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The Radiochemistry of Beryllium
National Academy of Sciences National Research Council I NUCLEAR SCIENCE SERIES The Radiochemistry ·of Beryllium COMMITTEE ON NUCLEAR SCIENCE L. F. CURTISS, Chairman ROBLEY D. EVANS, Vice Chairman National Bureau of Standards MassaChusetts Institute of Technol0gy J. A. DeJUREN, Secretary ./Westinghouse Electric Corporation H.J. CURTIS G. G. MANOV Brookhaven National' LaboratOry Tracerlab, Inc. SAMUEL EPSTEIN W. WAYNE MEINKE CalUornia Institute of Technology University of Michigan HERBERT GOLDSTEIN A.H. SNELL Nuclear Development Corporation of , oak Ridge National Laboratory America E. A. UEHLING H.J. GOMBERG University of Washington University of Michigan D. M. VAN PATTER E.D.KLEMA Bartol Research Foundation Northwestern University ROBERT L. PLATZMAN Argonne National Laboratory LIAISON MEMBERS PAUL C .. AEBERSOLD W.D.URRY Atomic Energy Commission U. S. Air Force J. HOW ARD McMILLEN WILLIAM E. WRIGHT National Science Foundation Office of Naval Research SUBCOMMITTEE ON RADIOCHEMISTRY W. WAYNE MEINKE, Chairman HAROLD KIRBY University of Michigan Mound Laboratory GREGORY R. CHOPPIN GEORGE LEDDICOTTE Florida State University. Oak Ridge National Laboratory GEORGE A. COW AN JULIAN NIELSEN Los Alamos Scientific Laboratory Hanford Laboratories ARTHUR W. FAIRHALL ELLIS P. STEINBERG University of Washington Argonne National Laboratory JEROME HUDIS PETER C. STEVENSON Brookhaven National Laboratory University of California (Livermore) EARL HYDE LEO YAFFE University of CalUornia (Berkeley) McGill University CONSULTANTS NATHAN BALLOU WILLIAM MARLOW Naval Radiological Defense Laboratory N atlonal Bureau of Standards JAMESDeVOE University of Michigan CHF.MISTRY-RADIATION AND RADK>CHEMIST The Radiochemistry of Beryllium By A. W. FAIRHALL. Department of Chemistry University of Washington Seattle, Washington May 1960 ' Subcommittee on Radiochemistry National Academy of Sciences - National Research Council Printed in USA. -
US 2018/0240561 Al Giraldo Et Al
US 20180240561A1 (i9) United States (12) Patent Application Publication oo) Pub. No.: US 2018/0240561 Al Giraldo et al. (43) Pub. Date: Aug. 23,2018 (54) DIRECT SYNTHESIS OF RADIOACTIVE Publication Classification NANOPARTICLES INVOLVING NEUTRONS (51) Int. Cl. G21G 1/06 (2006.01) (71) Applicants:Carlos Henry Castano Giraldo, Rolla, G21G 1/12 (2006.01) MO (US); Maria Camila Garcia Toro, B82Y 5/00 (2006.01) Rolla, MO (US); Brian Michael Mills, (52) U.S. Cl. Rolla, MO (US) CPC ...... G21G 1/06 (2013.01); G21G 2001/0094 (2013.01); B82Y5/00 (2013.01); G21G 1/12 (72) Inventors: Carlos Henry Castano Giraldo, Rolla, (2013.01) MO (US); Maria Camila Garcia Toro, Rolla, MO (US); Brian Michael Mills, (57) ABSTRACT Rolla, MO (US) A method to synthesize radioactive nanoparticles includes the production of metallic and multimetallic nanoparticles in a single step by providing an aqueous solution of the metal (73) Assignee: The Curators of the University of precursor, and irradiating the aqueous solution thereby pro Missouri, Columbia, MO (US) ducing nanoparticles. The obtained nanoparticles include one or more radioactive isotopes of gold, such as 198Au and 199Au as well as radioisotopes of silver when the obtained (21) Appl. No.: 15/892,520 nanoparticles are bimetallic. The aqueous solution is irradi ated in a radiation field that includes neutrons and gamma rays. The radiation field may be provided by a nuclear (22) Filed: Feb. 9, 2018 reactor. The aqueous solution may include silver, and bime tallic nanoparticles may be produced. Duration of the irra Related U.S. Application Data diation time is selected to control the particle size distribu tion of the produced nanoparticles. -
A 1 Case-PR/ }*Rciofft.;Is Report
.A 1 case-PR/ }*rciofft.;is Report (a) This eruption site on Mauna Loa Volcano was the main source of the voluminous lavas that flowed two- thirds of the distance to the town of Hilo (20 km). In the interior of the lava fountains, the white-orange color indicates maximum temperatures of about 1120°C; deeper orange in both the fountains and flows reflects decreasing temperatures (<1100°C) at edges and the surface. (b) High winds swept the exposed ridges, and the filter cannister was changed in the shelter of a p^hoehoc (lava) ridge to protect the sample from gas contamination. (c) Because of the high temperatures and acid gases, special clothing and equipment was necessary to protect the eyes. nose, lungs, and skin. Safety features included military flight suits of nonflammable fabric, fuil-face respirators that are equipped with dual acidic gas filters (purple attachments), hard hats, heavy, thick-soled boots, and protective gloves. We used portable radios to keep in touch with the Hawaii Volcano Observatory, where the area's seismic activity was monitored continuously. (d) Spatter activity in the Pu'u O Vent during the January 1984 eruption of Kilauea Volcano. Magma visible in the circular conduit oscillated in a piston-like fashion; spatter was ejected to heights of 1 to 10 m. During this activity, we sampled gases continuously for 5 hours at the west edge. Cover photo: This aerial view of Kilauea Volcano was taken in April 1984 during overflights to collect gas samples from the plume. The bluish portion of the gas plume contained a far higher density of fine-grained scoria (ash). -
Measurement of 10Be from Lake Malawi (Africa) Drill Core Sediments and Implications for Geochronology
Palaeogeography, Palaeoclimatology, Palaeoecology 303 (2011) 110–119 Contents lists available at ScienceDirect Palaeogeography, Palaeoclimatology, Palaeoecology journal homepage: www.elsevier.com/locate/palaeo Measurement of 10Be from Lake Malawi (Africa) drill core sediments and implications for geochronology L.R. McHargue a,⁎, A.J.T. Jull b, A. Cohen a a Department of Geosciences, University of Arizona, 1040 E. Fourth Street, Tucson, Arizona 85721, United States b NSF Arizona AMS Laboratory, University of Arizona, 1118 E. Fourth Street, Tucson, Arizona 85721, United States article info abstract Article history: The cosmogenic radionuclide 10Be was measured from drill core sediments from Lake Malawi in order to Received 19 August 2008 help construct a chronology for the study of the tropical paleoclimate in East Africa. Sediment samples were Received in revised form 29 January 2010 taken every 10 m from the core MAL05-1C to 80 m in depth and then from that depth in core MAL05-1B to Accepted 4 February 2010 382 m. Sediment samples were then later taken at a higher resolution of every 2 m from MAL05-1C. They Available online 12 February 2010 were then leached to remove the authigenic fraction, the leachate was processed to separate out the beryllium isotopes, and 10Be was measured at the TAMS Facility at the University of Arizona. The 10Be/9Be Keywords: fi Beryllium-10 pro le from Lake Malawi sediments is similar to those derived from marine sediment cores for the late Cosmogenic radionuclide Pleistocene, and is consistent with the few radiocarbon and OSL IR measurements made from the same core. Lake sediments Nevertheless, a strong correlation between the stable isotope 9Be and the cosmogenic isotope 10Be suggests Lake Malawi that both isotopes have been well mixed before deposition unlike in some marine sediment cores. -
Measurement and Analysis of the Resolved Resonance Cross Sections of the Natural Hafnium Isotopes
CORE Metadata, citation and similar papers at core.ac.uk Provided by University of Birmingham Research Archive, E-theses Repository MEASUREMENT AND ANALYSIS OF THE RESOLVED RESONANCE CROSS SECTIONS OF THE NATURAL HAFNIUM ISOTOPES by TIMOTHY CHRISTOPHER WARE A thesis submitted to The University of Birmingham for the degree of DOCTOR OF PHILOSOPHY School of Physics and Astronomy College of Engineering and Physical Sciences The University of Birmingham June 2010 University of Birmingham Research Archive e-theses repository This unpublished thesis/dissertation is copyright of the author and/or third parties. The intellectual property rights of the author or third parties in respect of this work are as defined by The Copyright Designs and Patents Act 1988 or as modified by any successor legislation. Any use made of information contained in this thesis/dissertation must be in accordance with that legislation and must be properly acknowledged. Further distribution or reproduction in any format is prohibited without the permission of the copyright holder. ABSTRACT Hafnium is a ductile metallic element with a large neutron absorption cross section. It can be used in reactor control rods to regulate the fission process. The NEA High Priority Request List for nuclear data presents a need for improved characterisation of the hafnium cross section in the resolved resonance region. This thesis presents new resonance cross section parameters for the six natural hafnium isotopes. Cross section measurements, supported by the NUDAME and EUFRAT projects, were performed at the IRMM Geel GELINA time-of-flight facility. Capture experiments were conducted on the 12 m, 28 m and 58 m flight paths using C6D6 detectors and transmission experiments were performed at flight paths of 26 m and 49 m using a 6Li glass detector. -
First Search for $\Alpha $ Decays of Naturally Occurring Hf Nuclides With
First search for α decays of naturally occurring Hf nuclides with emission of γ quanta F.A. Danevicha,1, M. Hultb, D.V. Kasperovycha, G.P. Kovtunc,d, K.V. Kovtune, G. Lutterb, G. Marissensb, O.G. Polischuka, S.P. Stetsenkoc, V.I. Tretyaka aInstitute for Nuclear Research, 03028 Kyiv, Ukraine bEuropean Commission, Joint Research Centre, Retieseweg 111, 2440 Geel, Belgium cNational Scientific Center Kharkiv Institute of Physics and Technology, 61108 Kharkiv, Ukraine dKarazin Kharkiv National University, 61022 Kharkiv, Ukraine ePublic Enterprise “Scientific and Technological Center Beryllium”, 61108 Kharkiv, Ukraine Abstract The first ever search for α decays to the first excited state in Yb was performed for six isotopes of hafnium (174, 176, 177, 178, 179, 180) using a high purity Hf-sample of natural isotopic abundance with a mass of 179.8 g. For 179Hf, also α decay to the ground state of 175Yb was searched for thanks to the β-instability of the daughter nuclide 175Yb. The measurements were conducted using an ultra low-background HPGe-detector system located 225 m underground. After 75 d of data taking no decays were detected but lower 15 18 bounds for the half-lives of the decays were derived on the level of lim T1/2 ∼ 10 −10 a. The decay with the shortest half-life based on theoretical calculation is the decay of 174Hf to the first 2+ 84.3 keV excited level of 170Yb. The experimental lower bound was found 15 to be T1/2 ≥ 3.3 × 10 a. Keywords: Alpha decay; 174Hf, 176Hf, 177Hf, 178Hf, 179Hf, 180Hf, Low-background HPGe γ spec- trometry arXiv:1911.02597v1 [nucl-ex] 6 Nov 2019 1 INTRODUCTION Alpha decay is one of the most important topics of nuclear physics both from the theoretical and experimental points of view. -
Status of Fission Yield Measurements
nij»wiiM>iT»i»n'i»wwr I '• • «• PORTIOHS OF THIS &EPOTT ARE till •{•1& * i STATUS OF FI5.SIOM YIELD MEASUREHEMTS - i William J. Maeck Exxon Nuclear Idaho Company, Inc.* Idaho National Engineering Laboratory P.O. Box 2300 Idaho Fails, Idaho 83401, USA NOTICE . vtrpiird at Mt t*W. nm my < at i!tt$lte<K of anunwi my I*gal ! •prfn-nu Urn in uu *nuld noi | in(iuif.f privately 'IUWII n Prepared For Third ASTM-EURATOM Symposium On Reactor Dosimetry To be held at Ispra, Italy October 1-5, 1979 rUnder U^S... Department of Energy Idaho Operations Office Contract £- /L- - AC 07- 7c!XV>o 1. INTRODUCTION Fission yield data, for all neutron energies, play an important role in f many of the disiplines (fuel burnup, /ission rate measurements, dosimetry, reactor physics, damage studies, post irradiation fuel analysis, etc-) being discussed at this symposium. This paper reviews and presents a brief discussion i of the current status of fission yield measurement programs being conducted in the major laboratories throughout the world, and when possible, to—identify future activities. The contents of this paper are based on tv/o sources: 1) a mailing by the author to various principal investigators furnishing a form which could be used to describe their most current work, and 2) reference to the most recent IAEA Nuclear Data Section document "Progress in Fission Product Nuclear Data" , which is a compilation of current measurement activities relative i to fission product nuclear data, • • , The~gGnera-l-orgunizat.ij?Jl_oI._t]ie,.p.aper_Js..by-_f.issioning. -
Cosmogenic Production As a Background in Searching For
Cosmogenic Production as a Background in Searching for Rare Physics Processes D.-M. Mei a , Z.-B. Yin a,b,c,1, S. R. Elliott d aDepartment of Physics, The University of South Dakota, Vermillion, South Dakota 57069 bInstitute of Particle Physics, Huazhong Normal University, Wuhan 430079, China cKey Laboratory of Quark & Lepton Physics (Huazhong Normal University), Ministry of Education, China dLos Alamos National Laboratory, Los Alamos, New Mexico 87545 Abstract We revisit calculations of the cosmogenic production rates for several long-lived iso- topes that are potential sources of background in searching for rare physics processes such as the detection of dark matter and neutrinoless double-beta decay. Using up- dated cosmic-ray neutron flux measurements, we use TALYS 1.0 to investigate the cosmogenic activation of stable isotopes of several detector targets and find that the cosmogenic isotopes produced inside the target materials and cryostat can result in large backgrounds for dark matter searches and neutrinoless double-beta decay. We use previously published low-background HPGe data to constrain the production of 3H on the surface and the upper limit is consistent with our calculation. We note that cosmogenic production of several isotopes in various targets can generate po- arXiv:0903.2273v1 [nucl-ex] 12 Mar 2009 tential backgrounds for dark matter detection and neutrinoless double-beta decay with a massive detector, thus great care should be taken to limit and/or deal with the cosmogenic activation of the targets. Key words: Cosmogenic activation, Dark matter detection, Double-beta decay PACS: 13.85.Tp, 23.40-s, 25.40.Sc, 28.41.Qb, 95.35.+d, 29.40.Wk Email address: [email protected] (D.-M. -
Meteoric Be and Be As Process Tracers in the Environment
Chapter 5 Meteoric 7Be and 10Be as Process Tracers in the Environment James M. Kaste and Mark Baskaran 7 10 Abstract Be (T1/2 ¼ 53 days) and Be (T1/2 ¼ occurring Be isotopes of use to Earth scientists are the 7 1.4 Ma) form via natural cosmogenic reactions in the short-lived Be (T1/2 ¼ 53.1 days) and the longer- 10 atmosphere and are delivered to Earth’s surface by wet lived Be (T1/2 ¼ 1.4 Ma; Nishiizumi et al. 2007). and dry deposition. The distinct source term and near- Because cosmic rays that cause the initial cascade of constant fallout of these radionuclides onto soils, vege- neutrons and protons in the upper atmosphere respon- tation, waters, ice, and sediments makes them valuable sible for the spallation reactions are attenuated by tracers of a wide range of environmental processes the mass of the atmosphere itself, production rates of operating over timescales from weeks to millions of comsogenic Be are three orders of magnitude higher in years. Beryllium tends to form strong bonds with oxygen the stratosphere than they are at sea-level (Masarik and atoms, so 7Be and 10Be adsorb rapidly to organic and Beer 1999, 2009). Most of the production of cosmo- inorganic solid phases in the terrestrial and marine envi- genic Be therefore occurs in the upper atmosphere ronment. Thus, cosmogenic isotopes of beryllium can be (5–30 km), although there is trace, but measurable used to quantify surface age, sediment source, mixing production as oxygen atoms in minerals at the Earth’s rates, and particle residence and transit times in soils, surface are spallated (in situ produced; see Lal 2011, streams, lakes, and the oceans. -
Oxidation-Reduction Alternating Copolymerization of Germylene and N-Phenyl-P-Quinoneimine
Polymer Journal (2015) 47, 31–36 & 2015 The Society of Polymer Science, Japan (SPSJ) All rights reserved 0032-3896/15 www.nature.com/pj ORIGINAL ARTICLE Oxidation-reduction alternating copolymerization of germylene and N-phenyl-p-quinoneimine Satoru Iwata1, Mitsunori Abe1, Shin-ichiro Shoda1 and Shiro Kobayashi1,2 The germylenes bis[bis(trimethylsilyl)amido]germanium (1a) and bis[t-butyl-trimethylsilyl]amido]germanium (1b) were reacted with N-phenyl-p-quinoneimine (2) to give copolymers (3a and 3b) with alternating tetravalent germanium and p-aminophenol units. The copolymerization took place smoothly at 0 °C without added catalyst or initiator. 1 acted as a reductant monomer, and 2 acted as an oxidant monomer (oxidation-reduction alternating copolymerization). Product copolymers were obtained in very high yields and had high molecular weights. The copolymers were soluble in toluene, benzene, n-hexane and chloroform, whereas they were insoluble in acetonitrile and acetone. Additionally, they were stable toward hydrolytic degradation. Electron spin resonance (ESR) spectroscopic studies of the reaction suggested a structure of a stable germyl radical and a plausible mechanism of biradical copolymerization. Polymer Journal (2015) 47, 31–36; doi:10.1038/pj.2014.84; published online 8 October 2014 INTRODUCTION investigations.10 Five- and six-membered cyclic germylenes, conver- Divalent germanium compounds (germylenes) and their tin analogs sely, were copolymerized with p-benzoquinone derivatives in similar (stannylenes) continue to attract -
(12) Patent Application Publication (10) Pub. No.: US 2008/0232532 A1 Larsen Et Al
US 20080232532A1 (19) United States (12) Patent Application Publication (10) Pub. No.: US 2008/0232532 A1 Larsen et al. (43) Pub. Date: Sep. 25, 2008 (54) APPARATUS AND METHOD FOR Related U.S. Application Data GENERATION OF ULTRA LOW MOMENTUM NEUTRONS (60) Provisional application No. 60/676,264, filed on Apr. 29, 2005. Provisional application No. 60/715,622, filed on Sep. 9, 2005. (76) Inventors: Lewis G. Larsen, Chicago, IL (US); Alan Widom, Brighton, MA (US) Publication Classification (51) Int. Cl. Correspondence Address: H05H 3/06 (2006.01) COOK, ALEX, MCFARRON, MANZO, (52) U.S. Cl. .............................................................. 376/108 CUMMINGS & MEHLER LTD (57) ABSTRACT SUTE 28SO Method and apparatus for generating ultra low momentum 2OO WESTADAMS STREET neutrons (ULMNS) using Surface plasmon polariton elec CHICAGO, IL 60606 (US) trons, hydrogen isotopes, Surfaces of metallic Substrates, col Appl. No.: 11/912,793 lective many-body effects, and weak interactions in a con (21) trolled manner. The ULMNs can be used to trigger nuclear PCT Filed: Apr. 28, 2006 transmutation reactions and produce heat. One aspect of the (22) present invention effectively provides a “transducer mecha (86) PCT NO.: PCT/US06/16379 nism that permits controllable two-way transfers of energy back-and-forth between chemical and nuclear realms in a S371(c)(1), Small-scale, low-energy, Scalable condensed matter system at (2), (4) Date: Oct. 26, 2007 comparatively modest temperatures and pressures. 1222222 Patent Application Publication Sep. 25, 2008 Sheet 1 of 8 US 2008/0232532 A1 Patent Application Publication Sep. 25, 2008 Sheet 3 of 8 US 2008/0232532 A1 & N. -
Stable Isotopes of Niobium Properties of Niobium
Stable Isotopes of Niobium Isotope Z(p) N(n) Atomic Mass Natural Abundance Nuclear Spin Nb-93 41 52 92.906376 100% 9/2+ Niobium was discovered in 1801 by Charles Hatchett. Its name comes from the Greek name Niobe, meaning “daughter of Tantalus” (tantalum is closely related to niobium in the periodic table of elements). Because the niobium was discovered in an ore called columbite, it was known temporarily as columbium. Niobium, a gray or silvery soft metal, is ductile and very malleable at room temperature and does not tarnish or oxidize at room temperature. It only reacts with oxygen and halogens when heated. It is less corrosion- resistant than tantalum is at high temperatures. Niobium is not attacked by nitric acid up to 100 °C but is vigorously attacked by the mixture of nitric and hydrofluoric acids. It is unaffected at room temperature by most acids and by aqua regia. It is attacked by alkaline solutions, to some extent, at all temperatures. Niobium becomes a superconductor at 9.15 °K. It is insoluble in water, hydrochloric acid, nitric acid and aqua regia; soluble in hydrofluoric acid; and soluble in fused alkali hydroxide. At ordinary temperatures niobium does not react with most chemicals; however, the metal is slowly attacked by hydrofluoric acid and dissolves and is attacked by hydrogen fluoride and fluorine gases, forming niobium pentafluoride. Niobium is oxidized by air at 350 ºC, first forming a pale yellow oxide film of increasing thickness, which changes its color to blue. On further heating to 400 ºC, it converts to a black film of niobium dioxide.