The Physics of Nuclear Weapons
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Glossary Physics (I-Introduction)
1 Glossary Physics (I-introduction) - Efficiency: The percent of the work put into a machine that is converted into useful work output; = work done / energy used [-]. = eta In machines: The work output of any machine cannot exceed the work input (<=100%); in an ideal machine, where no energy is transformed into heat: work(input) = work(output), =100%. Energy: The property of a system that enables it to do work. Conservation o. E.: Energy cannot be created or destroyed; it may be transformed from one form into another, but the total amount of energy never changes. Equilibrium: The state of an object when not acted upon by a net force or net torque; an object in equilibrium may be at rest or moving at uniform velocity - not accelerating. Mechanical E.: The state of an object or system of objects for which any impressed forces cancels to zero and no acceleration occurs. Dynamic E.: Object is moving without experiencing acceleration. Static E.: Object is at rest.F Force: The influence that can cause an object to be accelerated or retarded; is always in the direction of the net force, hence a vector quantity; the four elementary forces are: Electromagnetic F.: Is an attraction or repulsion G, gravit. const.6.672E-11[Nm2/kg2] between electric charges: d, distance [m] 2 2 2 2 F = 1/(40) (q1q2/d ) [(CC/m )(Nm /C )] = [N] m,M, mass [kg] Gravitational F.: Is a mutual attraction between all masses: q, charge [As] [C] 2 2 2 2 F = GmM/d [Nm /kg kg 1/m ] = [N] 0, dielectric constant Strong F.: (nuclear force) Acts within the nuclei of atoms: 8.854E-12 [C2/Nm2] [F/m] 2 2 2 2 2 F = 1/(40) (e /d ) [(CC/m )(Nm /C )] = [N] , 3.14 [-] Weak F.: Manifests itself in special reactions among elementary e, 1.60210 E-19 [As] [C] particles, such as the reaction that occur in radioactive decay. -
2012 04 Newsletter
United States Atmospheric & Underwater Atomic Weapon Activities National Association of Atomic Veterans, Inc. 1945 “TRINITY“ “Assisting America’s Atomic Veterans Since 1979” ALAMOGORDO, N. M. Website: www.naav.com E-mail: [email protected] 1945 “LITTLE BOY“ HIROSHIMA, JAPAN R. J. RITTER - Editor April, 2012 1945 “FAT MAN“ NAGASAKI, JAPAN 1946 “CROSSROADS“ BIKINI ISLAND 1948 “SANDSTONE“ ENEWETAK ATOLL 1951 “RANGER“ NEVADA TEST SITE 1951 “GREENHOUSE“ ENEWETAK ATOLL 1951 “BUSTER – JANGLE“ NEVADA TEST SITE 1952 “TUMBLER - SNAPPER“ NEVADA TEST SITE 1952 “IVY“ ENEWETAK ATOLL 1953 “UPSHOT - KNOTHOLE“ NEVADA TEST SITE 1954 “CASTLE“ BIKINI ISLAND 1955 “TEAPOT“ NEVADA TEST SITE 1955 “WIGWAM“ OFFSHORE SAN DIEGO 1955 “PROJECT 56“ NEVADA TEST SITE 1956 “REDWING“ ENEWETAK & BIKINI 1957 “PLUMBOB“ NEVADA TEST SITE 1958 “HARDTACK-I“ ENEWETAK & BIKINI 1958 “NEWSREEL“ JOHNSTON ISLAND 1958 “ARGUS“ SOUTH ATLANTIC 1958 “HARDTACK-II“ NEVADA TEST SITE 1961 “NOUGAT“ NEVADA TEST SITE 1962 “DOMINIC-I“ CHRISTMAS ISLAND JOHNSTON ISLAND 1965 “FLINTLOCK“ AMCHITKA, ALASKA 1969 “MANDREL“ AMCHITKA, ALASKA 1971 “GROMMET“ AMCHITKA, ALASKA 1974 “POST TEST EVENTS“ ENEWETAK CLEANUP ------------ “ IF YOU WERE THERE, YOU ARE AN ATOMIC VETERAN “ The Newsletter for America’s Atomic Veterans COMMANDER’S COMMENTS knowing the seriousness of the situation, did not register any Outreach Update: First, let me extend our discomfort, or dissatisfaction on her part. As a matter of fact, it thanks to the membership and friends of NAAV was kind of nice to have some of those callers express their for supporting our “outreach” efforts over the thanks for her kind attention and assistance. We will continue past several years. It is that firm dedication to to insure that all inquires, along these lines, are fully and our Mission-Statement that has driven our adequately addressed. -
A Simple Approach to the Supernova Progenitor-Explosion Connection
A Simple Approach to the Supernova Progenitor-Explosion Connection Bernhard Müller Queen's University Belfast Monash Alexander Heger, David Liptai, Joshua Cameron (Monash University) Many potential/indirect observables from core-collapse supernovae, but some of the most direct ones (explosion energies, remnant masses) are heavy elements challenging for SN theory! massive star core-collapse supernovae neutron stars & gravitational waves neutrinos supernova remnants The neutrino-driven mechanism in its modern flavour shock ● Stalled accretion shock still oscillations (“SASI”) pushed outward to ~150km as matter piles up on the PNS, then recedes again convection ● Heating or gain region g develops some tens of ms n i t g a n after bounce e li h o o c ● Convective overturn & shock oscillations “SASI” enhance the efficiency of -heating, shock which finally revives the shock ● Big challenge: Show that this works! Status of 3D Neutrino Hydrodynamics Models with Multi-Group Transport First-principle 3D models: ● Mixed record, some failures ● Some explosions, delayed compared to 2D ● Models close to the threshold So what is missing? 27 M Hanke et al. (2013) 2 3/5 2 −3/5 ⊙ ● Lcrit ∝M˙ M 14 Ma /3 ● → Increase neutrino heating or Reynolds stresses ● Unknown/undetermined microphysics (e.g. Melson et al. 2015)? ● 20 M Melson et al. (2015) Lower explosion threshold in ⊙ SASI-dominated regime (Fernandez 2015)? 15 M⊙ Lentz et al. (2015) ● Better 1D/multi-D progenitor Or with simpler schemes: e.g. IDSA+leakage Takiwaki et al. (2014) models? Challenge: Connecting to Observables Several 50 diagnostic 10 erg with explosion sustained energy accretion . l a ) t 2 e 1 a 0 k 2 ( n Pejcha & Prieto (2015): Explosion energies a J vs. -
Report: the New Nuclear Arms Race
The New Nuclear Arms Race The Outlook for Avoiding Catastrophe August 2020 By Akshai Vikram Akshai Vikram is the Roger L. Hale Fellow at Ploughshares Fund, where he focuses on U.S. nuclear policy. A native of Louisville, Kentucky, Akshai previously worked as an opposition researcher for the Democratic National Committee and a campaign staffer for the Kentucky Democratic Party. He has written on U.S. nuclear policy and U.S.-Iran relations for outlets such as Inkstick Media, The National Interest, Defense One, and the Quincy Institute’s Responsible Statecraft. Akshai holds an M.A. in International Economics and American Foreign Policy from the Johns Hopkins University SAIS as well as a B.A. in International Studies and Political Science from Johns Hopkins Baltimore. On a good day, he speaks Spanish, French, and Persian proficiently. Acknowledgements This report was made possible by the strong support I received from the entire Ploughshares Fund network throughout my fellowship. Ploughshares Fund alumni Will Saetren, Geoff Wilson, and Catherine Killough were extremely kind in offering early advice on the report. From the Washington, D.C. office, Mary Kaszynski and Zack Brown offered many helpful edits and suggestions, while Joe Cirincione, Michelle Dover, and John Carl Baker provided much- needed encouragement and support throughout the process. From the San Francisco office, Will Lowry, Derek Zender, and Delfin Vigil were The New Nuclear Arms Race instrumental in finalizing this report. I would like to thank each and every one of them for their help. I would especially like to thank Tom Collina. Tom reviewed numerous drafts of this report, never The Outlook for Avoiding running out of patience or constructive advice. -
Table 2.Iii.1. Fissionable Isotopes1
FISSIONABLE ISOTOPES Charles P. Blair Last revised: 2012 “While several isotopes are theoretically fissionable, RANNSAD defines fissionable isotopes as either uranium-233 or 235; plutonium 238, 239, 240, 241, or 242, or Americium-241. See, Ackerman, Asal, Bale, Blair and Rethemeyer, Anatomizing Radiological and Nuclear Non-State Adversaries: Identifying the Adversary, p. 99-101, footnote #10, TABLE 2.III.1. FISSIONABLE ISOTOPES1 Isotope Availability Possible Fission Bare Critical Weapon-types mass2 Uranium-233 MEDIUM: DOE reportedly stores Gun-type or implosion-type 15 kg more than one metric ton of U- 233.3 Uranium-235 HIGH: As of 2007, 1700 metric Gun-type or implosion-type 50 kg tons of HEU existed globally, in both civilian and military stocks.4 Plutonium- HIGH: A separated global stock of Implosion 10 kg 238 plutonium, both civilian and military, of over 500 tons.5 Implosion 10 kg Plutonium- Produced in military and civilian 239 reactor fuels. Typically, reactor Plutonium- grade plutonium (RGP) consists Implosion 40 kg 240 of roughly 60 percent plutonium- Plutonium- 239, 25 percent plutonium-240, Implosion 10-13 kg nine percent plutonium-241, five 241 percent plutonium-242 and one Plutonium- percent plutonium-2386 (these Implosion 89 -100 kg 242 percentages are influenced by how long the fuel is irradiated in the reactor).7 1 This table is drawn, in part, from Charles P. Blair, “Jihadists and Nuclear Weapons,” in Gary A. Ackerman and Jeremy Tamsett, ed., Jihadists and Weapons of Mass Destruction: A Growing Threat (New York: Taylor and Francis, 2009), pp. 196-197. See also, David Albright N 2 “Bare critical mass” refers to the absence of an initiator or a reflector. -
An Introduction to Isotopic Calculations John M
An Introduction to Isotopic Calculations John M. Hayes ([email protected]) Woods Hole Oceanographic Institution, Woods Hole, MA 02543, USA, 30 September 2004 Abstract. These notes provide an introduction to: termed isotope effects. As a result of such effects, the • Methods for the expression of isotopic abundances, natural abundances of the stable isotopes of practically • Isotopic mass balances, and all elements involved in low-temperature geochemical • Isotope effects and their consequences in open and (< 200°C) and biological processes are not precisely con- closed systems. stant. Taking carbon as an example, the range of interest is roughly 0.00998 ≤ 13F ≤ 0.01121. Within that range, Notation. Absolute abundances of isotopes are com- differences as small as 0.00001 can provide information monly reported in terms of atom percent. For example, about the source of the carbon and about processes in 13 13 12 13 atom percent C = [ C/( C + C)]100 (1) which the carbon has participated. A closely related term is the fractional abundance The delta notation. Because the interesting isotopic 13 13 fractional abundance of C ≡ F differences between natural samples usually occur at and 13F = 13C/(12C + 13C) (2) beyond the third significant figure of the isotope ratio, it has become conventional to express isotopic abundances These variables deserve attention because they provide using a differential notation. To provide a concrete the only basis for perfectly accurate mass balances. example, it is far easier to say – and to remember – that Isotope ratios are also measures of the absolute abun- the isotope ratios of samples A and B differ by one part dance of isotopes; they are usually arranged so that the per thousand than to say that sample A has 0.3663 %15N more abundant isotope appears in the denominator and sample B has 0.3659 %15N. -
Nonproliferation and Nuclear Forensics: Detailed, Multi- Analytical Investigation of Trinitite Post-Detonation Materials
SIMONETTI ET AL. CHAPTER 14: NONPROLIFERATION AND NUCLEAR FORENSICS: DETAILED, MULTI- ANALYTICAL INVESTIGATION OF TRINITITE POST-DETONATION MATERIALS Antonio Simonetti, Jeremy J. Bellucci, Christine Wallace, Elizabeth Koeman, and Peter C. Burns, Department of Civil and Environmental Engineering and Earth Sciences, University of Notre Dame, Notre Dame, Indiana, 46544, USA e-mail: [email protected] INTRODUCTION (and ≤7% 240Pu), whereas it is termed “reactor fuel In 2010, the Joint Working Group of the grade” if the material consists >8% 240Pu. American Physical Society and the American Production of enriched U is costly and an energy- Association for the Advancement of Science defined intensive process, and the most widely used Nuclear Forensics as “the technical means by which processes are gaseous diffusion of UF6 (employed nuclear materials, whether intercepted intact or by the United States and France) and high- retrieved from post-explosion debris, are performance centrifugation of UF6 (e.g., Russia, characterized (as to composition, physical condition, Europe, and South Africa). The uranium processed age, provenance, history) and interpreted (as to under the “Manhattan Project” and used within the provenance, industrial history, and implications for device detonated over Hiroshima was produced by nuclear device design).” Detailed investigation of electromagnetic separation; the latter process was post-detonation material (PDM) is critical in ultimately abandoned in the late 1940s because of preventing and/or responding to nuclear-based its significant energy demands. The minimum terrorist activities/threats. However, accurate amount of fissionable material required for a nuclear identification of nuclear device components within reaction is termed its “critical mass”, and the value PDM typically requires a variety of instrumental depends on the isotope employed, properties of approaches and sample characterization strategies; materials, local environment, and weapon design the latter may include radiochemical separations, (Moody et al. -
Images of Nuclear Energy: Why People Feel the Way They Do Emotions and Ideas Are More Deeply Rooted Than Realized
SPECIAL REPORT Images of nuclear energy: Why people feel the way they do Emotions and ideas are more deeply rooted than realized by ^/ontroversy over nuclear energy, both bombs anxiety and anger. Even among pro-nuclear Spencer R. Weart and reactors, has been exceptionally durable and people, beneath the controlled language, there is violent, exciting more emotion and public a lot of anxiety, a lot of anger. And why not? protest than any other technology. A main reason After all, everyone has heard that nuclear is that during the 20th century, nuclear energy weapons can blow up the world — or maybe gradually became a condensed symbol for many deter those who would blow it up. With nuclear features of industrial and bureucratic authority reactors, too, everyone agrees they are immense- (especially the horrors of modern war). ly important. They will save us from the global Propagandists found nuclear energy a useful disasters of the Greenhouse Effect — or perhaps symbol because it had become associated with they will poison all our posterity. potent images: not only weapons, but also un- Most of us take for granted these intensely canny scientists with mysterious rays' and mutant emotional ideas; we suppose the ideas flow from monsters; technological Utopia or universal the nature of the bombs and reactors themselves. doom; and even spiritual degradation or rebirth. But I have come to feel uneasy about this over These images had archaic connections stretching the years doing historical research on nuclear back to alchemical visions of transmutation. energy. The fact is, emotions came first, and the Decades before fission was discovered, the im- powerful devices themselves came later. -
Power Sources Challenge
POWER SOURCES CHALLENGE FUSION PHYSICS! A CLEAN ENERGY Summary: What if we could harness the power of the Sun for energy here on Fusion reactions occur when two nuclei come together to form one Earth? What would it take to accomplish this feat? Is it possible? atom. The reaction that happens in the sun fuses two Hydrogen atoms together to produce Helium. It looks like this in a very simplified way: Many researchers including our Department of Energy scientists and H + H He + ENERGY. This energy can be calculated by the famous engineers are taking on this challenge! In fact, there is one DOE Laboratory Einstein equation, E = mc2. devoted to fusion physics and is committed to being at the forefront of the science of magnetic fusion energy. Each of the colliding hydrogen atoms is a different isotope of In order to understand a little more about fusion energy, you will learn about hydrogen, one deuterium and one the atom and how reactions at the atomic level produce energy. tritium. The difference in these isotopes is simply one neutron. Background: It all starts with plasma! If you need to learn more about plasma Deuterium has one proton and one physics, visit the Power Sources Challenge plasma activities. neutron, tritium has one proton and two neutrons. Look at the The Fusion Reaction that happens in the SUN looks like this: illustration—do you see how the mass of the products is less than the mass of the reactants? That is called a mass deficit and that difference in mass is converted into energy. -
Free Radical Reactions (Read Chapter 4) A
Chemistry 5.12 Spri ng 2003, Week 3 / Day 2 Handout #7: Lecture 11 Outline IX. Free Radical Reactions (Read Chapter 4) A. Chlorination of Methane (4-2) 1. Mechanism (4-3) B. Review of Thermodynamics (4-4,5) C. Review of Kinetics (4-8,9) D. Reaction-Energy Diagrams (4-10) 1. Thermodynamic Control 2. Kinetic Control 3. Hammond Postulate (4-14) 4. Multi-Step Reactions (4-11) 5. Chlorination of Methane (4-7) Suggested Problems: 4-35–37,40,43 IX. A. Radical Chlorination of Methane H heat (D) or H H C H Cl Cl H C Cl H Cl H light (hv) H H Cl Cl D or hv D or hv etc. H C Cl H C Cl H Cl Cl C Cl H Cl Cl Cl Cl Cl H H H • Why is light or heat necessary? • How fast does it go? • Does it give off or consume heat? • How fast are each of the successive reactions? • Can you control the product ratio? To answer these questions, we need to: 1. Understand the mechanism of the reaction (arrow-pushing!). 2. Use thermodynamics and kinetics to analyze the reaction. 1 1. Mechanism of Radical Chlorination of Methane (Free-Radical Chain Reaction) Free-radical chain reactions have three distinct mechanistic steps: • initiation step: generates reactive intermediate • propagation steps: reactive intermediates react with stable molecules to generate other reactive intermediates (allows chain to continue) • termination step: side-reactions that slow the reaction; usually combination of two reactive intermediates into one stable molecule Initiation Step: Cl2 absorbs energy and the bond is homolytically cleaved. -
Could a Nearby Supernova Explosion Have Caused a Mass Extinction? JOHN ELLIS* and DAVID N
Proc. Natl. Acad. Sci. USA Vol. 92, pp. 235-238, January 1995 Astronomy Could a nearby supernova explosion have caused a mass extinction? JOHN ELLIS* AND DAVID N. SCHRAMMtt *Theoretical Physics Division, European Organization for Nuclear Research, CH-1211, Geneva 23, Switzerland; tDepartment of Astronomy and Astrophysics, University of Chicago, 5640 South Ellis Avenue, Chicago, IL 60637; and *National Aeronautics and Space Administration/Fermilab Astrophysics Center, Fermi National Accelerator Laboratory, Batavia, IL 60510 Contributed by David N. Schramm, September 6, 1994 ABSTRACT We examine the possibility that a nearby the solar constant, supernova explosions, and meteorite or supernova explosion could have caused one or more of the comet impacts that could be due to perturbations of the Oort mass extinctions identified by paleontologists. We discuss the cloud. The first of these has little experimental support. possible rate of such events in the light of the recent suggested Nemesis (4), a conjectured binary companion of the Sun, identification of Geminga as a supernova remnant less than seems to have been excluded as a mechanism for the third,§ 100 parsec (pc) away and the discovery ofa millisecond pulsar although other possibilities such as passage of the solar system about 150 pc away and observations of SN 1987A. The fluxes through the galactic plane may still be tenable. The supernova of y-radiation and charged cosmic rays on the Earth are mechanism (6, 7) has attracted less research interest than some estimated, and their effects on the Earth's ozone layer are of the others, perhaps because there has not been a recent discussed. -
NUREG-1350, Vol. 31, Information
NRC Figure 31. Moisture Density Guage Bioshield Gauge Surface Detectors Depth Radiation Source GLOSSARY 159 GLOSSARY Glossary (Abbreviations, Definitions, and Illustrations) Advanced reactors Reactors that differ from today’s reactors primarily by their use of inert gases, molten salt mixtures, or liquid metals to cool the reactor core. Advanced reactors can also consider fuel materials and designs that differ radically from today’s enriched-uranium dioxide pellets within zirconium cladding. Agreement State A U.S. State that has signed an agreement with the U.S. Nuclear Regulatory Commission (NRC) authorizing the State to regulate certain uses of radioactive materials within the State. Atomic energy The energy that is released through a nuclear reaction or radioactive decay process. One kind of nuclear reaction is fission, which occurs in a nuclear reactor and releases energy, usually in the form of heat and radiation. In a nuclear power plant, this heat is used to boil water to produce steam that can be used to drive large turbines. The turbines drive generators to produce electrical power. NUCLEUS FRAGMENT Nuclear Reaction NUCLEUS NEW NEUTRON NEUTRON Background radiation The natural radiation that is always present in the environment. It includes cosmic radiation that comes from the sun and stars, terrestrial radiation that comes from the Earth, and internal radiation that exists in all living things and enters organisms by ingestion or inhalation. The typical average individual exposure in the United States from natural background sources is about 310 millirem (3.1 millisievert) per year. 160 8 GLOSSARY 8 Boiling-water reactor (BWR) A nuclear reactor in which water is boiled using heat released from fission.