Summary Report of the Consultants' Meeting on Nuclear Data for Production of Therapeutic Radioisotopes
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The Separation and Determination of Osmium and Ruthenium
Louisiana State University LSU Digital Commons LSU Historical Dissertations and Theses Graduate School 1969 The epS aration and Determination of Osmium and Ruthenium. Harry Edward Moseley Louisiana State University and Agricultural & Mechanical College Follow this and additional works at: https://digitalcommons.lsu.edu/gradschool_disstheses Recommended Citation Moseley, Harry Edward, "The eS paration and Determination of Osmium and Ruthenium." (1969). LSU Historical Dissertations and Theses. 1559. https://digitalcommons.lsu.edu/gradschool_disstheses/1559 This Dissertation is brought to you for free and open access by the Graduate School at LSU Digital Commons. It has been accepted for inclusion in LSU Historical Dissertations and Theses by an authorized administrator of LSU Digital Commons. For more information, please contact [email protected]. ThU dissertation has been 69-17,123 microfilmsd exactly as received MOSELEY, Harry Edward, 1929- THE SEPARATION AND DETERMINATION OF OSMIUM AND RUTHENIUM. Louisiana State University and Agricultural and Mechanical College, PhJ>., 1969 Chemistry, analytical University Microfilms, Inc., Ann Arbor, Michigan THE SEPARATION AND DETERMINATION OF OSMIUM AND RUTHENIUM A Dissertation Submitted to the Graduate Faculty of the Louisiana State University and Agricultural and Mechanical College in partial fulfillment of the requirements for the degree of Doctor of Philosophy in The Department of Chemistry Harry Edward Moseley B.S., Lpuisiana State University, 1951 M.S., Louisiana State University, 1952 J anuary, 1969 ACKNOWLEDGMENTS Thanks are due to Dr. Eugene W. Berg under whose direction this work was performed, to Dr. A. D. Shendrikar for his help in the tracer studies, and to Mr. J. H. R. Streiffer for his help in writing the com puter program. -
How Earth Got Its Moon Article
FEATURE How Earth Got its MOON Standard formation tale may need a rewrite By Thomas Sumner he moon’s origin story does not add up. Most “Multiple impacts just make more sense,” says planetary scientists think that the moon formed in the earli- scientist Raluca Rufu of the Weizmann Institute of Science in est days of the solar system, around 4.5 billion years Rehovot, Israel. “You don’t need this one special impactor to Tago, when a Mars-sized protoplanet called Theia form the moon.” whacked into the young Earth. The collision sent But Theia shouldn’t be left on the cutting room floor just debris from both worlds hurling into orbit, where the rubble yet. Earth and Theia were built largely from the same kind of eventually mingled and combined to form the moon. material, new research suggests, and so had similar composi- If that happened, scientists expect that Theia’s contribution tions. There is no sign of “other” material on the moon, this would give the moon a different composition from Earth’s. perspective holds, because nothing about Theia was different. Yet studies of lunar rocks show that Earth and its moon are “I’m absolutely on the fence between these two opposing compositionally identical. That fact throws a wrench into the ideas,” says UCLA cosmochemist Edward Young. Determining planet-on-planet impact narrative. which story is correct is going to take more research. But the Researchers have been exploring other scenarios. Maybe answer will offer profound insights into the evolution of the the Theia impact never happened (there’s no direct evidence early solar system, Young says. -
Optimization Studies of the CERN-ISOLDE Neutron Converter and Fission Target System
Optimization Studies of the CERN-ISOLDE neutron converter and fission target system Raul Luís1, José G. Marques, Thierry Stora, Pedro Vaz, Luca Zanini 1ITN – Estrada Nacional 10, 2686-953, Sacavém, Portugal 2CERN – CH-1211, Genève 23, Switzerland 3PSI – 5232 Villigen, Switzerland E-mail: [email protected] Abstract. The ISOLDE facility at CERN has been one of the leading isotope separator on-line (ISOL) facilities worldwide since it became operative in 1967. More than 1000 isotopes are available at ISOLDE, produced after the bombardment of various primary targets with a pulsed proton beam of energy 1.4 GeV and an average intensity of 2 μA. A tungsten solid neutron converter has been used for ten years to produce neutron-rich fission fragments in UCx targets. In this work, the Monte Carlo code FLUKA and the cross section codes TALYS and ABRABLA were used to study the current layout of the neutron converter and fission target system of the ISOLDE facility. An optimized target system layout is proposed, which maximizes the production of neutron-rich isotopes and reduces the contamination by undesired proton-rich isobars. The studies here reported can already be applied to ISOLDE and will be of special relevance for the future facilities HIE-ISOLDE and EURISOL. 1. Introduction One of the most efficient ways to study nuclei far from stability is the Isotope Separation On-Line (ISOL) method, in which a beam of high-energy hadrons hits a thick target, producing a great variety of radioactive products through different processes like fission, spallation and fragmentation [1]. The resulting nuclides can be studied after they are extracted from the target, ionized and mass separated. -
Concurrent Reduction and Distillation; an Improved Technique for the Recovery and Chemical Refinement of the Isotopes of Cadmium and Zinc*
If I CONCURRENT REDUCTION AND DISTILLATION; AN IMPROVED TECHNIQUE FOR THE RECOVERY AND CHEMICAL REFINEMENT OF THE ISOTOPES OF CADMIUM AND ZINC* H. H. Cardill L. E. McBride LOHF-821046—2 E. W. McDaniel DE83 001931 Operations Division Oak Ridge National Laboratory Oak Ridge, Tennessee 3 7830 .DISCLAIMER • s prepared es an accouni oi WOTk sconsQ'ed by an agency of itie United Slates Cover r "iiit?3 Stilt 65 Gov(?fnft»gn ^ ri(jt ^nv aQcncy Tllf GO* ^or rlny O^ tt^^ir ^rnployut^. TigV MASTER lostifl. ion, apod'aiuj pioiJut;. <y vned nghtv Reference hcein xc any v>t^-'T*t. ^ Dv ^.r^de narno, tf^Oernafk^ mir'ij'iJClureT. or otrierw «d <Jo*^ •nenaalion. or liivONng bv 'Vhe United _^_ . vs and opinions of authors enp'«i«] herein do noi IOM t' irip UnitK* Stales Govefnrneni c a^v agency For presentation at the 11th World Conference of the International Nuclear Target Development Society, October 6-8, 1982, Seattle, Washington. By acceptance of this article, the publisher or recipient acknowledge* the U.S. Govarnment's right to retain a nonaxclusiva, royalty-frtta license in and to any copyright covering tha article. NOTICE P0T09_0£-Jfns,J^SPQRT_JfgE_Il,LESIBLE. I has been reproauce.1 from the best available aopy to pensit the broadest possible avail- ability* *Research sponsored by the Office of Basic Energy Science, U.S. Department of Energy under contract W-7405-eng-26 with the Union Carbide Co rpcration,, DISTRIBUTION OF THIS DOCUMEHT 18 UNLIMITED ' CONCURRENT REDUCTION AND DISTILLATION - AY. IMPROVED TECHNIQUE FOR THE RECOVERY AND CHEMICAL REFINEMENT OF THE ISOTOPES OF CADMIUM AND ZINC H. -
Jahresbericht 2007
IKMz 2008- 1 ISSN 0932-7622 INSTITUT FÜR KERNCHEMIE UNIVERSITÄT MAINZ JAHRESBERICHT 2007 August 2008 FRITZ-STRASSMANN-WEG 2, D-55128 MAINZ, TELEFON (06131) 3925879, TELEFAX (06131) 3925253 Kernchemie im Internet Das Institut für Kernchemie der Universität Mainz ist mit einer Homepage im World Wide Web vertreten. Unter der Adresse http://www.kernchemie.uni-mainz.de finden Sie aktuelle Informationen zum Institut, seinen Mitarbeitern, den Lehrveranstaltungen und den Forschungsaktivitäten. Die in diesem Bericht vorgelegten Ergebnisse stammen zum Teil aus noch nicht abgeschlossenen Arbeiten und sind daher als vorläufige Mitteilung zu bewerten. INSTITUT FÜR KERNCHEMIE UNIVERSITÄT MAINZ JAHRESBERICHT 2007 Herausgeber: Frank Rösch Mainz, im August 2008 Vorwort Der vorliegende Jahresbericht 2007 gibt einen Überblick über die wissenschaftlichen Aktivitäten des Instituts für Kernchemie. Er legt damit gleichzeitig all denen, die uns in ideeller und finanzieller Weise gefördert haben, Rechenschaft ab über die Verwendung nicht unerheblicher öffentlicher Mittel. Außerdem beschreibt er den Status der technischen Einrichtungen des Instituts und technische Neu- entwicklungen. Schließlich stellt er die Ergebnisse des Instituts in Form von Publikationen, Konferenzbeiträgen, Dissertationen, Diplom- und Staatsexamensarbeiten sowie die Beiträge seiner Hochschullehrer in der Lehre und Weiterbildung dar. Der wissenschaftliche Bericht umfasst die drei Forschungsschwerpunkte: • Kernchemie im Sinne grundlegender Fragestellungen, • Radiopharmazeutische Chemie und Anwendung radiochemischer Methoden mit medizinischer Zielsetzung, • Hochempfindliche und –selektive Analytik für umweltrelevante, technische und biologische Probleme. Im August 2007 hat der Präsident unserer Universität, Herr Prof. Dr. Krausch, die Laufzeit des Forschungsreaktors TRIGA Mainz bis zunächst 2020 verlängert. Die Carl-Zeiss-Stiftung hat 2007 die Einrichtung einer Juniorprofessur für das Thema „Ultrakalte Neutronen“ am Institut für Kernchemie ab 2008 ermöglicht. -
I, Bichard Lewis Woodward, Was Horn in Kansas City
AUTOBIOGRAPHT I, Bichard Lewis Woodward, was horn in Kansas City, Missouri, December 11, 1913 - My elementary and secondary school education was in the public schools of Kansas City and St . Louis, Missouri. In June, 1935. I received the degree Bachelor of Science in Civil Engineering from Washington University. I received the degree Master of Science from Harvard University in June, 1948. Since 1937 I have been an officer of tie United States Public Health Service . Under the auspices of this organisation, I have studied in the Department of Physics at the Ohio State University since June, 1949- - 42 - ACKNOWLEDGMENTS I wish to acknowledge the assistance of my adviser Prof M. L. Pool, of my coworker Mr. S . C. Fultz, of our chemist Mr. James McGlotten, and of Mr. Claude McWhlrt and other members of the staff of the Physics Department shops. - hi - BLBLIOGEAPHT 1. J. H. Buck, Fhys. Rev., 59, 1025 (1938) 2. A. Mukerji. P. Preiswerk, Felv . Phys. Acta, 23, 516 (1950) 3* G • T. Seahorg, I. Perlman, Rev. Mod. Phys., 20, 585 (1998) 9-. G. E. Valley, R. 1. McCreary, Phys. Rev., 5 6, 863 (1939) 5 . S. Sag&ne, S . Kojina, G. Miyamoto, Fhys. Math. Soc . Japan, Proc., 21, 728 (1939) 6 . E. C. Barker, Plutonium Proj . Report Mon. P-269, 8 (199-7) 7. S . E. Haynes, Phys. Rev., 79, 9-23 (1998) 8 . I*. M. Langer, R. D. Moffat, Ihys . Rev., 80, 6 51 (1950) 9. A. C. Helmholz, Phys. Rev., 60, 9-15 (1991) 10. J. M. Cork, L. N. Hadley, Jr., C. V. -
Beta Decay of Neutron-Rich Isotopes of Zinc and Gallium
University of Tennessee, Knoxville TRACE: Tennessee Research and Creative Exchange Doctoral Dissertations Graduate School 5-2015 Beta decay of neutron-rich isotopes of zinc and gallium Mohammad Faleh M. Al-Shudifat University of Tennessee - Knoxville, [email protected] Follow this and additional works at: https://trace.tennessee.edu/utk_graddiss Part of the Nuclear Commons Recommended Citation Al-Shudifat, Mohammad Faleh M., "Beta decay of neutron-rich isotopes of zinc and gallium. " PhD diss., University of Tennessee, 2015. https://trace.tennessee.edu/utk_graddiss/3288 This Dissertation is brought to you for free and open access by the Graduate School at TRACE: Tennessee Research and Creative Exchange. It has been accepted for inclusion in Doctoral Dissertations by an authorized administrator of TRACE: Tennessee Research and Creative Exchange. For more information, please contact [email protected]. To the Graduate Council: I am submitting herewith a dissertation written by Mohammad Faleh M. Al-Shudifat entitled "Beta decay of neutron-rich isotopes of zinc and gallium." I have examined the final electronic copy of this dissertation for form and content and recommend that it be accepted in partial fulfillment of the equirr ements for the degree of Doctor of Philosophy, with a major in Physics. Robert Grzywacz, Major Professor We have read this dissertation and recommend its acceptance: Soren Sorensen, Thomas Papenbrock, Jason P. Hayward Accepted for the Council: Carolyn R. Hodges Vice Provost and Dean of the Graduate School (Original signatures are on file with official studentecor r ds.) Beta decay of neutron-rich isotopes of zinc and gallium A Dissertation Presented for the Doctor of Philosophy Degree The University of Tennessee, Knoxville Mohammad Faleh M. -
Evolution of Nuclear Structure in Neutron-Rich Odd-Zn Isotopes and Isomers ∗ C
Physics Letters B 771 (2017) 385–391 Contents lists available at ScienceDirect Physics Letters B www.elsevier.com/locate/physletb Evolution of nuclear structure in neutron-rich odd-Zn isotopes and isomers ∗ C. Wraith a, X.F. Yang b, , L. Xie c, C. Babcock a, J. Bieron´ d, J. Billowes c, M.L. Bissell b,c, K. Blaum e, B. Cheal a, L. Filippin f, R.F. Garcia Ruiz b,c, W. Gins b, L.K. Grob g, G. Gaigalas h, M. Godefroid f, C. Gorges i, H. Heylen b, M. Honma j, P. Jönsson k, S. Kaufmann g, M. Kowalska l, J. Krämer i, S. Malbrunot-Ettenauer l, R. Neugart e,g, G. Neyens b, W. Nörtershäuser g,i, F. Nowacki m, T. Otsuka n, J. Papuga b, R. Sánchez o, Y. Tsunoda p, D.T. Yordanov q a Oliver Lodge Laboratory, Oxford Street, University of Liverpool, Liverpool, L69 7ZE, United Kingdom b KU Leuven, Instituut voor Kern- en Stralingsfysica, B-3001 Leuven, Belgium c School of Physics and Astronomy, The University of Manchester, Manchester, M13 9PL, United Kingdom d Instytut Fizyki imienia Mariana Smoluchowskiego, Uniwersytet Jagiello´nski, ul. prof. Stanisława Łojasiewicza 11, Kraków, Poland e Max-Plank-Institut für Kernphysik, D-69117 Heidelberg, Germany f Chimie Quantique et Photophysique, Université Libre de Bruxelles, B-1050 Brussels, Belgium g Institut für Kernchemie, Universität Mainz, D-55128 Mainz, Germany h Institute of Theoretical Physics and Astronomy, Vilnius University, Sauletekio˙ av. 3, LT-10222 Vilnius, Lithuania i Institut für Kernphysik, TU Darmstadt, D-64289 Darmstadt, Germany j Center for Mathematical Sciences, University of Aizu, Tsuruga, -
Stable Isotope Separation in Calutrons
Printed ill tho llnitzd Statss ot 4mcm 4vailsble frurii Nations' Technical Information Service U S :3ep?rtmelli uf Commerce 5285 Port 4oyal Cosd Spririizflald Viryinis 22161 NTlS ptwiodes P~III~~Copy ,498, Microfiche P,C1 I his rcpoti \*!is prspxed as an account of >,dSi-k sponsored by a3 agsncy of the United Sraies Governr;,ent. Neither thc !J nited Skiics i<n.~cti $IK~: nor any agency th2reof. no? any of thzir employoes, (ciakc?.Aijy ivarranty, express or irripiled, or assunias any legal liability or responsibility for ihe accuracy. compleienass, or usefulness of any inforriraiton. ;p ius, product, or process disclosed, or represents that its usewould not infr privately o-v?d ilghts Rcferencc herein to ai-y specific commercial product, process, or service by trade nziile, Zi'adei*lark, manufacturer, or otherwise, does not necsssarily constitute or imply its enduisemcat, recorn,n faVOiii-,g by ille United States(;ovc;riiiie!ii 01- any Zgency thereof Th opinions of auiihols cxp:essed here:!: d~ ~iui neccssarily statc or refisc?!host of the United Sta?ezGovernmer:?or any ngcncy therccf. ____ ___________... ..... .____ ORNL/TM-10356 OPERATIONS DIVISION STABLE ISOTOPE SEPARATION IN CALUTRONS: FORTY YEARS OF PRODUCTION AND DISTRIBUTION W. A. Bell J. G. Tracy Date Published: November 1987 Prepared by the OAK RIDGE NATIONAL LABORATORY Oak Ridge, Tennessee 37831 operated by MARTIN MARIETTA ENERGY SYSTEMS, INC. for the U.S. DEPARTMENT OF ENERGY under Contract No. DE-AC05-840R21400 iti CONTENTS Page ACKNOWLEDGMENTS ................................................. iv I. INTRODUCTION .............................................. 1 11. PROGRAM EVOLUTION ......................................... 1 111. RESEARCH AND DEVELOPMENT .................................. 5 IV. CHEMISTRY ................................................. 8 V. -
Rotation Aligned Negative Parity Side Bands in Light Tungsten and Osmium Nuclei G.D
ROTATION ALIGNED NEGATIVE PARITY SIDE BANDS IN LIGHT TUNGSTEN AND OSMIUM NUCLEI G.D. Dracoulis To cite this version: G.D. Dracoulis. ROTATION ALIGNED NEGATIVE PARITY SIDE BANDS IN LIGHT TUNG- STEN AND OSMIUM NUCLEI. Journal de Physique Colloques, 1980, 41 (C10), pp.C10-66-C10-78. 10.1051/jphyscol:19801007. jpa-00220626 HAL Id: jpa-00220626 https://hal.archives-ouvertes.fr/jpa-00220626 Submitted on 1 Jan 1980 HAL is a multi-disciplinary open access L’archive ouverte pluridisciplinaire HAL, est archive for the deposit and dissemination of sci- destinée au dépôt et à la diffusion de documents entific research documents, whether they are pub- scientifiques de niveau recherche, publiés ou non, lished or not. The documents may come from émanant des établissements d’enseignement et de teaching and research institutions in France or recherche français ou étrangers, des laboratoires abroad, or from public or private research centers. publics ou privés. JOURNAL DE PHYSIQUE CoZZoque CIO, suppZe'ment au n012, Tome 41, de'cembre 1980, page C10-66 ROTATION ALIGNED NEGATIVE PARITY SIDE BANDS IN LIGHT TUNGSTEN AND OSMIUM NUCLEI G.D. Dracoulis. Department of Nuclear Physics, Research SchooZ of PhysicaZ Sciences, Australian National University, P. 0. Box 4, A. C. T. Canberrra, Australia. Abstract.- Rotation aligned negative parity sidebands have been observed in the light Tungsten and Osmium isotopes. The development from octupole bands to aligned 2-quasiparticle bands is discussed. The hghproton and i13/2 neutron are the likely configurations causing the alignment. Backbending observed in the odd spin negative parity sidebands in lEOOs suggests that both proton and neutron configurations are involved at high spin. -
Zinc Isotope Composition of the Earth and Its Behaviour During Planetary Accretion Paolo Sossi, Oliver Nebel, Hugh St.C
Zinc isotope composition of the Earth and its behaviour during planetary accretion Paolo Sossi, Oliver Nebel, Hugh St.C. O’Neill, Frédéric Moynier To cite this version: Paolo Sossi, Oliver Nebel, Hugh St.C. O’Neill, Frédéric Moynier. Zinc isotope composition of the Earth and its behaviour during planetary accretion. Chemical Geology, Elsevier, 2018, 477, pp.73-84. 10.1016/j.chemgeo.2017.12.006. insu-02917173 HAL Id: insu-02917173 https://hal-insu.archives-ouvertes.fr/insu-02917173 Submitted on 19 Aug 2020 HAL is a multi-disciplinary open access L’archive ouverte pluridisciplinaire HAL, est archive for the deposit and dissemination of sci- destinée au dépôt et à la diffusion de documents entific research documents, whether they are pub- scientifiques de niveau recherche, publiés ou non, lished or not. The documents may come from émanant des établissements d’enseignement et de teaching and research institutions in France or recherche français ou étrangers, des laboratoires abroad, or from public or private research centers. publics ou privés. Accepted Manuscript Zinc isotope composition of the Earth and its behaviour during planetary accretion Paolo A. Sossi, Oliver Nebel, Hugh St.C. O'Neill, Frédéric Moynier PII: S0009-2541(17)30678-2 DOI: https://doi.org/10.1016/j.chemgeo.2017.12.006 Reference: CHEMGE 18577 To appear in: Chemical Geology Received date: 22 September 2017 Revised date: 6 December 2017 Accepted date: 8 December 2017 Please cite this article as: Paolo A. Sossi, Oliver Nebel, Hugh St.C. O'Neill, Frédéric Moynier , Zinc isotope composition of the Earth and its behaviour during planetary accretion. -
Accelerator-Based Production of High Specific Activity Radionuclides for Radiopharmaceutical Applications
ACCELERATOR-BASED PRODUCTION OF HIGH SPECIFIC ACTIVITY RADIONUCLIDES FOR RADIOPHARMACEUTICAL APPLICATIONS A Dissertation Presented to the Faculty of the Graduate School at the University of Missouri-Columbia In Partial Fulfillment of the Requirements for the Degree Doctor of Philosophy By MATTHEW DAVID GOTT Dr. Silvia S. Jurisson, Dissertation Advisor Dr. Cathy S. Cutler, Co-Advisor JULY 2015 The undersigned, appointed by the dean of the Graduate School, have examined the dissertation entitled ACCELERATOR-BASED PRODUCTION OF HIGH SPECIFIC ACTIVITY RADIONUCLIDES FOR RADIOPHARMACEUTICAL APPLICATIONS presented by Matthew David Gott, a candidate for the degree of Doctor of Philosophy, and hereby certify that, in their opinion, it is worthy of acceptance. Dr. Silvia S. Jurisson Dr. Cathy S. Cutler Dr. C. Michael Greenlief Dr. J. David Robertson DEDICATION This dissertation is dedicated to my wonderful parents, David and Cathy. You have always been my greatest supporters and encouraged me every step of the way. None of this would have been possible without you. ACKNOWLEDGMENTS I would like to thank Dr. C. Michael Greenlief and Dr. J. David Roberston for serving on my committee and providing advice throughout this process. I would like to thank all of my collaborators who provided assistance and guidance throughout this project. Dr. Donald Wycoff, Dr. Anthony Degraffenreid, and Yutian Feng were instrumental in the arsenic production work. Dr. Alan Ketring, Dr. John Lydon, Mary Embree, Stacy Wilder, Alex Saale, Melissa Evans-Blumer, and the staff at the University of Missouri Research Reactor provided support and ideas for experimental work throughout this dissertation. Dr. Michael Fassbender, Dr. Beau Ballard, and the members of the C-IIAC group at Los Alamos National Laboratory provided assistance and guidance with the experimental work for the W/Re separation method.