there is much overlap with experimental astro-, particle and nuclear physics And examples will be drawn from all of these fields 1 Introduction ¾While particle and medical radiation physics may seem unrelated, there is much commonality Interactions of radiation with matter is the same Detection principals of radiation are the same Some detectors are also the same, though possibly in different guises ¾Advances in medical physics have often followed quickly from advances in particle physics 2 Introduction ¾ Roentgen discovered x-rays in 1895 (Nobel Prize in 1901) ¾ A few weeks later he was photographing his wife’s hand ¾ Less than a year later x-rays were becoming routine in diagnostic radiography in US, Europe, and Japan ¾ Today the applications are ubiquitous (CAT, angiography, fluoroscopy, …) 3 Introduction ¾ Ernest Lawrence invented the cyclotron accelerator in 1930 (Nobel Prize in 1939) ¾ Five years later, John Lawrence began studies on cancer treatment using radioisotopes and neutrons (produced with the cyclotron) ¾ Their mother saved from cancer using massive x- ray dose 4 Introduction ¾Importance and relevance Radiation is often the only observable available in processes that occur on very short, very small, or very large scales Radiation detection
    [Show full text]
  • Nuclear Physics and Astrophysics SPA5302, 2019 Chris Clarkson, School of Physics & Astronomy [email protected]
    Nuclear Physics and Astrophysics SPA5302, 2019 Chris Clarkson, School of Physics & Astronomy [email protected] These notes are evolving, so please let me know of any typos, factual errors etc. They will be updated weekly on QM+ (and may include updates to early parts we have already covered). Note that material in purple ‘Digression’ boxes is not examinable. Updated 16:29, on 05/12/2019. Contents 1 Basic Nuclear Properties4 1.1 Length Scales, Units and Dimensions............................7 2 Nuclear Properties and Models8 2.1 Nuclear Radius and Distribution of Nucleons.......................8 2.1.1 Scattering Cross Section............................... 12 2.1.2 Matter Distribution................................. 18 2.2 Nuclear Binding Energy................................... 20 2.3 The Nuclear Force....................................... 24 2.4 The Liquid Drop Model and the Semi-Empirical Mass Formula............ 26 2.5 The Shell Model........................................ 33 2.5.1 Nuclei Configurations................................ 44 3 Radioactive Decay and Nuclear Instability 48 3.1 Radioactive Decay...................................... 49 CONTENTS CONTENTS 3.2 a Decay............................................. 56 3.2.1 Decay Mechanism and a calculation of t1/2(Q) .................. 58 3.3 b-Decay............................................. 62 3.3.1 The Valley of Stability................................ 64 3.3.2 Neutrinos, Leptons and Weak Force........................ 68 3.4 g-Decay...........................................
    [Show full text]
  • Periodic Table of Elements
    The origin of the elements – Dr. Ille C. Gebeshuber, www.ille.com – Vienna, March 2007 The origin of the elements Univ.-Ass. Dipl.-Ing. Dr. techn. Ille C. Gebeshuber Institut für Allgemeine Physik Technische Universität Wien Wiedner Hauptstrasse 8-10/134 1040 Wien Tel. +43 1 58801 13436 FAX: +43 1 58801 13499 Internet: http://www.ille.com/ © 2007 © Photographs of the elements: Mag. Jürgen Bauer, http://www.smart-elements.com 1 The origin of the elements – Dr. Ille C. Gebeshuber, www.ille.com – Vienna, March 2007 I. The Periodic table............................................................................................................... 5 Arrangement........................................................................................................................... 5 Periodicity of chemical properties.......................................................................................... 6 Groups and periods............................................................................................................. 6 Periodic trends of groups.................................................................................................... 6 Periodic trends of periods................................................................................................... 7 Examples ................................................................................................................................ 7 Noble gases .......................................................................................................................
    [Show full text]
  • HANDBOOK on NUCLEAR DATA for BOREHOLE LOGGING and MINERAL ANALYSIS the Following States Are Members of the International Atomic Energy Agency
    E = 14.00 MeV Sin SIGTOT = 1.81 b MFP = 11.08 cm I TOTAL INELASTIC {n, 2n) {n, no) (n, n'p) (n, d) 2.6% 0.4% 4.3% 1.0% TECHNICAL REPORTS SERIES No. 357 Handbook on ^ l INTERNATIONAL ATOMIC ENERGY AGENCY, VIENNA, 1993 HANDBOOK ON NUCLEAR DATA FOR BOREHOLE LOGGING AND MINERAL ANALYSIS The following States are Members of the International Atomic Energy Agency: AFGHANISTAN HAITI PANAMA ALBANIA HOLY SEE PARAGUAY ALGERIA HUNGARY PERU ARGENTINA ICELAND PHILIPPINES AUSTRALIA INDIA POLAND AUSTRIA INDONESIA PORTUGAL BANGLADESH IRAN, ISLAMIC REPUBLIC OF QATAR BELARUS IRAQ ROMANIA BELGIUM IRELAND RUSSIAN FEDERATION BOLIVIA ISRAEL SAUDI ARABIA BRAZIL ITALY SENEGAL BULGARIA JAMAICA SIERRA LEONE CAMBODIA JAPAN SINGAPORE CAMEROON JORDAN SLOVENIA CANADA KENYA SOUTH AFRICA CHILE KOREA, REPUBLIC OF SPAIN CHINA KUWAIT SRI LANKA COLOMBIA LEBANON SUDAN COSTA RICA LIBERIA SWEDEN COTE D'lVOIRE LIBYAN ARAB JAMAHIRTYA SWITZERLAND CROATIA LIECHTENSTEIN SYRIAN ARAB REPUBLIC CUBA LUXEMBOURG THAILAND CYPRUS MADAGASCAR TUNISIA DEMOCRATIC PEOPLE'S MALAYSIA TURKEY REPUBLIC OF KOREA MALI UGANDA DENMARK MAURITIUS UKRAINE DOMINICAN REPUBLIC MEXICO UNITED ARAB EMIRATES ECUADOR MONACO UNITED KINGDOM OF GREAT EGYPT MONGOLIA BRITAIN AND NORTHERN EL SALVADOR MOROCCO IRELAND ESTONIA MYANMAR UNITED REPUBLIC OF TANZANIA ETHIOPIA NAMIBIA UNITED STATES OF AMERICA FINLAND NETHERLANDS URUGUAY FRANCE NEW ZEALAND VENEZUELA GABON NICARAGUA VIET NAM GERMANY NIGER YUGOSLAVIA GHANA NIGERIA ZAIRE GREECE NORWAY ZAMBIA GUATEMALA PAKISTAN ZIMBABWE The Agency's Statute was approved on 23 October 1956 by the Conference on the Statute of the IAEA held at United Nations Headquarters, New York; it entered into force on 29 July 1957. The Head- quarters of the.
    [Show full text]
  • Reactor Fuel Isotopics and Code Validation for Nuclear Applications
    ORNL/TM-2014/464 Reactor Fuel Isotopics and Code Validation for Nuclear Applications Matthew W. Francis Charles F. Weber Marco T. Pigni Approved for public release; Ian C. Gauld distribution is unlimited. September 2014 DOCUMENT AVAILABILITY Reports produced after January 1, 1996, are generally available free via US Department of Energy (DOE) SciTech Connect. Website http://www.osti.gov/scitech/ Reports produced before January 1, 1996, may be purchased by members of the public from the following source: National Technical Information Service 5285 Port Royal Road Springfield, VA 22161 Telephone 703-605-6000 (1-800-553-6847) TDD 703-487-4639 Fax 703-605-6900 E-mail [email protected] Website http://www.ntis.gov/help/ordermethods.aspx Reports are available to DOE employees, DOE contractors, Energy Technology Data Exchange representatives, and International Nuclear Information System representatives from the following source: Office of Scientific and Technical Information PO Box 62 Oak Ridge, TN 37831 Telephone 865-576-8401 Fax 865-576-5728 E-mail [email protected] Website http://www.osti.gov/contact.html This report was prepared as an account of work sponsored by an agency of the United States Government. Neither the United States Government nor any agency thereof, nor any of their employees, makes any warranty, express or implied, or assumes any legal liability or responsibility for the accuracy, completeness, or usefulness of any information, apparatus, product, or process disclosed, or represents that its use would not infringe privately owned rights. Reference herein to any specific commercial product, process, or service by trade name, trademark, manufacturer, or otherwise, does not necessarily constitute or imply its endorsement, recommendation, or favoring by the United States Government or any agency thereof.
    [Show full text]
  • Inventory of Radiological Methodologies for Sites
    A \ Inventory of Radiological Methodologies For Sites Contaminated with Radioactive Materials EPA 402-R-06-007 www.epa.gov October 2006 Inventory of Radiological Methodologies For Sites Contaminated With Radioactive Materials U.S. Environmental Protection Agency Office of Air and Radiation Office of Radiation and Indoor Air National Air and Radiation Environmental Laboratory Montgomery, AL 36115 Inventory of Radiological Methodologies This report was prepared for the National Air and Radiation Environmental Laboratory of the Office of Radiation and Indoor Air, United States Environmental Protection Agency. It was prepared by Environmental Management Support, Inc., of Silver Spring, Maryland, under contract 68-W-00-084, work assignment 46, and contract 68-W-03-038, work assignments 10 and 26, all managed by David Garman. Mention of trade names or specific applications does not imply endorsement or acceptance by EPA. For further information, contact Dr. John Griggs, U.S. EPA, Office of Radiation and Indoor Air, National Air and Radiation Environmental Laboratory, 540 South Morris Avenue, Montgomery, AL 36115-2601. Inventory of Radiological Methodologies Preface This compendium is part of a continuing effort by the Office of Radiation and Indoor Air and the Office of Superfund Remediation and Technology Innovation to provide guidance to engineers and scientists responsible for managing the cleanup of sites contaminated with radioactive materials. The document focuses on the radionuclides likely to be found in soil and water at cleanup sites contaminated with radioactive materials. However, its general principles apply also to other media that require analysis to support cleanup activities. It is not a complete catalog of analytical method­ ologies, but rather is intended to assist project managers in understanding the concepts, require­ ments, practices, and limitations of radioanalytical laboratory analyses of environmental samples.
    [Show full text]
  • Chapter 3 Radioactivity
    Nuclear Science—A Guide to the Nuclear Science Wall Chart ©2018 Contemporary Physics Education Project (CPEP) Chapter 3 Radioactivity In radioactive processes, particles or electromagnetic radiation are emitted from the nucleus. The most common forms of radiation emitted have been traditionally classified as alpha (a), beta (b), and gamma (g) radiation. Nuclear radiation occurs in other forms, including the emission of protons or neutrons or spontaneous fission of a massive nucleus. Of the nuclei found on Earth, the vast majority is stable. This is so because almost all short-lived radioactive nuclei have decayed during the history of the Earth. There are approximately 270 stable isotopes and 50 naturally occurring radioisotopes (radioactive isotopes). Thousands of other radioisotopes have been made in the laboratory. Fig. 3-1. The lower end of the Chart of the Nuclides. Radioactive decay will change one nucleus to another if the product nucleus has a greater nuclear binding energy than the initial decaying nucleus. The difference in binding energy (comparing the before and after states) determines which decays are 3-1 Chapter 3—Radioactivity energetically possible and which are not. The excess binding energy appears as kinetic energy or rest mass energy of the decay products. The Chart of the Nuclides, part of which is shown in Fig. 3-1, is a plot of nuclei as a function of proton number, Z, and neutron number, N. All stable nuclei and known radioactive nuclei, both naturally occurring and manmade, are shown on this chart, along with their decay properties. Nuclei with an excess of protons or neutrons in comparison with the stable nuclei will decay toward the stable nuclei by changing protons into neutrons or neutrons into protons, or else by shedding neutrons or protons either singly or in combination.
    [Show full text]
  • Inventory of Radiological Methodologies for Sites
    EPA 402-R-06-007 www.epa.gov October 2006 Inventory of Radiological Methodologies For Sites Contaminated With Radioactive Materials U.S. Environmental Protection Agency Office of Air and Radiation Office of Radiation and Indoor Air National Air and Radiation Environmental Laboratory Montgomery, AL 36115 Inventory of Radiological Methodologies This report was prepared for the National Air and Radiation Environmental Laboratory of the Office of Radiation and Indoor Air, United States Environmental Protection Agency. It was prepared by Environmental Management Support, Inc., of Silver Spring, Maryland, under contract 68-W-00-084, work assignment 46, and contract 68-W-03-038, work assignments 10 and 26, all managed by David Garman. Mention of trade names or specific applications does not imply endorsement or acceptance by EPA. For further information, contact Dr. John Griggs, U.S. EPA, Office of Radiation and Indoor Air, National Air and Radiation Environmental Laboratory, 540 South Morris Avenue, Montgomery, AL 36115-2601. Inventory of Radiological Methodologies Preface This compendium is part of a continuing effort by the Office of Radiation and Indoor Air and the Office of Superfund Remediation and Technology Innovation to provide guidance to engineers and scientists responsible for managing the cleanup of sites contaminated with radioactive materials. The document focuses on the radionuclides likely to be found in soil and water at cleanup sites contaminated with radioactive materials. However, its general principles apply also to other media that require analysis to support cleanup activities. It is not a complete catalog of analytical method­ ologies, but rather is intended to assist project managers in understanding the concepts, require­ ments, practices, and limitations of radioanalytical laboratory analyses of environmental samples.
    [Show full text]
  • Isotopes: Production and Application
    Isotopes: production and application Kornoukhov Vasily Nikolaevich [email protected] Lecture No1 Isotopes: Introduction & History of discovery Milestones of History of isotopes 1896 – Discovery of radioactivity by Henri Becquerel. Nobel prize of 1903 1898 - Discovery of Po-212 by P. Curie and M. Curie and Ra-226 by P. Curie and M. Curie and G. Bemont. 1910-1913 – Investigation of the properties of isotopes and origin. Introduction of the term “Isotope” by Frederick Soddy. Nobel prize of 1921. 1911 – The first direct observation of the stable isotopes (Ne-20 and Ne-22) in experiments with “canal (anode) rays” by Joseph John Thomson. Nobel prize of 1906. 1919 – Investigation of isotope phenomenon. The first mass-spectrometer by Francis Aston. He identified isotopes of Cl-35, -37, Br-79, -81, and Kr-78, -80, -82, -83, -84, -86. Nobel prize of 1922. 1934 – Discovery of artificial radioactivity. Production of P-30 as a very first “artificial” isotope by Irène and Jean Frédéric Joliot-Curie. 1934 –Enrico Fermi reported the discovery of neutron-induced radioactivity in the Italian journal La Ricerca Scientifica on 25 March 1934. Production of new radionuclides. 1936 - Emilio Segre discovered the very first artificial element Technetium Tc (in Greek - τεχνητός — “artificial”). 10.112020 Lecture No1 Isotopes: introduction V.N. Kornoukhov 2 Isotope: definition “ISOTOPES (from the Greek isos - equal, the same and topos - place), varieties of atoms of the same chemical element whose atomic nuclei have the same number of protons (Z) and different numbers of neutrons (N). (Isotopes are the nuclides of one element.) The nuclei of such atoms are also called isotopes.
    [Show full text]