William Draper Harkins
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A Doubly-Magic Storage Ring EDM Measurement Method
A doubly-magic storage ring EDM measurement method Richard Talman Cornell University, Ithaca, U.S.A. 10 December, 2018 arXiv:1812.05949v1 [physics.acc-ph] 14 Dec 2018 1 Abstract This paper discusses \doubly-magic trap" operation of storage rings with su- perimposed electric and magnetic bending, allowing spins in two beams to be frozen (at the same time, if necessary), and their application to electric dipole moment (EDM) measurement. Especially novel is the possibility of simultaneous storage in the same ring of frozen spin beams of two different particle types. A few doubly-magic cases have been found: One has an 86.62990502 MeV frozen spin proton beam and a 30.09255159 MeV frozen spin positron beam (with accu- racies matching their known magnetic moments) counter-circulating in the same storage ring. (Assuming the positron EDM to be negligibly small) the positron beam can be used to null the worst source of systematic EDM error|namely, the existence of unintentional and unknown average radial magnetic field < Br > which, acting on the MDM, causes spurious background spin precession indis- tinguishable from foreground EDM-induced precession. The resulting measured proton minus positron EDM difference is then independent of < Br >. This amounts to being a measurement of the proton EDM. Most doubly-magic features can be tested in one or more \small" EDM proto- type rings. One promising example is a doubly-magic proton-helion combination, which would measure the difference between helion (i.e. helium-3) and proton EDM's. This combination can be used in the near future for EDM measurement, for example in a 10 m bending radius ring, using only already well-understood and proven technology. -
Chemistry: the Molecular Nature of Matter and Change
REVISED CONFIRMING PAGES The Components of Matter 2.1 Elements, Compounds, and 2.5 The Atomic Theory Today 2.8 Formula, Name, and Mass of Mixtures: An Atomic Overview Structure of the Atom a Compound 2.2 The Observations That Led to Atomic Number, Mass Number, and Binary Ionic Compounds an Atomic View of Matter Atomic Symbol Compounds That Contain Polyatomic Mass Conservation Isotopes Ions Definite Composition Atomic Masses of the Elements Acid Names from Anion Names Multiple Proportions 2.6 Elements: A First Look at the Binary Covalent Compounds The Simplest Organic Compounds: Dalton’s Atomic Theory Periodic Table 2.3 Straight-Chain Alkanes Postulates of the Atomic Theory Organization of the Periodic Table Masses from a Chemical Formula How the Atomic Theory Explains Classifying the Elements Representing Molecules with a the Mass Laws Compounds: An Introduction 2.7 Formula and a Model to Bonding 2.4 The Observations That Led to Mixtures: Classification and the Nuclear Atom Model The Formation of Ionic Compounds 2.9 Separation Discovery of the Electron and The Formation of Covalent An Overview of the Components of Its Properties Compounds Matter Discovery of the Atomic Nucleus (a) (b) (right) ©Rudy Umans/Shutterstock IN THIS CHAPTER . We examine the properties and composition of matter on the macroscopic and atomic scales. By the end of this chapter, you should be able to • Relate the three types of matter—elements or elementary substances, compounds, and mixtures—to the simple chemical entities that they comprise—atoms, ions, and molecules; -
Models of the Atomic Nucleus
Models of the Atomic Nucleus Second Edition Norman D. Cook Models of the Atomic Nucleus Unification Through a Lattice of Nucleons Second Edition 123 Prof. Norman D. Cook Kansai University Dept. Informatics 569 Takatsuki, Osaka Japan [email protected] Additional material to this book can be downloaded from http://extras.springer.com. ISBN 978-3-642-14736-4 e-ISBN 978-3-642-14737-1 DOI 10.1007/978-3-642-14737-1 Springer Heidelberg Dordrecht London New York Library of Congress Control Number: 2010936431 © Springer-Verlag Berlin Heidelberg 2006, 2010 This work is subject to copyright. All rights are reserved, whether the whole or part of the material is concerned, specifically the rights of translation, reprinting, reuse of illustrations, recitation, broadcasting, reproduction on microfilm or in any other way, and storage in data banks. Duplication of this publication or parts thereof is permitted only under the provisions of the German Copyright Law of September 9, 1965, in its current version, and permission for use must always be obtained from Springer. Violations are liable to prosecution under the German Copyright Law. The use of general descriptive names, registered names, trademarks, etc. in this publication does not imply, even in the absence of a specific statement, that such names are exempt from the relevant protective laws and regulations and therefore free for general use. Cover design: WMXDesign GmbH, Heidelberg Printed on acid-free paper Springer is part of Springer Science+Business Media (www.springer.com) Preface to the Second Edition Already by the 1970s, some theorists had declared that nuclear structure physics was a “closed chapter” in science, but since then it has repeatedly been found necessary to re-open this closed chapter to address old problems and to explain new phenom- ena. -
A Brief History of Nuclear Astrophysics
A BRIEF HISTORY OF NUCLEAR ASTROPHYSICS PART I THE ENERGY OF THE SUN AND STARS Nikos Prantzos Institut d’Astrophysique de Paris Stellar Origin of Energy the Elements Nuclear Astrophysics Astronomy Nuclear Physics Thermodynamics: the energy of the Sun and the age of the Earth 1847 : Robert Julius von Mayer Sun heated by fall of meteors 1854 : Hermann von Helmholtz Gravitational energy of Kant’s contracting protosolar nebula of gas and dust turns into kinetic energy Timescale ~ EGrav/LSun ~ 30 My 1850s : William Thompson (Lord Kelvin) Sun heated at formation from meteorite fall, now « an incadescent liquid mass » cooling Age 10 – 100 My 1859: Charles Darwin Origin of species : Rate of erosion of the Weald valley is 1 inch/century or 22 miles wild (X 1100 feet high) in 300 My Such large Earth ages also required by geologists, like Charles Lyell A gaseous, contracting and heating Sun 푀⊙ Mean solar density : ~1.35 g/cc Sun liquid Incompressible = 4 3 푅 3 ⊙ 1870s: J. Homer Lane ; 1880s :August Ritter : Sun gaseous Compressible As it shrinks, it releases gravitational energy AND it gets hotter Earth Mayer – Kelvin - Helmholtz Helmholtz - Ritter A gaseous, contracting and heating Sun 푀⊙ Mean solar density : ~1.35 g/cc Sun liquid Incompressible = 4 3 푅 3 ⊙ 1870s: J. Homer Lane ; 1880s :August Ritter : Sun gaseous Compressible As it shrinks, it releases gravitational energy AND it gets hotter Earth Mayer – Kelvin - Helmholtz Helmholtz - Ritter A gaseous, contracting and heating Sun 푀⊙ Mean solar density : ~1.35 g/cc Sun liquid Incompressible = 4 3 푅 3 ⊙ 1870s: J. -
Integrated M.Sc. Chemistry (CBCS) SYLLABUS Department of Chemistry Central University of Tamil Nadu Thiruvarur 610
Integrated M.Sc. Chemistry (CBCS) SYLLABUS Department of Chemistry Central University of Tamil Nadu Thiruvarur 610 101 Name of the course : Integrated M. Sc. (Chemistry) Duration : 10 semesters Intake : 30 Eligibility : Plus two examination or equivalent of any recognized board in India with 60% marks (Chemistry, Mathematics, Physics and Computer Science/Biology) for general category, 55% marks for OBC (Non-creamy layer) and 50% marks for SC/ST candidates. The candidates should not have completed 20 years of age as on 01-07-2015. Course Structure The five year program is spread into ten semesters where in first four semesters are designed for broad subject based understanding. Later six semesters will have increased focus on chemistry. The subject courses in the early stage of iM.Sc programme are simplified and of basic level that bolsters the inter-disciplinary way of learning. The third and subsequent year courses have been designed on advanced theories in chemistry with emphasis on concurrent modern laboratory techniques. Further the iM.Sc (Chemistry) programme has been included with experiments that provide exhaustive hands on experience on various sophisticated instruments, experimental techniques to enable the students secure jobs in corporate. The final semester is dedicated to specialization within the subject with research level training. The rules and regulations of Choice Based Credit System (CBCS) are applicable to this program. Generally, a student takes ten semesters to complete the program. The courses offered under CBCS, has certain credit number (2, 3 or 4). Core requirements of the programs are clearly defined. In the first two years of the program, a student has common course load with students from other departments. -
Forward Helion Scattering and Neutron Polarization N
Forward Helion Scattering and Neutron Polarization N. H. Buttimore Trinity College Dublin, Ireland Abstract. The elastic scattering of spin half helium-3 nuclei at small angles can show a sufficiently large analyzing power to enable the level of helion polarization to be evaluated. As the helion to a large extent inherits the polarization of its unpaired neutron the asymmetry observed in helion collisions can be transformed into a measurement of the polarization of its constituent neutron. Neutron polarimetry therefore relies upon understanding the spin dependence of the electromagnetic and hadronic interactions in the region of interference where there is an optimal analyzing power. Keywords: Neutron, spin polarization, helion, elastic scattering, asymmetry PACS: 11.80.Cr, 12.20.Ds, 13.40.Ks, 25.55.Ci, 13.85.Dz, 13.88.+e INTRODUCTION The spin polarized neutrons available from a polarized helium-3 beam would be very suitable for the study of polarized down quarks in various QCD processes particularly relating to transversity [1], nucleon spin structure [2], multi Pomeron exchange [3], gluon distributions [4], and additional dimensions [5]. Measuring the analyzing power in small angle elastic scattering of hadrons with spin provides an opportunity for evaluating the level of polarisation of incident helium-3 nuclei (helions) [6] thereby providing an effective neutron polarimeter [7]. Such a method relies upon an understanding of high energy spin dependence in diffractive processes [8]. Here, the interference of elastic hadronic and electromagnetic interactions in a suitable peripheral region enhances the size of the transverse spin asym- metry sufficiently to offer a tangible polarimeter for high energy helions. -
Appendix: Key Concepts and Vocabulary for Nuclear Energy
Appendix: Key Concepts and Vocabulary for Nuclear Energy The likelihood of fission depends on, among other Power Plant things, the energy of the incoming neutron. Some In most power plants around the world, heat, usually nuclei can undergo fission even when hit by a low- produced in the form of steam, is converted to energy neutron. Such elements are called fissile. electricity. The heat could come through the burning The most important fissile nuclides are the uranium of coal or natural gas, in the case of fossil-fueled isotopes, uranium-235 and uranium-233, and the power plants, or the fission of uranium or plutonium plutonium isotope, plutonium-239. Isotopes are nuclei. The rate of electrical power production in variants of the same chemical element that have these power plants is usually measured in megawatts the same number of protons and electrons, but or millions of watts, and a typical large coal or nuclear differ in the number of neutrons. Of these, only power plant today produces electricity at a rate of uranium-235 is found in nature, and it is found about 1,000 megawatts. A much smaller physical only in very low concentrations. Uranium in nature unit, the kilowatt, is a thousand watts, and large contains 0.7 percent uranium-235 and 99.3 percent household appliances use electricity at a rate of a few uranium-238. This more abundant variety is an kilowatts when they are running. The reader will have important example of a nucleus that can be split only heard about the “kilowatt-hour,” which is the amount by a high-energy neutron. -
Project Note Weston Solutions, Inc
PROJECT NOTE WESTON SOLUTIONS, INC. To: Canadian Radium & Uranium Corp. Site File Date: June 5, 2014 W.O. No.: 20405.012.013.2222.00 From: Denise Breen, Weston Solutions, Inc. Subject: Determination of Significant Lead Concentrations in Sediment Samples References 1. New York State Department of Environmental Conservation. Technical Guidance for Screening Contaminated Sediments. March 1998. [45 pages] 2. U.S. Environmental Protection Agency (EPA) Office of Emergency Response. Establishing an Observed Release – Quick Reference Fact Sheet. Federal Register, Volume 55, No. 241. September 1995. [7 pages] 3. International Union of Pure and Applied Chemistry, Inorganic Chemistry Division Commission on Atomic Weights and Isotopic Abundances. Atomic Weights of Elements: Review 2000. 2003. [120 pages] WESTON personnel collected six sediment samples (including one environmental duplicate sample) from five locations along the surface water pathway of the Canadian Radium & Uranium Corp. (CRU) site in May 2014. The sediment samples were analyzed for Target Analyte List (TAL) Metals and Stable Lead Isotopes. 1. TAL Lead Interpretation: In order to quantify the significance for Lead, Thallium and Mercury the following was performed: 1. WESTON personnel tabulated all available TAL Metal data from the May 2014 Sediment Sampling event. 2. For each analyte of concern (Lead, Thallium, and Mercury), the highest background concentration was selected and then multiplied by three. This is the criteria to find the significance of site attributable release as per Hazard Ranking System guidelines. 3. One analytical lead result (2222-SD04) of 520 mg/kg (J) was qualified with an unknown bias. In accordance with US EPA document “Using Data to Document an Observed Release and Observed Contamination”, 2222-SD03 lead concentration was adjusted by dividing by the factor value for lead of 1.44 to equal 361 mg/kg. -
ISOTOPIC ELEMENTS) and the WHOLE NUMBER RULE for ATOMIC WEIGHTS by William D
624 CHEMISTRY: W. D. HARKINS PROC. N. A. -S. -To summarize, the mechanism tentatively proposed above may be dia.. grammatically represented as follows: Insulin Glycogen-*Hexose ---Hexose mono-phosphate Hexose di-phosphate-<r-Triose phosphate and Reactive triose Carbon Lactic dioxide acid and Water 1 It has recently been noted from the Zentralblatt that Euler and Myrback (Svensk. Kem. Tidskr., 36, 295-306 (1924)) have made an apparently similar suggestion. As the originAl article has not been available it has been impossible to learn how closely the two theories coincide. 2R. Robison, Biochem. J., 16, 809 (1922). 'This step has been definitely established by Harden and his co-workers and the enzyme accomplishing the change has been named hexosephosphatase. 4 Neuberg and Kerb, Biocerm. Zs., 58, 158-170. (1913). ' Euler and Myrback, Chemie Zele Gewebe, 12, 57 (1925). THE SEPARATION OF CHLORINE INTO ISOTOPES (ISOTOPIC ELEMENTS) AND THE WHOLE NUMBER RULE FOR ATOMIC WEIGHTS By WILLiAM D. HARKINs KENT CHEMICAL LABORATORY, UNIvRSITY OP CHCAGO Comminicated August 26, 1925 Introduction.-The existence of isotopes among the heaviest or radio- active elements was demonstrated by the difference in the rays emitted by "different radioactive elements of almost identical chemical properties" now designated as isotopes of the same chemical element. Isotopes have been shown to exist in the light elements by two independent methods: by their detection in the positive ray method, and by the actual separation of the isotopes. The earliest use of the positive ray method for detecting isotopes by J. J. Thomson' resulted in the discovery of the isotopes of neon, while the separation of chlorine into isotopic fractions by Harkins and Downloaded by guest on September 25, 2021 VOL. -
Small-Scale Fusion Tackles Energy, Space Applications
NEWS FEATURE NEWS FEATURE Small-scalefusiontacklesenergy,spaceapplications Efforts are underway to exploit a strategy that could generate fusion with relative ease. M. Mitchell Waldrop, Science Writer On July 14, 2015, nine years and five billion kilometers Cohen explains, referring to the ionized plasma inside after liftoff, NASA’s New Horizons spacecraft passed the tube that’s emitting the flashes. So there are no the dwarf planet Pluto and its outsized moon Charon actual fusion reactions taking place; that’s not in his at almost 14 kilometers per second—roughly 20 times research plan until the mid-2020s, when he hopes to faster than a rifle bullet. be working with a more advanced prototype at least The images and data that New Horizons pains- three times larger than this one. takingly radioed back to Earth in the weeks that If that hope pans out and his future machine does followed revealed a pair of worlds that were far more indeed produce more greenhouse gas–free fusion en- varied and geologically active than anyone had ergy than it consumes, Cohen and his team will have thought possible. The revelations were breathtak- beaten the standard timetable for fusion by about a ing—and yet tinged with melancholy, because New decade—using a reactor that’s just a tiny fraction of Horizons was almost certain to be both the first and the size and cost of the huge, donut-shaped “tokamak” the last spacecraft to visit this fascinating world in devices that have long devoured most of the research our lifetimes. funding in this field. -
Atomic Engery Education Volume Four.Pdf
~ t a t e of ~ ofua 1952 SCIENTIFIC AND SOCIAL ASPECTS OF ATOMIC ENERGY (A Source Book /or General Use in Colleges) Volume IV The Iowa Plan for Atomic Energy Education Issu ed by the D epartment of Public Instruction J essie M. Parker Superintendent Des Moines, Iowa Published by the State .of Iowa ''The release of atomic energy on a large scale is practical. It is reasonable to anticipate that this new source of energy will cause profound changes in our present way of life." - Quoted from the Copyright 1952 Atomic Energy Act of 1946. by The State of Iowa "Unless the people have the essential facts about atonuc energy, they cannot act wisely nor can they act democratically."-. -David I Lilienthal, formerly chairman of the Atomic Energy Com.mission. IOWA PLAN FOR ATOMIC ENERGY EDUCATION FOREWORD Central Planning Committee About five years ago the Iowa State Department of Public Instruction became impressed with the need for promoting Atomic Energy Education throughout the state. Following a series of Glenn Hohnes, Iowa State Col1ege, Ames, General Chairman conferences, in which responsible educators and laymen shared their views on this problem, Emil C. Miller, Luther College, Decorah plans were made to develop material for use at the elementary, high school, college, and Barton Morgan, Iowa State College, Ames adult education levels. This volume is a resource hook for use with and by college students. M. J. Nelson, Iowa State Teachers College, Cedar Falls Actually, many of the materials in this volume have their origin in the Atomic Energy Day Hew Roberts, State University of Iowa, Iowa City programs which were sponsored by Cornell College and Luther College two or three years L. -
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).