Spectroscopic, Thermal, and Physical Analysis of the Raw Materials in Europium Doped Cesium Strontium Iodide Scintillator
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ZEPLIN I—The UKDM Single Phase Xenon Experiment at Boulby Neil Spooner∗ Department of Physics and Astronomy University of Sheffield, Hounsfield Road, Sheffield, S3 7RH, UK
ZEPLIN I—The UKDM Single Phase Xenon Experiment at Boulby Neil Spooner∗ Department of Physics and Astronomy University of Sheffield, Hounsfield Road, Sheffield, S3 7RH, UK I briefly review the ZEPLIN I liquid xenon detector of the UKDM collaboration. 1. ZEPLIN I Detector The ZEPLIN I detector is a single phase, 3.6 kg fiducial mass, liquid xenon scintillation detector built by the UKDM Collaboration (RAL-Sheffield-ICSTM) and running at the Boulby underground site (see Figure 1). The target mass is housed in a Cu-101 copper vessel, shaped to maximise light collection, which provides a uniform temperature environment through the use of a cryo- liquid jacket. The fiducial volume of xenon is surrounded bya5mmPTFE reflector, giving diffuse scattering of the 175 nm scintillation photons to maximise light collection. This volume is viewed through 3 mm silica windows by three quartz windowed photomultipliers through optically isolated Œturrets¹ of liquid xenon. These act both as light guides and passive shielding for the X-ray emission from the photomultipliers. The novel use of the xenon turrets arose from experience with NaI detectors where solid high-grade silica is used for light guides and shields. However, the extensive use of such material for liquid xenon is precluded due to the absorption of the 175 nm photons. Scintillation light produced in the turret regions is seen predominantly by the nearest photomultiplier which allows the rejection of the photomultiplier X-ray events and the definition of a fiducial volume through a comparison of the light seen by each tube. Purification of the xenon is performed using Oxysorb ion exchange columns with additional purification by vacuum pumping on frozen xenon and subsequent fractionation of the xenon gas. -
Muon Decay 1
Muon Decay 1 LIFETIME OF THE MUON Introduction Muons are unstable particles; otherwise, they are rather like electrons but with much higher masses, approximately 105 MeV. Radioactive nuclear decays do not release enough energy to produce them; however, they are readily available in the laboratory as the dominant component of the cosmic ray flux at the earth’s surface. There are two types of muons, with opposite charge, and they decay into electrons or positrons and two neutrinos according to the rules + + µ → e νe ν¯µ − − µ → e ν¯e νµ . The muon decay is a radioactiveprocess which follows the usual exponential law for the probability of survival for a given time t. Be sure that you understand the basis for this law. The goal of the experiment is to measure the muon lifetime which is roughly 2 µs. With care you can make the measurement with an accuracy of a few percent or better. In order to achieve this goal in a conceptually simple way, we look only at those muons that happen to come to rest inside our detector. That is, we first capture a muon and then measure the elapsed time until it decays. Muons are rather penetrating particles, they can easily go through meters of concrete. Nevertheless, a small fraction of the muons will be slowed down and stopped in the detector. As shown in Figure 1, the apparatus consists of two types of detectors. There is a tank filled with liquid scintillator (a big metal box) viewed by two photomultiplier tubes (Left and Right) and two plastic scintillation counters (flat panels wrapped in black tape), each viewed by a photomul- tiplier tube (Top and Bottom). -
Strontium Iodide Radiation Instrument (SIRI) – Early On-Orbit Results Lee J
Strontium Iodide Radiation Instrument (SIRI) – Early On-Orbit Results Lee J. Mitchella, Bernard F. Phlipsa, J. Eric Grovea, Theodore Finnea, Mary Johnson-Ramberta, b W. Neil, Johnson a United States Naval Research Laboratory, 4555 Overlook Ave. S.W., Washington, DC 20375 b Praxis Inc., 251 18th Street South, Suite 610, Arlington, VA 22202 Abstract— The Strontium Iodide Radiation Instrument (SIRI) or proven components to reduce costs associated with drawing is a single detector, gamma-ray spectrometer designed to down that risk. space-qualify the new scintillation detector material europium- A number of new gamma-ray scintillation materials look doped strontium iodide (SrI2:Eu) and new silicon promising and have been proposed for space missions [1] [2] photomultiplier (SiPM) technology. SIRI covers the energy [3] [4], while silicon photomultiplier (SiPM) readout range from .04 - 8 MeV and was launched into 600 km sun- technologies are also quickly replacing traditional synchronous orbit on Dec 3, 2018 onboard STPSat-5 with a photomultiplier tubes (PMTs) in instrument concepts [5] [6] one-year mission to investigate the detector’s response to on- [7]. The goal of the Strontium Iodide Radiation Instrument orbit background radiation. The detector has an active volume (SIRI) mission is to study the performance of new SiPM of 11.6 cm3 and a photo fraction efficiency of 50% at 662 keV technology and a new scintillation material, europium-doped for gamma-rays parallel to the long axis of the crystal. Its strontium iodide (SrI2:Eu), for space-based gamma-ray spectroscopic resolution of 4.3% was measured by the full- spectrometry. -
1. Gamma-Ray Detectors for Nondestructive Analysis P
1. GAMMA-RAY DETECTORS FOR NONDESTRUCTIVE ANALYSIS P. A. Russo and D. T. Vo I. INTRODUCTION AND OVERVIEW Gamma rays are used for nondestructive quantitative analysis of nuclear material. Knowledge of both the energy of the gamma ray and its rate of emission from the unknown mass of nuclear material is required to interpret most measurements of nuclear material quantities. Therefore, detection of gamma rays for nondestructive analysis of nuclear materials requires both spectroscopy capability and knowledge of absolute specific detector response. Some techniques nondestructively quantify attributes other than nuclear material mass, but all rely on the ability to distinguish elements or isotopes and measure the relative or absolute yields of their corresponding radiation signatures. All require spectroscopy and most require high resolution. Therefore, detection of gamma rays for quantitative nondestructive analysis (NDA) of the mass or of other attributes of nuclear materials requires spectroscopy. A previous book on gamma-ray detectors for NDA1 provided generic descriptions of three detector categories: inorganic scintillation detectors, semiconductor detectors, and gas-filled detectors. This report described relevant detector properties, corresponding spectral characteristics, and guidelines for choosing detectors for NDA. The current report focuses on significant new advances in detector technology in these categories. Emphasis here is given to those detectors that have been developed at least to the stage of commercial prototypes. The type of NDA application – fixed installation in a count room, portable measurements, or fixed installation in a processing line or other active facility (storage, shipping/receiving, etc.) – influences the choice of an appropriate detector. Some prototype gamma-ray detection techniques applied to new NDA approaches may revolutionize how nuclear materials are quantified in the future. -
Scintillation Detectors for X-Rays
INSTITUTE OF PHYSICS PUBLISHING MEASUREMENT SCIENCE AND TECHNOLOGY Meas. Sci. Technol. 17 (2006) R37–R54 doi:10.1088/0957-0233/17/4/R01 REVIEW ARTICLE Scintillation detectors for x-rays Martin Nikl Institute of Physics, Academy of Sciences of the Czech Republic, Cukrovarnicka 10, 162 53 Prague, Czech Republic Received 23 March 2005 Published 10 February 2006 Online at stacks.iop.org/MST/17/R37 Abstract Recent research in the field of phosphor and scintillator materials and related detectors is reviewed. After a historical introduction the fundamental issues are explained regarding the interaction of x-ray radiation with a solid state. Crucial parameters and characteristics important for the performance of these materials in applications, including the employed measurement methods, are described. Extended description of the materials currently in use or under intense study is given. Scintillation detector configurations are further briefly overviewed and selected applications are mentioned in more detail to provide an illustration. Keywords: luminescence intensity, luminescence kinetics, light detection, x-ray detection, scintillators, phosphors, traps and material imperfections (Some figures in this article are in colour only in the electronic version) 1. Introduction development of phosphor and scintillator materials to be used in their exploitation. It was 110 years ago in November 1895 that Wilhelm Conrad It is to be noticed that for registration of x-ray the so- Roentgen noticed the glow of a barium platino-cyanide screen, called direct registration principle is widely used, in which the placed next to his operating discharge tube, and discovered new incoming radiation is directly converted into electrical current invisible and penetrating radiation [1], which was named x-ray in a semiconducting material. -
Manipulating Nonproportionality of Strontium Iodide Crystals with High-Flux Irradiation by 137Cs Gamma Rays
Manipulating Nonproportionality of Strontium Iodide Crystals with High-Flux Irradiation by 137Cs Gamma Rays By David D. Caudel Dissertation Submitted to the Faculty of the Graduate School of Vanderbilt University in partial fulfillment of the requirements for the degree of DOCTOR OF PHILOSOPHY in Physics May 2017 Nashville, Tennessee Approved: Keivan Stassun, Ph.D. Arnold Burger, Ph.D. Richard Haglund, Ph.D. Ashley Stowe, Ph.D. In dedication to my children and in loving memory of my father. Also, to the Fisk-to-Vanderbilt Bridge Program, for giving me the chance to fulfill my dream of becoming a physicist. ii ACKNOWLEDGMENTS The work in this dissertation has been supported by the following entities and funding sources: the Fisk-to-Vanderbilt Bridge Program, the BOLD fellowship, the GAANN fellowship CFDA 84.200, the NSF Grant HRD 1547757 (CREST-BioSS Center), the Vanderbilt Discovery Grant, and Fisk University’s subaward with ORNL GO under prime contract DE-AC52-07NA27344 from the United States Department of Energy. iii TABLE OF CONTENTS Page DEDICATION .......................................................................................................................... ii ACKNOWLEDGEMENTS ............................................................................................... iii LIST OF TABLES ....................................................................................................................... vi LIST OF FIGURES ......................................................................................................... -
THE INFLUENCE of LIGHT ANION IMPURITIES UPON Sri2(EU) SCINTILLATOR CRYSTALS 2831
2830 IEEE TRANSACTIONS ON NUCLEAR SCIENCE, VOL. 63, NO. 6, DECEMBER 2016 The Influence of Light Anion Impurities Upon SrI2(Eu) Scintillator Crystals S. E. Swider, S. Lam, and A. Datta, Member, IEEE Abstract— To better identify the influence of light anion impu- as metallic strontium is known to react aggressively with rities on the scintillation performance, small boules of SrI2(Eu) nitrogen Halide impurities such as chlorine and bromine may were grown by the vertical Bridgman-Stockbarger method, each 0 2− 3− be introduced via impurities in the hydrogen-iodide acid used co-doped with 0.2% of one of the following: C ,CO3 ,N , 2− − 3− 2− 2− − − to convert strontium carbonate into strontium iodide. Likewise, O ,OH ,PO4 ,S ,SO4 ,Cl and Br . Residual impurity concentrations were measured, and the scintillation performance residual phosphorous may be present in the hydrogen-iodide of resulting detectors was characterized. Oxygen was tolerated acid, or in the minerals from which strontium is mined. up to 0.2% on a molar basis. Sulfur proved to be highly To maintain and improve purity, crystal growers handle SrI2 detrimental to both crystallinity and scintillation performance. and similar salts in low-moisture, argon-filled glove boxes. Nitrogen produced additional emission near 480 nm. This study They also employ melt-filtration [5] and reactive gasses such suggests that SrI2(Eu) readily incorporates anion impurities, which may substitute for iodine, but these may also be removed as HI(g) [10]–[11]. However, since it is not clear which light before and during growth by volatilization. Purity metrics for impurities are most detrimental to single-crystal growth and starting materials should include sulfur and carbon, as well as scintillation performance, current purification efforts are not oxygen and H2O. -
Neutrino Detection with Liquid Scintillator Detectors
Neutrino Detection with Liquid Scintillator Detectors Minfang Yeh Neutrino and Nuclear Chemistry Chemistry/Instrumentation BNL VIRTUAL SYMPOSIUM FOR ETI/MTV CONSORTIA, 2021 Neutrino and Nuclear Chemistry at BNL since 1960+ 37 37 - HOMESTAKE 615t Cl + νe → Ar + e 71 71 - Gallex 30-t Ga + νe → Ge + e 780t D2O CC/NC SNO 200-kt H2O or 37-kt LAr LBNE (DUNE) 120-t 8% In-LS LENS 200-t 0.1% Gd-LS Daya Bay 780t 0.3% Nd/Te-LS SNO+ 6Li, 10B or Gd doped LS PROSPECT/LZ Metal-doped WbLS and 0νββ, dark-matter, AIT- plastic scintillator resins NEO, medical Water-based LS Scintillator Radiochemical Cerenkov 1960 1970 1980 1990 2000 2010 2020 M Yeh, BNL VIRTUAL SYMPOSIUM 2 LZ (Gd-doped) Dark Matter BNL-ν-Map SD, USA by liquid scintillator detectors AIT-NEO (WbLS) Boulby, UK JSNS2 (Gd-doped) SNO+ (Te-doped) Kamioka, Japan ANNIE Sudbury Canada (WbLS) BNL FNAL Daya Bay (Gd- doped), China PROSPECT (6Li-doped ), ORNL, TN, USA Cover a wide range of physics topics! neutrinos, dark matter, 0νββ, nonproliferation, medical physics,… M Yeh, BNL VIRTUAL SYMPOSIUM 3 Scintillation Mechanism S. Hans, J. Cumming, R. Rosero, S. Gokhale, R. Diaz, C. Camilo, M. Yeh, Light-yield quenching and remediation in liquid scintillator detectors, 2020 JINST 15 P12020 fast slow Stokes shift, photon-yield, timing structure, and C/H density determine the detector responses M Yeh, BNL VIRTUAL SYMPOSIUM 4 Scintillator Components C. Buck and M. Yeh, J. Phys. G: Nucl. Part. Phys. 43 093001 (2016) 200tons of Daya Bay Gd-LS produced in 2010; stable since production. -
United States Patent 0 "3 Cc Patented Apr
2,882,298 _, United States Patent 0 "3 cc Patented Apr. 14, 1959 1 2 a mixture of equimolar quantities of nickel iodide (Nilz) and either sodium iodide (NaI) or zinc iodide (Znlz) 2,882,298 will provide the required increased ratio of iodide ion to nickel ion concentration. Alternatively, a catalyst PREPARATION OF ACRYLIC ACID ESTERS mixture of one mol of nickel chloride and three mols of Benjamin J. Luberolf, Stamford, Conn., assignor to sodium iodide may be used. American 'Cyanamid Company, New York, N.Y., Although the reason for the synergistic e?ect is not a corporation of Maine entirely understood, the activity of such a catalyst mix No Drawing. Application March 26, 1956 ture in the aforedescribed process is materially increased Serial No. 573,658 ‘over that of either nickel iodide as catalyst or the relative 1y inert supplemental iodide alone. In general, how 2 Claims. (Cl. 260-486) ever, the ratio of iodide 'ion to nickel ion is greater than two but less than about ?ve. It is therefore a good practice to use about equal amounts of nickel iodide This invention relates to a novel and improved method 15 and the supplemental iodide. for‘. preparing acrylic acid and esters thereof. More par Typically illustrative soluble metal iodide compounds ticnlarly, it relates 'to a liquid phase reaction whereby other than nickel iodide will include a variety of broad acetylene, carbon monoxide and .either ‘water or an alco classes. However, the prime requirement is that the hol all being present in equivalent amounts are reacted alkali metal be soluble in the reaction medium. -
Cosmic Ray Detector Hardware
Cosmic Ray Detector Hardware How it detects cosmic rays, what it measures and how to use it… Matthew Jones Purdue University 2012 QuarkNet Summer Workshop 1 What are Cosmic Rays? • Mostly muons down here… • Why are they called “rays”? – Purely historical • How can we detect them? – Muons are like heavy electrons – They have an electric charge – “Ionizing radiation”… – Some of their energy is transferred to the electrons in the material the move through – That’s what we detect… 2 Detecting Ionizing Radiation Cloud Chamber Solid State Geiger Counters Detectors Bubble Chamber Radiation creates Ion Chambers electron/hole pairs in Ionization initiates a silicon or germanium physical change in a that allow a current to gas or liquid. Wire Chambers flow. Photographic Film Crystal Scintillator GEM Detectors Photographic Organic An electric field does Emulsion Scintillator WORK on ionized gas Recombination of atoms to produce a Ionization initiates a electrons and ions voltage pulse. chemical reaction. produces light! 3 Plastic Scintillator 4 Plastic Scintillator • See, for example, Saint-Gobain, Inc. • Clear plastic traps light by total internal reflection. • Doped with a secret chemical that emits light when ionized, but does not re-absorb it. • Easy to cut, polish, bend, glue… • How much light is produced? – A muon travelling through 1 cm of plastic scintillator might produce about a thousand photons – Most of them would be blue – They bounce around inside the scintillator until they either escape or are absorbed • Usually wrapped in tin foil or white paper and then in black plastic or opaque paper to keep other light out. 5 The Cosmic Ray Detector Plastic scintillator wrapped in white paper and black plastic. -
Tuesday, June 3 Plan of the Day
Tuesday, June 3 Tuesday, June 3 Plan of the Day SORMA West 2008 moves from International House to an adjacent part of the campus: Stanley Hall and Bechtel Engineering Center, Sibley Auditorium. Contributed orals in parallel sessions will be given in the morning. Early in the noon hour, after a brief break (not long enough to return to the Doubletree or explore the campus), buses will load for the San Francisco and Muir Woods tours. Box lunches will be provided. The buses will return to the Doubletree. Those who did not sign up for a tour are free for the afternoon and may wish to stop by the information desk for maps, restaurant guides, etc. 8:00am-12:00pm Information Desk Sibley Auditorium Foyer 9:00am-10:15am Parallel Sessions Stanley Hall and Bechtel/Sibley Aud. 10:15am-10:45am Break 10:45am-12:00 Parallel Sessions Stanley Hall and Bechtel/Sibley Aud. Noon- Lunch (Boxed) Afternoon SF Tour/ Muir Woods Tour Plan of the Day Page Tuesday-1 Tuesday, June 3 New Scintillators Tuesday AM I: Stanley 105 Chair: Chuck Melcher, Univ. of Tennessee Tuesday AM I: Stanley 105-1 Crystal Growth and Scintillation Properties of Strontium Iodide Scintillators Edgar Van Loef, Radiation Monitoring Devices, Inc. (RMD) Cody M. Wilson; Nerine J. Cherepy, Giulia Hull, Stephen A. Payne (LLNL); Woon-Seng Choong, William W. Moses (LBNL); Kanai S. Shah (RMD) Security applications and nuclear non-proliferation depend on the rapid identification of highly enriched uranium, weapons grade plutonium, radioactive sources and other special nuclear materials. Efficient detection of their gamma-ray signature is the most common method for identification and requires a scintillator that has a high light yield, good energy resolution, fast scintillation decay and high effective atomic number. -
Maine Remedial Action Guidelines (Rags) for Contaminated Sites
Maine Department of Environmental Protection Remedial Action Guidelines for Contaminated Sites (RAGs) Effective Date: May 1, 2021 Approved by: ___________________________ Date: April 27, 2021 David Burns, Director Bureau of Remediation & Waste Management Executive Summary MAINE DEPARTMENT OF ENVIRONMENTAL PROTECTION 17 State House Station | Augusta, Maine 04333-0017 www.maine.gov/dep Maine Department of Environmental Protection Remedial Action Guidelines for Contaminated Sites Contents 1 Disclaimer ...................................................................................................................... 1 2 Introduction and Purpose ............................................................................................... 1 2.1 Purpose ......................................................................................................................................... 1 2.2 Consistency with Superfund Risk Assessment .............................................................................. 1 2.3 When to Use RAGs and When to Develop a Site-Specific Risk Assessment ................................. 1 3 Applicability ................................................................................................................... 2 3.1 Applicable Programs & DEP Approval Process ............................................................................. 2 3.1.1 Uncontrolled Hazardous Substance Sites ............................................................................. 2 3.1.2 Voluntary Response Action Program