Determination of the Isotopic Composition of Gadolinium Using
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(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. -
Discovery of Samarium, Europium, Gadolinium, and Terbium Isotopes
Discovery of Samarium, Europium, Gadolinium, and Terbium Isotopes E. May, M. Thoennessen∗ National Superconducting Cyclotron Laboratory and Department of Physics and Astronomy, Michigan State University, East Lansing, MI 48824, USA Abstract Currently, thirty-four samarium, thirty-four europium, thirty-one gadolinium, and thirty-one terbium isotopes have been observed and the discovery of these isotopes is discussed here. For each isotope a brief synopsis of the first refereed publication, including the production and identification method, is presented. arXiv:1201.4159v1 [nucl-ex] 19 Jan 2012 ∗Corresponding author. Email address: [email protected] (M. Thoennessen) Preprint submitted to Atomic Data and Nuclear Data Tables October 21, 2018 Contents 1. Introduction . 2 2. Discovery of 129−162Sm ................................................................................. 3 3. Discovery of 130−165Eu.................................................................................. 10 4. Discovery of 135−166Gd ................................................................................. 18 5. Discovery of 135−168Tb ................................................................................. 26 6. Summary ............................................................................................. 34 References . 34 Explanation of Tables . 41 7. Table 1. Discovery of samarium, europium, gadolinium, and terbium isotopes . 41 Table 1. Discovery of samarium, europium, gadolinium, and terbium isotopes. See page 41 for Explanation -
Neutron Capture Measurements and Resonance Parameters of Gadolinium
NUCLEAR SCIENCE AND ENGINEERING: 180, 86–116 (2015) Neutron Capture Measurements and Resonance Parameters of Gadolinium Y.-R. Kang and M. W. Lee Dongnam Institute of Radiological and Medical Sciences, Research Center Busan 619-953, Korea G. N. Kim* Kyungpook National University, Department of Physics Daegu 702-701, Korea T.-I. Ro Dong-A University, Department of Physics Busan 604-714, Korea Y. Danon and D. Williams Rensselaer Polytechnic Institute, Department of Mechanical, Aerospace, and Nuclear Engineering Troy, New York 12180-3590 and G. Leinweber, R. C. Block, D. P. Barry, and M. J. Rapp Bechtel Marine Propulsion Corporation, Knolls Atomic Power Laboratory P.O. Box 1072, Schenectady, New York 12301 Received June 6, 2014 Accepted July 15, 2014 http://dx.doi.org/10.13182/NSE14-80 Abstract – Neutron capture measurements were performed with the time-of-flight method at the Gaerttner LINAC Center at Rensselaer Polytechnic Institute (RPI) using isotopically enriched gadolinium (Gd) samples (155Gd, 156Gd, 157Gd, 158Gd, and 160Gd). The neutron capture measurements were made at the 25-m flight station with a 16-segment sodium iodide multiplicity detector. After the data were collected and reduced to capture yields, resonance parameters were obtained by a combined fitting of the neutron capture data for five enriched Gd isotopes and one natural Gd sample using the multilevel R-matrix Bayesian code SAMMY. A table of resonance parameters and their uncertainties is presented. We observed 2, 169, 96, and 1 new resonances in 154Gd, 155Gd, 157Gd, and 158Gd isotopes, respectively. Resonances in the ENDF/B-VII.0 evaluation that were not observed in the current experiment and could not be traced to a literature reference were removed. -
CROSS SECTIONS of (N,P), (N,Α), (N,2N) REACTIONS on ISOTOPES
CROSS SECTIONS OF (n, p), (n, α), (n, 2n) REACTIONS ON ISOTOPES OF Dy, Er, Yb AT En= 14.6 MEV А.O. Kadenko, O.M. Gorbachenko, V.A. Plujko, G.I. Primenko Nuclear Physics Department, Taras Shevchenko National University, Kyiv, Ukraine Abstract The cross sections of the neutron reactions at En= 14.6 MeV on the isotopes of Dy, Er, Yb with emission of neutrons, proton and alpha-particle were studied by the use of new experimental data and different theoretical approaches. New and improved experimental data were obtained by the neutron- activation technique. Present experimental results and evaluated nuclear data from EXFOR, TENDL, ENDF data libraries were compared with different systematics and calculations within codes of EMPIRE 3.0 and TALYS 1.2. Contribution of pre-equilibrium decay was studied. The recommendations on validity of different systematics for estimations of cross-sections of considered reactions are given. 1. Introduction Studies of the nuclear reaction cross sections induced by neutrons provides an opportunity to get information on the excited states of atomic nuclei and nuclear reaction mechanisms [1]. In addition, nuclear reaction cross section data are necessary in applied applications such as the design of fusion reactors protection and modernization of existing nuclear power plants [2, 3]. In particular, they allow to calculate the activity and the degree of radiation damage to structural elements of nuclear reactors [3]. Practical interest in cross sections of nuclear reactions caused by their wide use in experimental nuclear physics methods, such as the method of boundary indicators in measuring the spectrum of neutrons in the reactor core of a nuclear reactor, or neutron activation analysis. -
The Elements.Pdf
A Periodic Table of the Elements at Los Alamos National Laboratory Los Alamos National Laboratory's Chemistry Division Presents Periodic Table of the Elements A Resource for Elementary, Middle School, and High School Students Click an element for more information: Group** Period 1 18 IA VIIIA 1A 8A 1 2 13 14 15 16 17 2 1 H IIA IIIA IVA VA VIAVIIA He 1.008 2A 3A 4A 5A 6A 7A 4.003 3 4 5 6 7 8 9 10 2 Li Be B C N O F Ne 6.941 9.012 10.81 12.01 14.01 16.00 19.00 20.18 11 12 3 4 5 6 7 8 9 10 11 12 13 14 15 16 17 18 3 Na Mg IIIB IVB VB VIB VIIB ------- VIII IB IIB Al Si P S Cl Ar 22.99 24.31 3B 4B 5B 6B 7B ------- 1B 2B 26.98 28.09 30.97 32.07 35.45 39.95 ------- 8 ------- 19 20 21 22 23 24 25 26 27 28 29 30 31 32 33 34 35 36 4 K Ca Sc Ti V Cr Mn Fe Co Ni Cu Zn Ga Ge As Se Br Kr 39.10 40.08 44.96 47.88 50.94 52.00 54.94 55.85 58.47 58.69 63.55 65.39 69.72 72.59 74.92 78.96 79.90 83.80 37 38 39 40 41 42 43 44 45 46 47 48 49 50 51 52 53 54 5 Rb Sr Y Zr NbMo Tc Ru Rh PdAgCd In Sn Sb Te I Xe 85.47 87.62 88.91 91.22 92.91 95.94 (98) 101.1 102.9 106.4 107.9 112.4 114.8 118.7 121.8 127.6 126.9 131.3 55 56 57 72 73 74 75 76 77 78 79 80 81 82 83 84 85 86 6 Cs Ba La* Hf Ta W Re Os Ir Pt AuHg Tl Pb Bi Po At Rn 132.9 137.3 138.9 178.5 180.9 183.9 186.2 190.2 190.2 195.1 197.0 200.5 204.4 207.2 209.0 (210) (210) (222) 87 88 89 104 105 106 107 108 109 110 111 112 114 116 118 7 Fr Ra Ac~RfDb Sg Bh Hs Mt --- --- --- --- --- --- (223) (226) (227) (257) (260) (263) (262) (265) (266) () () () () () () http://pearl1.lanl.gov/periodic/ (1 of 3) [5/17/2001 4:06:20 PM] A Periodic Table of the Elements at Los Alamos National Laboratory 58 59 60 61 62 63 64 65 66 67 68 69 70 71 Lanthanide Series* Ce Pr NdPmSm Eu Gd TbDyHo Er TmYbLu 140.1 140.9 144.2 (147) 150.4 152.0 157.3 158.9 162.5 164.9 167.3 168.9 173.0 175.0 90 91 92 93 94 95 96 97 98 99 100 101 102 103 Actinide Series~ Th Pa U Np Pu AmCmBk Cf Es FmMdNo Lr 232.0 (231) (238) (237) (242) (243) (247) (247) (249) (254) (253) (256) (254) (257) ** Groups are noted by 3 notation conventions. -
Periodic Table of Elements
The origin of the elements – Dr. Ille C. Gebeshuber, www.ille.com – Vienna, March 2007 The origin of the elements Univ.-Ass. Dipl.-Ing. Dr. techn. Ille C. Gebeshuber Institut für Allgemeine Physik Technische Universität Wien Wiedner Hauptstrasse 8-10/134 1040 Wien Tel. +43 1 58801 13436 FAX: +43 1 58801 13499 Internet: http://www.ille.com/ © 2007 © Photographs of the elements: Mag. Jürgen Bauer, http://www.smart-elements.com 1 The origin of the elements – Dr. Ille C. Gebeshuber, www.ille.com – Vienna, March 2007 I. The Periodic table............................................................................................................... 5 Arrangement........................................................................................................................... 5 Periodicity of chemical properties.......................................................................................... 6 Groups and periods............................................................................................................. 6 Periodic trends of groups.................................................................................................... 6 Periodic trends of periods................................................................................................... 7 Examples ................................................................................................................................ 7 Noble gases ....................................................................................................................... -
Dynamics of Population of Gadolinium-156 Nuclei Energy Levels During Neutron Pumping of Isotope-Modified Gadolinium Oxide
Dynamics of population of gadolinium-156 nuclei energy levels during neutron pumping of isotope-modified gadolinium oxide Igor V. Shamanina, Mishik A. Kazaryanb, Sergei V. Bedenkoa, Vladimir.V. Knysheva, Vitaly I. Shamanina a National research Tomsk polytechnic university, prospekt Lenina, 30, 634050, Tomsk, Russia; b Physical institute RAS, Leninsky prospekt, 53, 119991, Moscow, Russia ABSTRACT The possibility of transformation of energy of fast and epithermal neutrons to energy of coherent photon radiation at the expense of a neutron pumping of the active medium formed by nucleus with long-living isomerous states is theoretically described. The channel of the nucleus formation in isomeric state as a daughter nucleus resulting from the nuclear reaction of neutron capture by a lighter nucleus is taken into consideration for the first time. The analysis of cross sections dependence of radiative neutron capture by the nuclei of gadolinium isotopes Gd155 and Gd156 is performed. As a result, it is stated that the speed of Gd156 nuclei formation exceeds the speed of their “burnup” in the neutron flux. It is provided by a unique combination of absorbing properties of two isotopes of gadolinium Gd155 and Gd156 in both thermal and resonance regions of neutron energy. The possibility of excess energy accumulation in the participating medium created by the nuclei of the pair of gadolinium isotopes Gd155 and Gd156 due to formation and storage of nuclei in isomeric state at radiative neutron capture by the nuclei of the stable isotope with a smaller mass is shown. It is concluded that when the active medium created by gadolinium nuclei is pumped by neutrons with the flux density of the order of 1013 cm-2·s-1, the condition of levels population inversion can be achieved in a few tens of seconds. -
The Radioactivity of Some Ruthenium and Erbium
THE RADIOACTIVITY OF SOME RUTHENIUM AND ERBIUM ISOTOPES DISSERTATION Presented in Partial Fulfillment of the Requirements for the Degree Doctor of Philosophy in the Graduate School of The Ohio State University By BASANT LAL SHARMA, B. Sc., M. Sc. The Ohio State University 1959 Approved by: " - y n - L . t o J Z ------------------ x a s i s e r ----------^ -------- Department of Physics and Astronomy Acknowledgm ent I take this opportunity to express my sincere appreciation to Professor M. L. Pool for his interest, suggestions, and encouragement throughout this work. Table of Contents Page General Introduction ................................................................................................. 1 Instrumentation ................................................................................................................................ PART I RADIOACTIVE DECAY OF Ru106 AND THE ESTIMATION OF THE THERMAL NEUTRON ACTIVATION CROSS SECTION OF Ru105 Introduction........................................................................................................................................... 8 Experimental D ata............................................................................................. 11 Calculation of the Thermal Neutron Activation Cross Section of R u ^ ^.....................................................................................................23 Results and Discussion............................................................................................... 28 Bibliography ........................................... -
First Search for $2\Varepsilon $ and $\Varepsilon\Beta^+ $ Decay Of
First search for 2ε and εβ+ decay of 162Er and new limit on 2β− decay of 170Er to the first excited level of 170Yb P. Bellia, R. Bernabeia,b,1, R.S. Boikoc,d, F. Cappellae, V. Caracciolof , R. Cerullia, F.A. Danevichc, A. Incicchittie,g, B.N. Kropivyanskyc, M. Laubensteinf , S. Nisif , D.V. Podac,h, O.G. Polischukc, V.I. Tretyakc aINFN sezione Roma “Tor Vergata”, I-00133 Rome, Italy bDipartimento di Fisica, Universita` di Roma “Tor Vergata”, I-00133 Rome, Italy cInstitute for Nuclear Research, 03028 Kyiv, Ukraine dNational University of Life and Environmental Sciences of Ukraine, 03041 Kyiv, Ukraine eINFN sezione Roma, I-00185 Rome, Italy f INFN, Laboratori Nazionali del Gran Sasso, I-67100 Assergi (AQ), Italy gDipartimento di Fisica, Universita` di Roma “La Sapienza”, I-00185 Rome, Italy hCSNSM, Universit´eParis-Sud, CNRS/IN2P3, Universit´eParis-Saclay, 91405 Orsay, France Abstract The first search for double electron capture (2ε) and electron cap- arXiv:1808.01782v1 [nucl-ex] 6 Aug 2018 ture with positron emission (εβ+) of 162Er to the ground state and to several excited levels of 162Dy was realized with 326 g of highly purified erbium oxide. The sample was measured over 1934 h by the ultra-low background HP Ge γ spectrometer GeCris (465 cm3) at the Gran Sasso underground laboratory. No effect was observed, the half- 15 18 life limits were estimated at the level of lim T1/2 ∼ 10 − 10 yr. A 162 + possible resonant 0νKL1 capture in Er to the 2 1782.7 keV ex- 162 17 cited state of Dy is restricted as T1/2 ≥ 5.0 × 10 yr at 90% C.L. -
United States Patent 19 11 Patent Number: 5,437,795 Snyder Et Al
US005437795A United States Patent 19 11 Patent Number: 5,437,795 Snyder et al. 45) Date of Patent: Aug. 1, 1995 (54) CHROMATOGRAPHIC SEPARATION OF 5,098,678 3/1992 Lee et al. .............................. 423/70 ERBUMISOTOPES 5,110,566 5/1992 Snyder et al. ......................... 423/70 5,124,023 6/1992 Bosserman . 210/659 (75) Inventors: Thomas S. Snyder, Oakmont; Steven 5,133,869 7/1992 Taniguchi. 210/659 H. Peterson; Umesh P. Nayak, both 5,174,971 12/1992 Snyder et al.......................... 423/70 of Murrysville; Richard J. Beleski, Pittsburgh, all of Pa. Primary Examiner-Ernest G. Therkorn 57 ABSTRACT 73 Assignee: Westinghouse Electric Corporation, Pittsburgh, Pa. A process for the partial or complete simultaneous sepa ration of isotopes of erbium, especially high thermal (21) Appl. No.: 264,810 neutron capture cross-section erbium isotopes, using 22 Filed: Jun. 23, 1994 continuous, steady-state, chromatography in which an (51) Int. Cl............................................... B01D 15/08 ion exchange resin is the stationary phase, an aqueous (52) U.S.C. .................................... 210/635; 210/656; solution of ions based on a mixture of erbium isotopes is 210/657; 210/659; 210/1982; 423/21.5; the feed phase, and an aqueous acid eluant solution is 423/263 the mobile phase. The process involves the mobile (58) Field of Search ............... 210/635,656,657, 659, phase eluting or desorbing the erbium isotopic solute 210/1982; 423/263, 21.1, 21.5 adsorbed on the stationary phase under conditions such that each of the various naturally occurring isotopes of (56) References Cited erbium is primarily eluted in an elution volume distinct U.S. -
Optimization of Transcurium Isotope Production in the High Flux Isotope Reactor
University of Tennessee, Knoxville TRACE: Tennessee Research and Creative Exchange Doctoral Dissertations Graduate School 12-2012 Optimization of Transcurium Isotope Production in the High Flux Isotope Reactor Susan Hogle [email protected] Follow this and additional works at: https://trace.tennessee.edu/utk_graddiss Part of the Nuclear Engineering Commons Recommended Citation Hogle, Susan, "Optimization of Transcurium Isotope Production in the High Flux Isotope Reactor. " PhD diss., University of Tennessee, 2012. https://trace.tennessee.edu/utk_graddiss/1529 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 Susan Hogle entitled "Optimization of Transcurium Isotope Production in the High Flux Isotope Reactor." 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 Nuclear Engineering. G. Ivan Maldonado, Major Professor We have read this dissertation and recommend its acceptance: Lawrence Heilbronn, Howard Hall, Robert Grzywacz 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.) Optimization of Transcurium Isotope Production in the High Flux Isotope Reactor A Dissertation Presented for the Doctor of Philosophy Degree The University of Tennessee, Knoxville Susan Hogle December 2012 © Susan Hogle 2012 All Rights Reserved ii Dedication To my father Hubert, who always made me feel like I could succeed and my mother Anne, who would always love me even if I didn’t. -
Modern Physics
REVIEWS OF MODERN PHYSICS VoLUME 29, NuMBER 4 OcroBER, 1957 Synthesis of the Elements in Stars* E. MARGARET BURBIDGE, G. R. BURBIDGE, WILLIAM: A. FOWLER, AND F. HOYLE Kellogg Radiation1Laboratory, California Institute of Technology, and M aunt Wilson and Palomar Observatories, Carnegie Institution of Washington, California Institute of Technology, Pasadena, California "It is the stars, The stars above us, govern our conditions"; (King Lear, Act IV, Scene 3) but perhaps "The fault, dear Brutus, is not in our stars, But in ourselves," (Julius Caesar, Act I, Scene 2) TABLE OF CONTENTS Page I. Introduction ...............................................................· ............... 548 A. Element Abundances and Nuclear Structure. 548 B. Four Theories of the Origin of the Elements ............................................... 550 C. General Features of Stellar Synthesis ..................................................... 550 II. Physical Processes Involved in Stellar Synthesis, Their Place of Occurrence, and the Time-Scales Associated with Them ...............· ..................... · ................................. 551 A. Modes of Element Synthesis ............................................................. 551 B. Method of Assignment of Isotopes among Processes (i) to (viii) .............................. 553 C. Abundances and Synthesis Assignments Given in the Appendix. 555 D. Time-Scales for Different Modes of Synthesis .............................................. 556 III. Hydrogen Burning, Helium Burning, the a Process,