Spallation Neutron Sources for Science and Technology
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Resolution Neutron Scattering Technique Using Triple-Axis
1 High -resolution neutron scattering technique using triple-axis spectrometers ¢ ¡ ¡ GUANGYONG XU, ¡ * P. M. GEHRING, V. J. GHOSH AND G. SHIRANE ¢ ¡ Physics Department, Brookhaven National Laboratory, Upton, NY 11973, and NCNR, National Institute of Standards and Technology, Gaithersburg, Maryland, 20899. E-mail: [email protected] (Received 0 XXXXXXX 0000; accepted 0 XXXXXXX 0000) Abstract We present a new technique which brings a substantial increase of the wave-vector £ - resolution of triple-axis-spectrometers by matching the measurement wave-vector £ to the ¥§¦©¨ reflection ¤ of a perfect crystal analyzer. A relative Bragg width of can be ¡ achieved with reasonable collimation settings. This technique is very useful in measuring small structural changes and line broadenings that can not be accurately measured with con- ventional set-ups, while still keeping all the strengths of a triple-axis-spectrometer. 1. Introduction Triple-axis-spectrometers (TAS) are widely used in both elastic and inelastic neutron scat- tering measurements to study the structures and dynamics in condensed matter. It has the £ flexibility to allow one to probe nearly all coordinates in energy ( ) and momentum ( ) space in a controlled manner, and the data can be easily interpreted (Bacon, 1975; Shirane et al., 2002). The resolution of a triple-axis-spectrometer is determined by many factors, including the ¨ incident (E ) and final (E ) neutron energies, the wave-vector transfer , the monochromator PREPRINT: Acta Crystallographica Section A A Journal of the International Union of Crystallography 2 and analyzer mosaic, and the beam collimations, etc. This has been studied in detail by Cooper & Nathans (1967), Werner & Pynn (1971) and Chesser & Axe (1973). -
Neutron Scattering
Neutron Scattering John R.D. Copley Summer School on Methods and Applications of High Resolution Neutron Spectroscopy and Small Angle Neutron Scattering NIST Center for NeutronNCNR Summer Research, School 2011 June 12-16, 2011 Acknowledgements National Science Foundation NIST Center for Neutron (grant # DMR-0944772) Research (NCNR) Center for High Resolution Neutron Scattering (CHRNS) 2 NCNR Summer School 2011 (Slow) neutron interactions Scattering plus Absorption Total =+Elastic Inelastic scattering scattering scattering (diffraction) (spectroscopy) includes “Quasielastic neutron Structure Dynamics scattering” (QENS) NCNR Summer School 2011 3 Total, elastic, and inelastic scattering Incident energy Ei E= Ei -Ef Scattered energy Ef (“energy transfer”) Total scattering: Elastic scattering: E = E (i.e., E = 0) all Ef (i.e., all E) f i Inelastic scattering: E ≠ E (i.e., E ≠ 0) D f i A M M Ef Ei S Ei D S Diffractometer Spectrometer (Some write E = Ef –Ei) NCNR Summer School 2011 4 Kinematics mv= = k 1 222 Emvk2m==2 = Scattered wave (m is neutron’s mass) vector k , energy E 2θ f f Incident wave vector ki, energy Ei N.B. The symbol for scattering angle in Q is wave vector transfer, SANS experiments is or “scattering vector” Q =Q is momentum transfer θ, not 2θ. Q = ki - kf (For x-rays, Eck = = ) (“wave vector transfer”) NCNR Summer School 2011 5 Elastic scattering Q = ki - kf G In real space k In reciprocal space f G G G kf Q ki 2θ 2θ G G k Q i E== 0 kif k Q =θ 2k i sin NCNR Summer School 2011 6 Total scattering, inelastic scattering Q = ki - kf G kf G Q Qkk2kkcos2222= +− θ 2θ G if if ki At fixed scattering angle 2θ, the magnitude (and the direction) of Q varies with the energy transfer E. -
Neutron Scattering
Neutron Scattering Basic properties of neutron and electron neutron electron −27 −31 mass mkn =×1.675 10 g mke =×9.109 10 g charge 0 e spin s = ½ s = ½ −e= −e= magnetic dipole moment µnn= gs with gn = 3.826 µee= gs with ge = 2.0 2mn 2me =22k 2π =22k Ek== E = 2m λ 2m energy n e 81.81 150.26 Em[]eV = 2 Ee[]V = 2 λ ⎣⎡Å⎦⎤ λ ⎣⎦⎡⎤Å interaction with matter: Coulomb interaction — 9 strong-force interaction 9 — magnetic dipole-dipole 9 9 interaction Several salient features are apparent from this table: – electrons are charged and experience strong, long-range Coulomb interactions in a solid. They therefore typically only penetrate a few atomic layers into the solid. Electron scattering is therefore a surface-sensitive probe. Neutrons are uncharged and do not experience Coulomb interaction. The strong-force interaction is naturally strong but very short-range, and the magnetic interaction is long-range but weak. Neutrons therefore penetrate deeply into most materials, so that neutron scattering is a bulk probe. – Electrons with wavelengths comparable to interatomic distances (λ ~2Å ) have energies of several tens of electron volts, comparable to energies of plasmons and interband transitions in solids. Electron scattering is therefore well suited as a probe of these high-energy excitations. Neutrons with λ ~2Å have energies of several tens of meV , comparable to the thermal energies kTB at room temperature. These so-called “thermal neutrons” are excellent probes of low-energy excitations such as lattice vibrations and spin waves with energies in the meV range. -
Fusion and Spallation Irradiation Conditions Steven J
Fusion and Spallation Irradiation Conditions Steven J. Zinkle Metals and Ceramics Division Oak Ridge National Laboratory, Oak Ridge, TN International Workshop on Advanced Computational Science: Application to Fusion and Generation-IV Fission Reactors Washington DC, March 31-April 2, 2004 Comparison of fission and fusion (ITER) neutron spectra Stoller & Greenwood, JNM 271-272 (1999) 57 • Main difference between fission and DT fusion neutron spectra is the presence of significant flux above ~4 MeV for fusion –High energy neutrons typically cause enhanced production of numerous transmutation products including H and He –The Primary Knock-on Atom (PKA) spectra are similar for fission and fusion at low energies; fusion contains significant high-energy PKAs (>100 keV) Displacement Damage Mechanisms are being investigated with Molecular Dynamics Simulations Damage efficiency saturates when subcascade formation occurs Avg. Avg. fission fusion Molecular dynamics modeling of displacement cascades up to 50 keV PKA 200 keV and low-dose experimental tests (microstructure, tensile (ave. fusion) properties, etc.) indicates that defect production from fusion and fission neutron collisions are similar 10 keV PKA => Defect source term is similar for fission and fusion conditions (ave. fission) Peak damage state in iron cascades at 100K 5 nm A critical unanswered question is the effect of higher transmutant H and He production in the fusion spectrum Radiation Damage can Produce Large Changes in Structural Materials • Radiation hardening and embrittlement -
Single Crystal Diffuse Neutron Scattering
Review Single Crystal Diffuse Neutron Scattering Richard Welberry 1,* ID and Ross Whitfield 2 ID 1 Research School of Chemistry, Australian National University, Canberra, ACT 2601, Australia 2 Neutron Scattering Division, Oak Ridge National Laboratory, Oak Ridge, TN 37831, USA; whitfi[email protected] * Correspondence: [email protected]; Tel.: +61-2-6125-4122 Received: 30 November 2017; Accepted: 8 January 2018; Published: 11 January 2018 Abstract: Diffuse neutron scattering has become a valuable tool for investigating local structure in materials ranging from organic molecular crystals containing only light atoms to piezo-ceramics that frequently contain heavy elements. Although neutron sources will never be able to compete with X-rays in terms of the available flux the special properties of neutrons, viz. the ability to explore inelastic scattering events, the fact that scattering lengths do not vary systematically with atomic number and their ability to scatter from magnetic moments, provides strong motivation for developing neutron diffuse scattering methods. In this paper, we compare three different instruments that have been used by us to collect neutron diffuse scattering data. Two of these are on a spallation source and one on a reactor source. Keywords: single crystal; diffuse scattering; neutrons; spallation source; time-of-flight 1. Introduction Bragg scattering, which is used in conventional crystallography, gives only information about the average crystal structure. Diffuse scattering from single crystals, on the other hand, is a prime source of local structural information. There is now a wealth of evidence to show that the more local structure is investigated the more we are obliged to reassess our understanding of crystalline structure and behaviour [1]. -
NUCLIDES FAR OFF the STABILITY LINE and SUPER-HEAVY NUCLEI in HEAVY-ION NUCLEAR REACTIONS Marc Lefort
NUCLIDES FAR OFF THE STABILITY LINE AND SUPER-HEAVY NUCLEI IN HEAVY-ION NUCLEAR REACTIONS Marc Lefort To cite this version: Marc Lefort. NUCLIDES FAR OFF THE STABILITY LINE AND SUPER-HEAVY NUCLEI IN HEAVY-ION NUCLEAR REACTIONS. Journal de Physique Colloques, 1972, 33 (C5), pp.C5-73-C5- 102. 10.1051/jphyscol:1972507. jpa-00215109 HAL Id: jpa-00215109 https://hal.archives-ouvertes.fr/jpa-00215109 Submitted on 1 Jan 1972 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 RE PHYSIQUE CoLIoque C5, supplement au no 8-9, Tome 33, Aoiit-Septembre 1972, page C5-73 NUCLIDES FAR OFF THE STABILITY LINE AND SUPER-HEAVY NUCLEI IN HEAW-ION NUCLEAR REACTIONS by Marc Lefort Chimie Nucleaire-Institut de Physique Nucleaire-ORSAY, France Abstract A review is given on the new species which attempts already made for the synthesis of super- have been produced in the recent years by heavy ion heavy elements. A discussion is presented on the reactions, mainly 12C, 160, ''0, 22~eand 20~eions. following problems : reaction thresholds and The first section is devoted to the formation of coulomb barriers for heavily charged projectiles, neutron rich exotic light nuclei and to the mecha- complete fusion cross section as compared to the nism of multinuclear transfer reactions responsible total cross section, main decay channels for exci- for this formation. -
Basics of Neutron Scattering
Part I Basics of neutron scattering 13 Chapter 1 Introduction to neutron scattering Neutron scattering is one of the most powerful and versatile experimental meth- ods to study the structure and dynamics of materials on the atomic and nanome- ter scale. Quoting the Nobel committee, when awarding the prize to C. Shull and B. Brockhouse in 1994, these pioneers have “helped answer the question of where atoms are and ... the question of what atoms do” [4]. Neutron scattering is presently used by more than 5000 researchers world- wide, and the scope of the method is continuously broadening. In the 1950’ies and 1960’ies, neutron scattering was an exotic tool in Solid State Physics and Chemical Crystallography, but today it serves communities as diverse as Biol- ogy, Earth Sciences, Planetary Science, Engineering, Polymer Chemistry, and Cultural Heritage. In brief, neutrons are used in all scientific fields that deal with hard, soft, or biological materials. It is, however, appropriate to issue a warning already here. Although neu- tron scattering is a great technique, it is also time-consuming and expensive. Neutron scattering experiments last from hours to days and are performed at large international facilities. Here, the running costs correspond to several thou- sand Euros per instrument day. Hence, neutron scattering should be used only where other methods are inadequate. For the study of atomic and nanometer-scale structure in materials, X-ray scattering is the technique of choice. X-ray sources are by far more abundant and are, especially for synchrotron X-ray sources, much stronger than neutron sources. Hence, the rule of thumb goes: “If an experiment can be performed with X-rays, use X-rays”. -
Opportunities and Challenges in Neutron Crystallography
EPJ Web of Conferences 236, 02001 (2020) https://doi.org/10.1051/epjconf/202023602001 JDN 24 Opportunities and challenges in neutron crystallography Nathan Richard Zaccai1,*, and Nicolas Coquelle2,† 1CIMR, University of Cambridge, Cambridge CB2 0XY, United Kingdom 2Institut Laue Langevin, 38042 Grenoble Cedex 9, France Abstract. Neutron and X-ray crystallography are complementary to each other. While X-ray scattering is directly proportional to the number of electrons of an atom, neutrons interact with the atomic nuclei themselves. Neutron crystallography therefore provides an excellent alternative in determining the positions of hydrogens in a biological molecule. In particular, since highly polarized hydrogen atoms (H+) do not have electrons, they cannot be observed by X-rays. Neutron crystallography has its own limitations, mainly due to inherent low flux of neutrons sources, and as a consequence, the need for much larger crystals and for different data collection and analysis strategies. These technical challenges can however be overcome to yield crucial structural insights about protonation states in enzyme catalysis, ligand recognition, as well as the presence of unusual hydrogen bonds in proteins. 1 Introduction Although X-ray crystallography has become the workhorse of structural biology, Neutron crystallography has several advantages to offer in the structural analysis of biological molecules. X-rays and neutrons interact differently with matter in general, and with biological macromolecules in particular. These two crystallography approaches are therefore complementary to each other [1]. While X-ray scattering is directly proportional to the number of electrons of an atom, neutrons interact with the atomic nuclei themselves. In this perspective, hydrogen atoms, which represent ~50% of the atomistic composition of proteins and DNA, are hardly visible using X-ray crystallography, while they can be observed in nuclear density maps derived from neutron diffraction data even at moderate resolution (2.5Å and higher). -
Synthesis of Neutron-Rich Transuranic Nuclei in Fissile Spallation Targets
Synthesis of neutron-rich transuranic nuclei in fissile spallation targets Igor Mishustina,b, Yury Malyshkina,c, Igor Pshenichnova,c, Walter Greinera aFrankfurt Institute for Advanced Studies, J.-W. Goethe University, 60438 Frankfurt am Main, Germany b“Kurchatov Institute”, National Research Center, 123182 Moscow, Russia cInstitute for Nuclear Research, Russian Academy of Science, 117312 Moscow, Russia Abstract A possibility of synthesizing neutron-reach super-heavy elements in spal- lation targets of Accelerator Driven Systems (ADS) is considered. A dedi- cated software called Nuclide Composition Dynamics (NuCoD) was developed to model the evolution of isotope composition in the targets during a long-time irradiation by intense proton and deuteron beams. Simulation results show that transuranic elements up to 249Bk can be produced in multiple neutron capture reactions in macroscopic quantities. However, the neutron flux achievable in a spallation target is still insufficient to overcome the so-called fermium gap. Fur- ther optimization of the target design, in particular, by including moderating material and covering it by a reflector will turn ADS into an alternative source of transuranic elements in addition to nuclear fission reactors. 1. Introduction Neutrons propagating in a medium induce different types of nuclear reactions depending on their energy. Apart of the elastic scattering, the main reaction types for low-energy neutrons are fission and neutron capture, which dominate, respectively, at higher and lower energies with the boarder -
Status of the Project and Physics of the Spallation Target
PHYSOR 2004 -The Physics of Fuel Cycles and Advanced Nuclear Systems: Global Developments Chicago, Illinois, April 25-29, 2004, on CD-ROM, American Nuclear Society, Lagrange Park, IL. (2004) The TRADE Experiment: Status of the Project and Physics of the Spallation Target C. Rubbia1, P. Agostini1, M. Carta1, S. Monti1, M. Palomba1, F. Pisacane1, C. Krakowiak2, M. Salvatores2, Y. Kadi*3, A. Herrera-Martinez3, L. Maciocco4 1ENEA, Lungotevere Thaon di Revel, 00196 Rome, ITALY 2CEA, CEN-Cadarache, 13108 Saint-Paul-Lez-Durance, FRANCE 3CERN, 1211 Geneva 23, SWITZERLAND 4AAA, 01630 Saint-Genis-Pouilly, FRANCE The neutronic characteristics of the target-core system of the TRADE facility have been established and optimized for a reference proton energy of 140 MeV. Similar simulations have been repeated for two successive upgrades of the proton energy, 200 and 300 MeV, corresponding to different performances and design requirements and different characteristics of the proposed cyclotron and, as a consequence, of the proton beam. An extensive comparison of the main physical parameters has been also carried out, in order to evaluate advantages and disadvantages of different proton beam energies in the design of the spallation target and to allow the optimal engineering design of the whole TRADE facility. KEYWORDS: TRADE facility, ADS, Spallation target physics, Experimentation, External neutron sources, intermediate proton energy. 1. Introduction The TRADE “TRiga Accelerator Driven Experiment”, to be performed in the existing TRIGA reactor of the ENEA Casaccia Centre, has been proposed as a major project in the way for validating the ADS concept. Actually, TRADE will be the first experiment in which the three main components of an ADS – the accelerator, the spallation target and the sub- critical blanket – will be coupled at a power level sufficient to appreciate feedback reactivity effects. -
Spallation and Neutron-Capture Produced Cosmogenic Nuclides in Aubrites
70th Annual Meteoritical Society Meeting (2007) 5054.pdf SPALLATION AND NEUTRON-CAPTURE PRODUCED COSMOGENIC NUCLIDES IN AUBRITES. J. Masarik1, K. Nishiizumi2 and K. C. Welten2, 1Department of Nuclear Physics, Comenius University Bratislava, Slovakia, E-mail: ma- [email protected], 2Space Sciences Laboratory, University of California, Berkeley, CA 94720, USA, Introduction: A purely physical model for the simulation of cosmic-ray-particle interactions with matter was used to investi- gate the production rates of cosmogenic nuclides in aubrites with radii ranging from 5 cm to 120 cm. Production rates of spal- logenic and neutron-capture produced nuclides were investigated and compared with measured cosmogenic nuclide concentrations to constrain the complex exposure histories of aubrites. Calculational Model: The numerical simulation of interac- tions of primary and secondary cosmic-ray particles was done with the LAHET Code System (LCS) [1] which uses MCNP [2] for transport of low energy neutrons. The investigated objects were spheres with various radii that were divided into spherical layers. We used the spectrum of the galactic-cosmic-ray particles corresponding to solar modulation parameter Φ = 550 MeV and a flux of 4.8 protons/s·cm2. The statistical errors of the LCS calcu- lated fluxes were 3–5%. The production rates of nuclides were calculated by integrating over energy the product of these fluxes and cross sections for the nuclear reactions making the investi- gated nuclide. For cross sections of spallogenic products, we relied on the values evaluated by us and tested by earlier calcula- tions [e.g., 3]. Previous calculations of the 53Mn production rate in aubrites showed good agreement with measured 53Mn concen- trations in the Norton County aubrite [4]. -
Pulsed Spallation Neutron Sources
(LoMr^** U-J / •*> =* —%3 f& APR 1 7 1938 OSTI PULSED SPALLATION NEUTRON SOURCES John M. Carpenter Intense Pulsed Neutron Source Division Argonne National Laboratory This paper reviews the early history of pulsed spallation neutron source development at Argonne and provides an overview of existing sources world wide. A number of proposals for machines more powerful than currently exist are under development, which are briefly described. I review the status of the Intense Pulsed Neutron Source, its instrumentation, and its user program, and provide a few examples of applications in fundamental condensed matter physics, materials science and technology. HISTORY OF PULSED SOURCE DEVELOPMENTS AT ARGONNE This is a day for remembering, reflecting and projecting into the future. Think back to the year 1968,26 years ago. Please don't fix upon the gathering war half a world away, the * burnings in our cities, or the riots in our own Grant Park; these were dark rumblings of political change that even now have not played out. Think instead of the scientific scene. ZGS had already been operating for five years and improvements were afoot. New, bigger machines were being designed and built around the world for high energy physics research. Several high flux research reactors were under design, construction or commissioning: HFBR (Brookhaven), HFIR (Oak Ridge), HFR (ILL Grenoble), A^R2 (Argonne), British HFR. Argonne had an already long-established tradition in neutron scattering based on its smaller research reactors, beginning with Enrico Fermi and Walter Zinn at CP-3, and continuing at the 5-MW CP-5. In January of 1968, as a young and dewy professor of Nuclear Engineering at the University of Michigan, where I had built some instruments for neutron scattering research at the 2-MW Ford Reactor, I was invited to serve in an instrument design group, led by Don Connor of the SSS division, that was supposed eventually to provide instruments for A^R2.