1511327847Paper8 Energyenv

Total Page:16

File Type:pdf, Size:1020Kb

1511327847Paper8 Energyenv Paper No:7 Energy and Environment Module:18 Nuclear energy from fission Development Team Prof. R.K. Kohli Principal Investigator & Prof. V.K. Garg &Prof.AshokDhawan Co- Principal Investigator Central University of Punjab, Bathinda Dr. Dhanya M.S., Paper Coordinator Central University of Punjab, Bathinda Dr. Sandeep Kumar and Dr. S. Prasad Content Writer IARI, New Delhi & Dhanya M.S, Central University of Punjab, Bathinda Content Reviewer Prof. A.K Jain, Former Director, SSSNIRE 1 Anchor Institute Central University of Punjab Energy and Environment Environmental Sciences Nuclear energy from fission Description of Module Subject Name Environmental Sciences Paper Name Energy and Environment Module Name/Title Nuclear energy- fission Module Id EVS/EE-VIII/18 Pre-requisites This module helps to learn What is the principle of nuclear fission? How to control of nuclear fission? Energy release by nuclear fission Objectives Types of nuclear reactors Components of a nuclear power plant Advantages and disadvantages of nuclear power plants Nuclear power plants in India Keywords Nuclear fission, nuclear power plant, energy 2 Energy and Environment Environmental Sciences Nuclear energy from fission Learning Objectives What is the principle of nuclear fission? How to control of nuclear fission? Energy Release by Nuclear Fission Types of nuclear reactors Components Of a Nuclear Power Plant Advantages and disadvantages of nuclear power plants Nuclear power plants in India 1. Introduction The nuclear fission is one type of nuclear reaction or a radioactive decay process in which the nucleus of an atom splits into smaller nuclei along with release of huge amounts of energy. Fission is a form of nuclear transmutation with unsimilar resulting particles which differ from parent nuclei. The fission occurs in heavy nuclei after the capture of a neutron. The slow or thermal neutrons cause fission only in those isotopes of uranium (U) and plutonium (Pu) whose nuclei having odd numbers of neutrons (e.g. U-233, U-235, and Pu-239). The fission in nuclei with even number of neutrons occurs only when the incident neutrons have energy above around one million electron volts (MeV). The two nuclei products from common fissile isotopes are comparable differing in sizes with a mass ratio of products of nearly 3 to 2. The binary fissions that produce two charged particles are common but three positively charged particles (ternary fission) are also produced occasionally. The electricity produced by nuclear fission in a self-sustaining nuclear chain reaction that releases a significant amount of energy at a controlled rate in a nuclear reactor had wide energy potential. 3 Energy and Environment Environmental Sciences Nuclear energy from fission 1.1. Discovery of nuclear fission In 1917, Rutherford was able to perform transmutation of nitrogen into oxygen, using alpha particles directed at nitrogen 14N + α → 17O + p That was the first observation of a nuclear reaction, in which particles from one decay are used to transform another atomic nucleus. Finally, in 1932, a fully artificial nuclear reaction and nuclear transmutation were concluded by Rutherford's colleagues Ernest Walton and John Cockcroft, who applied artificially accelerated protons against lithium-7 (Li-7), to split this nucleus into two alpha particles. Fermi and his colleagues studied the results of bombarding uranium with neutrons in 1934. The nuclear fission of heavy elements was identified on December 17, 1938, by German Otto Hahn and his colleague Fritz Strassmann, and described theoretically in January 1939 by Lise Meitner and her nephew, Otto Robert Frisch. 3. Principle of nuclear fission Nuclear fission occurs when a neutron hits with a nucleus of a large atom such as U and is absorbed into it causing the nucleus to become unstable and thus break down into two smaller and more stable atoms with the release of more neutrons and an enormous amount of energy. Nuclear fission can happen naturally with the spontaneous decay of radioactive material, or it can be induced by bombarding the fuel consisting of fissionable atoms with neutrons (Fig. 1). 4 Energy and Environment Environmental Sciences Nuclear energy from fission Fig 1: Nuclear fission process a) Fission Energy Release The fission of naturally occurring U isotope induced by thermal neutrons is U-235 which splits into Ba-141 and Kr-92 and emits excess free neutrons. When nucleus fission occurs, it breaks into several smaller fragments with release of two or three neutrons. The sum of the masses of fission products is less than the original mass. On an average near about 0.1% of the original mass has been transformed into energy according to Einstein's equation. And that reduction in mass comes off in the form of energy according to the Einstein equation E = mc2. The fission of U-235 in nuclear reactors is triggered by the absorption of a low energy neutron, usually termed a "slow neutron" or a "thermal neutron." Other fissionable isotopes which can be induced to fission by slow neutrons are Pu-239, U-233, and Th-232. 5 Energy and Environment Environmental Sciences Nuclear energy from fission 1.2. Fissionable isotopes The nuclear fission reactions start when isotopes are hit by either high energy (fast moving) neutrons or thermal (slow-moving) neutrons at the optimum speed. For examples, U-235 and Pu-239 are fissionable isotopes. U-235 is the naturally occurring fissionable isotope, and Pu-239 can be produced by "breeding" from U-238. U-238 and Th-232 are the chief naturally occurring fertile isotopes. U-238, which makes up 99.3% of natural uranium, is not fissionable by slow neutrons. U-238 has a little probability for spontaneous fission and also a small chance of fission when bombarded with fast neutrons. However, it is not useful as a nuclear fuel source. Th-232 is fissionable, so could conceivably be employed as a nuclear fuel. The other isotope of natural thorium which is known to undergo fission upon slow neutron bombardment is U-233. Pu-241 and Pu-241 are fissile materials. The isotopes as mentioned earlier can be created artificially in a nuclear reactor, from the fertile nuclei of Th-232, U-238, and Pu-240. U-235 is only naturally found isotope which is thermally fissile, and present in natural uranium at a concentration of 0.7%. 1.3. Principle of Nuclear Fission When U-235 or fissionable isotopes capture a neutron, the total energy is distributed amongst the nucleons (protons & neutrons) present in the compound nucleus. These nucleuses are relatively unstable, and it is likely to break into two fragments of near about half of the mass. Production of these fission fragments is followed almost immediately by the emission of some neutrons (commonly 2 or 3, average 2.45), which facilitate the chain reaction to be sustained (Fig. 3). 6 Energy and Environment Environmental Sciences Nuclear energy from fission Fig. 2: Energy path during fission About 85% of the energy released is initially the kinetic energy of the fission fragments (Fig. 2). The balance of the power comes from gamma rays emitted during or quickly following the fission process and from the kinetic energy of the neutrons. The immediate neutrons are called prompt neutrons, and there is a small portion of delayed neutrons, as these are linkedwith the radioactive decay of certain fission products. The highest delayed neutron group has a half-life of nearly 56 seconds. Fig. 3: Nuclear fission chain reaction 7 Energy and Environment Environmental Sciences Nuclear energy from fission The number of neutrons and the particular fission products from any fission case are guided by statistical probability, in that the precise break up of a single nucleus cannot be predicted. Nonetheless, conservation laws require the total number of nucleons and the total energy to be conserved during the reaction. The fission reaction in U-235 creates fission products like Ba, Kr, Sr, Cs, I and Xe with atomic masses distributed nearly 95 and 135. The following reactions are representing typical fissionable products: U-235 + n Ba-144 + Kr-90 + 2n + 200 MeV U-235 + n Ba-141 + Kr-92 + 3n + 170 MeV U-235 + n Zr-94 + Te-139 + 3n + 197 MeV In above reactions, the number of nucleons (protons + neutrons) is balanced. The total binding energy released in nuclear fission reaction of an atomic nucleus varies with the precise break up (near about 200 MeV for U-235). Near about 6% of the heat produced in the reactor core originates from radioactive decay of fission products and transuranic elements composed by neutron capture. That must be allowed for when the reactor is shut down since heat generation continues after fission stops. Even after one year, commonly used fuel generates about 10 kW of decay heat per ton, decreasing to about 1 kW per ton after ten years. 1.4. Nuclear Chain Reactions Nuclear chain reactions are series of nuclear fissions, each reaction initiated by a neutron produced in a preceding fission. This process may be controlled (nuclear power) or uncontrolled (nuclear weapons). If each neutron releases two more neutrons, then the number of fissions doubles each generation. In that case, in 10 generations there is 1,024 fission and in 80 generations about 6 x 10 23 (a mole) fissions (Fig. 4). The energy released from the kinetic energy of each fission reaction is nearly 200 MeV, which includes,165 MeV from fission, 6 MeV from neutrons. 7 MeV from gamma rays, 7 MeV from energy from fission products, 6 MeV from gamma rays and 9 MeV from anti-neutrinos from fission products (1 MeV = 1.609 x 10 -13 joules). 8 Energy and Environment Environmental Sciences Nuclear energy from fission Fig 4:Nuclear Chain Reactions 1.4.1. Critical Mass (K) Although two to three neutrons are created for every fission, not all of these neutrons are available for continuing the fission reaction.
Recommended publications
  • Nuclear Energy: Fission and Fusion
    CHAPTER 5 NUCLEAR ENERGY: FISSION AND FUSION Many of the technologies that will help us to meet the new air quality standards in America can also help to address climate change. President Bill Clinton 1 Two distinct processes involving the nuclei of atoms can be harnessed, in principle, for energy production: fission—the splitting of a nucleus—and fusion—the joining together of two nuclei. For any given mass or volume of fuel, nuclear processes generate more energy than can be produced through any other fuel-based approach. Another attractive feature of these energy-producing reactions is that they do not produce greenhouse gases (GHG) or other forms of air pollution directly. In the case of nuclear fission—a mature though controversial energy technology—electricity is generated from the energy released when heavy nuclei break apart. In the case of nuclear fusion, much work remains in the quest to sustain the fusion reactions and then to design and build practical fusion power plants. Fusion’s fuel is abundant, namely, light atoms such as the isotopes of hydrogen, and essentially limitless. The most optimistic timetable for fusion development is half a century, because of the extraordinary scientific and engineering challenges involved, but fusion’s benefits are so globally attractive that fusion R&D is an important component of today’s energy R&D portfolio internationally. Fission power currently provides about 17 percent of the world’s electric power. As of December 1996, 442 nuclear power reactors were operating in 30 countries, and 36 more plants were under construction. If fossil plants were used to produce the amount of electricity generated by these nuclear plants, more than an additional 300 million metric tons of carbon would be emitted each year.
    [Show full text]
  • Ternary Fission and Quasi-Fission of Superheavy Nuclei and Giant Nuclear Systems
    June 17, 2010 18:24 Proceedings Trim Size: 9in x 6in zagrebaev_¯ssion_2010b TERNARY FISSION AND QUASI-FISSION OF SUPERHEAVY NUCLEI AND GIANT NUCLEAR SYSTEMS V.I. ZAGREBAEV, A.V. KARPOV Flerov Laboratory of Nuclear Reactions, JINR, Dubna, Moscow Region, Russia WALTER GREINER Frankfurt Institute for Advanced Studies, J.W. Goethe-UniversitÄat,Germany We found that a true ternary ¯ssion with formation of a heavy third fragment (a new kind of radioactivity) is quite possible for superheavy nuclei due to the strong shell e®ects leading to a three-body clusterization with the two doubly magic tin- like cores. The three-body quasi-¯ssion process could be even more pronounced for giant nuclear systems formed in collisions of heavy actinide nuclei. In this case a three-body clusterization might be proved experimentally by detection of two coincident lead-like fragments in low-energy U+U collisions. 1. Introduction Today the term \ternary ¯ssion" is commonly used to denote the process of formation of light charged particle accompanied ¯ssion 1. This is a rare process (less than 1%) relative to binary ¯ssion, see Fig. 1. As can be seen the probability of such a process decreases sharply with increasing mass number of the accompanied third particle. These light particles are emitted almost perpendicularly with respect to the ¯ssion axis (equatorial emission) 1. It is interpreted as an indication that the light ternary particles are emitted from the neck region and are accelerated by the Coulomb ¯elds of both heavy fragments. In contrast to such a process, the term \true ternary ¯ssion" is used for a simultaneous decay of a heavy nucleus into three fragments of not very di®erent mass 1.
    [Show full text]
  • NETS 2020 Template
    بÀƵƧǘȁǞƧƊǶ §ȲȌǐȲƊǿ ƊƧDzɈȌɈǘƵwȌȌȁƊȁƮȌȁ ɈȌwƊȲȺɈǘȲȌɐǐǘƊƮɨƊȁƧǞȁǐ خȁɐƧǶƵƊȲɈƵƧǘȁȌǶȌǐǞƵȺƊȁƮ ǞȁȁȌɨƊɈǞȌȁ ǞȺ ȺȯȌȁȺȌȲƵƮ Ʀɯ ɈǘƵ ƊDz ªǞƮǐƵ yƊɈǞȌȁƊǶ ׁׂ׀ׂ y0À² ÀǘǞȺ ƧȌȁǏƵȲƵȁƧƵ خׁׂ׀ׂ ةɈǘ׀׃ƊȁƮ ɩǞǶǶƦƵ ǘƵǶƮ ǏȲȌǿȯȲǞǶ ׂ׆ɈǘٌةmƊƦȌȲƊɈȌȲɯ ɩǞǶǶ ƦƵ ǘƵǶƮ ɨǞȲɈɐƊǶǶɯ ȺȌ ɈǘƊɈ ɈǘƵ ƵȁɈǞȲƵ y0À² خƧȌǿǿɐȁǞɈɯǿƊɯȯƊȲɈǞƧǞȯƊɈƵǞȁɈǘǞȺƵɮƧǞɈǞȁǐǿƵƵɈǞȁǐ ǐȌɨخȌȲȁǶخخׁׂ׀ȁƵɈȺׂششبǘɈɈȯȺ Nuclear and Emerging Technologies for Space Sponsored by Oak Ridge National Laboratory, April 26th-30th, 2021. Available online at https://nets2021.ornl.gov Table of Contents Table of Contents .................................................................................................................................................... 1 Thanks to the NETS2021 Sponsors! ...................................................................................................................... 2 Nuclear and Emerging Technologies for Space 2021 – Schedule at a Glance ................................................. 3 Nuclear and Emerging Technologies for Space 2021 – Technical Sessions and Panels By Track ............... 6 Nuclear and Emerging Technologies for Space 2021 – Lightning Talk Final Program ................................... 8 Nuclear and Emerging Technologies for Space 2021 – Track 1 Final Program ............................................. 11 Nuclear and Emerging Technologies for Space 2021 – Track 2 Final Program ............................................. 14 Nuclear and Emerging Technologies for Space 2021 – Track 3 Final Program ............................................. 18
    [Show full text]
  • Compilation and Evaluation of Fission Yield Nuclear Data Iaea, Vienna, 2000 Iaea-Tecdoc-1168 Issn 1011–4289
    IAEA-TECDOC-1168 Compilation and evaluation of fission yield nuclear data Final report of a co-ordinated research project 1991–1996 December 2000 The originating Section of this publication in the IAEA was: Nuclear Data Section International Atomic Energy Agency Wagramer Strasse 5 P.O. Box 100 A-1400 Vienna, Austria COMPILATION AND EVALUATION OF FISSION YIELD NUCLEAR DATA IAEA, VIENNA, 2000 IAEA-TECDOC-1168 ISSN 1011–4289 © IAEA, 2000 Printed by the IAEA in Austria December 2000 FOREWORD Fission product yields are required at several stages of the nuclear fuel cycle and are therefore included in all large international data files for reactor calculations and related applications. Such files are maintained and disseminated by the Nuclear Data Section of the IAEA as a member of an international data centres network. Users of these data are from the fields of reactor design and operation, waste management and nuclear materials safeguards, all of which are essential parts of the IAEA programme. In the 1980s, the number of measured fission yields increased so drastically that the manpower available for evaluating them to meet specific user needs was insufficient. To cope with this task, it was concluded in several meetings on fission product nuclear data, some of them convened by the IAEA, that international co-operation was required, and an IAEA co-ordinated research project (CRP) was recommended. This recommendation was endorsed by the International Nuclear Data Committee, an advisory body for the nuclear data programme of the IAEA. As a consequence, the CRP on the Compilation and Evaluation of Fission Yield Nuclear Data was initiated in 1991, after its scope, objectives and tasks had been defined by a preparatory meeting.
    [Show full text]
  • Uranium (Nuclear)
    Uranium (Nuclear) Uranium at a Glance, 2016 Classification: Major Uses: What Is Uranium? nonrenewable electricity Uranium is a naturally occurring radioactive element, that is very hard U.S. Energy Consumption: U.S. Energy Production: and heavy and is classified as a metal. It is also one of the few elements 8.427 Q 8.427 Q that is easily fissioned. It is the fuel used by nuclear power plants. 8.65% 10.01% Uranium was formed when the Earth was created and is found in rocks all over the world. Rocks that contain a lot of uranium are called uranium Lighter Atom Splits Element ore, or pitch-blende. Uranium, although abundant, is a nonrenewable energy source. Neutron Uranium Three isotopes of uranium are found in nature, uranium-234, 235 + Energy FISSION Neutron uranium-235, and uranium-238. These numbers refer to the number of Neutron neutrons and protons in each atom. Uranium-235 is the form commonly Lighter used for energy production because, unlike the other isotopes, the Element nucleus splits easily when bombarded by a neutron. During fission, the uranium-235 atom absorbs a bombarding neutron, causing its nucleus to split apart into two atoms of lighter mass. The first nuclear power plant came online in Shippingport, PA in 1957. At the same time, the fission reaction releases thermal and radiant Since then, the industry has experienced dramatic shifts in fortune. energy, as well as releasing more neutrons. The newly released neutrons Through the mid 1960s, government and industry experimented with go on to bombard other uranium atoms, and the process repeats itself demonstration and small commercial plants.
    [Show full text]
  • 1 Phys:1200 Lecture 36 — Atomic and Nuclear Physics
    1 PHYS:1200 LECTURE 36 — ATOMIC AND NUCLEAR PHYSICS (4) This last lecture of the course will focus on nuclear energy. There is an enormous reservoir of energy in the nucleus and it can be released either in a controlled manner in a nuclear reactor, or in an uncontrolled manner in a nuclear bomb. The energy released in a nuclear reactor can be used to produce electricity. The two processes in which nuclear energy is released – nuclear fission and nuclear fusion, will be discussed in this lecture. The biological effects of nuclear radiation will also be discussed. 36‐1. Biological Effects of Nuclear Radiation.—Radioactive nuclei emit alpha, beta, and gamma radiation. These radiations are harmful to humans because they are ionizing radiation that have the ability to remove electrons from atoms and molecules in human cells. This can lead to the death or alterations of cells. Alteration of the cell can transform a healthy cell into a cancer cell. The hazards of radiation can be minimized by limiting ones overall exposure to radiation. However, there is still some uncertainty in the medical community about the possibility the effect of a single radioactive particle on the bottom. In other words, are the effects cumulative, or can a single exposure lead to cancer in the body. Exposure to radiation can produce either short term effects appearing within minutes of exposure, or long term effects that may appear in years or decades or even in future generations due to changes in DNA. The effects of absorbing ionizing radiation is measured in a unit called the rem.
    [Show full text]
  • 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.
    [Show full text]
  • 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.
    [Show full text]
  • Properties of Selected Radioisotopes
    CASE FILE COPY NASA SP-7031 Properties of Selected Radioisotopes A Bibliography PART I: UNCLASSIFIED LITERATURE NATIONAL AERONAUTICS AND SPACE ADMINISTRATION NASA SP-7031 PROPERTIES OF SELECTED RADIOISOTOPES A Bibliography Part I: Unclassified Literature A selection of annotated references to technical papers, journal articles, and books This bibliography was compiled and edited by DALE HARRIS and JOSEPH EPSTEIN Goddard Space Flight Center Greenbelt, Maryland Scientific and Technical Information Division / OFFICE OF TECHNOLOGY UTILIZATION 1968 USP. NATIONAL AERONAUTICS AND SPACE ADMINISTRATION Washington, D.C. PREFACE The increasing interest in the application of substantial quantities of radioisotopes for propulsion, energy conversion, and various other thermal concepts emphasizes a need for the most recent and most accurate information available describing the nuclear, chemical, and physical properties of these isotopes. A substantial amount of progress has been achieved in recent years in refining old and developing new techniques of measurement of the properties quoted, and isotope processing. This has resulted in a broad technological base from which both the material and information about the material is available. Un- fortunately, it has also resulted in a multiplicity of sources so that information and data are either untimely or present properties without adequately identifying the measurement techniques or describing the quality of material used. The purpose of this document is to make available, in a single reference, an annotated bibliography and sets of properties for nine of the more attractive isotopes available for use in power production. Part I contains all the unclassified information that was available in the literature surveyed. Part II is the classified counterpart to Part I.
    [Show full text]
  • Fission and Fusion Can Yield Energy
    Nuclear Energy Nuclear energy can also be separated into 2 separate forms: nuclear fission and nuclear fusion. Nuclear fusion is the splitting of large atomic nuclei into smaller elements releasing energy, and nuclear fusion is the joining of two small atomic nuclei into a larger element and in the process releasing energy. The mass of a nucleus is always less than the sum of the individual masses of the protons and neutrons which constitute it. The difference is a measure of the nuclear binding energy which holds the nucleus together (Figure 1). As figures 1 and 2 below show, the energy yield from nuclear fusion is much greater than nuclear fission. Figure 1 2 Nuclear binding energy = ∆mc For the alpha particle ∆m= 0.0304 u which gives a binding energy of 28.3 MeV. (Figure from: http://hyperphysics.phy-astr.gsu.edu/hbase/nucene/nucbin.html ) Fission and fusion can yield energy Figure 2 (Figure from: http://hyperphysics.phy-astr.gsu.edu/hbase/nucene/nucbin.html) Nuclear fission When a neutron is fired at a uranium-235 nucleus, the nucleus captures the neutron. It then splits into two lighter elements and throws off two or three new neutrons (the number of ejected neutrons depends on how the U-235 atom happens to split). The two new atoms then emit gamma radiation as they settle into their new states. (John R. Huizenga, "Nuclear fission", in AccessScience@McGraw-Hill, http://proxy.library.upenn.edu:3725) There are three things about this induced fission process that make it especially interesting: 1) The probability of a U-235 atom capturing a neutron as it passes by is fairly high.
    [Show full text]
  • Etude Des Évolutions Microstructurales Sous Irradiation De L’Alliage D’Aluminium 6061-T6
    THÈSE Pour obtenir le grade de DOCTEUR DE L’UNIVERSITÉ GRENOBLE ALPES Spécialité : Matériaux, Mécanique, Génie Civil, Electrochimie (2MGE) Arrêté ministériel : 7 août 2006 Présentée par Camille FLAMENT Thèse dirigée par Alexis DESCHAMPS et codirigée par Jérôme GARNIER et Joël RIBIS préparée au sein du Laboratoire d’étude du Comportement Mécanique des Matériaux (CEA) dans l'École Doctorale Ingénierie, Matériaux, Mécanique, Energétique, Environnement, Procédés, Production (I-MEP2) Etude des évolutions microstructurales sous irradiation de l’alliage d’aluminium 6061-T6 Thèse soutenue publiquement le 01 décembre 2015, devant le jury composé de : M. Alexis DESCHAMPS Professeur à l’INP de Grenoble, Directeur Mme. Myriam DUMONT Maître de conférences à l’Université Aix-Marseille, Rapporteur M. Thierry EPICIER Directeur de recherche au CNRS, Président M. Jérôme GARNIER Ingénieur de recherche au CEA, Co-encadrant M. Alexandre LEGRIS Professeur à l’Université Lille 1, Rapporteur M. Joël RIBIS Ingénieur de recherche au CEA, Co-encadrant REMERCIEMENTS Remerciements Cette thèse a été réalisée au Service de Recherches Métallurgiques Appliquées (SRMA) du Département des Matériaux pour le Nucléaire du CEA Saclay (DMN). Je souhaite donc tout d’abord remercier Messieurs Philippe Chapelot et Pascal Yvon de m’avoir accueillie respectivement au SRMA et DMN. Je remercie également Madame Laetitia Nicolas, ex-chef du Laboratoire d’étude du Comportement Mécanique des Matériaux qui fut mon laboratoire de rattachement et Monsieur Jean- Luc Béchade, ex-chef du Laboratoire d’Analyse Microstructurale des Matériaux (dorénavant chef du Service de Recherche de Métallurgie Physique) au sein duquel j’ai pu m’installer et utiliser les différents outils de caractérisation.
    [Show full text]
  • An Overview of the HIT-SI Research Program and Its Implications for Magnetic Fusion Energy
    An overview of the HIT-SI research program and its implications for magnetic fusion energy Derek Sutherland, Tom Jarboe, and The HIT-SI Research Group University of Washington 36th Annual Fusion Power Associates Meeting – Strategies to Fusion Power December 16-17, 2015, Washington, D.C. Motivation • Spheromaks configurations are attractive for fusion power applications. • Previous spheromak experiments relied on coaxial helicity injection, which precluded good confinement during sustainment. • Fully inductive, non-axisymmetric helicity injection may allow us to overcome the limitations of past spheromak experiments. • Promising experimental results and an attractive reactor vision motivate continued exploration of this possible path to fusion power. Outline • Coaxial helicity injection NSTX and SSPX • Overview of the HIT-SI experiment • Motivating experimental results • Leading theoretical explanation • Reactor vision and comparisons • Conclusions and next steps Coaxial helicity injection (CHI) has been used successfully on NSTX to aid in non-inductive startup Figures: Raman, R., et al., Nucl. Fusion 53 (2013) 073017 • Reducing the need for inductive flux swing in an ST is important due to central solenoid flux-swing limitations. • Biasing the lower divertor plates with ambient magnetic field from coil sets in NSTX allows for the injection of magnetic helicity. • A ST plasma configuration is formed via CHI that is then augmented with other current drive methods to reach desired operating point, reducing or eliminating the need for a central solenoid. • Demonstrated on HIT-II at the University of Washington and successfully scaled to NSTX. Though CHI is useful on startup in NSTX, Cowling’s theorem removes the possibility of a steady-state, axisymmetric dynamo of interest for reactor applications • Cowling* argued that it is impossible to have a steady-state axisymmetric MHD dynamo (sustain current on magnetic axis against resistive dissipation).
    [Show full text]