Low-Background Activation Analysis NAA for ultrapure materials analysis Richard M. Lindstrom Analytical Chemistry Division National Institute of Standards.

Slides:



Advertisements
Similar presentations
Contributions to Nuclear Data by Radiochemistry Division, BARC
Advertisements

Heeger theta13, May A Neutrino Project at Diablo Canyon.
M. Carson, University of Sheffield, UKDMC ILIAS-Valencia-April Gamma backgrounds, shielding and veto performance for dark matter detectors M. Carson,
Underground Facilities Stub 2 Stub 2a,3 ‘H’ Area JIF Area The underground research facilities have evolved since dark matter studies began at Boulby. There.
NSS Requirements Review: Labs and Workshops Michelle Everett Lab Coordinator Scientific Activities Division November 12,
Soudan Underground Laboratory Features Moderate depth (2100 mwe) augmented with active muon veto shield Existing infrastructure (power, water, networking,
ILIAS J1, 3rd General Meeting, Paris, 14th Feb Coordinated gamma measurements in the underground labs Jan Kisiel Institute of Physics, University.
Search for spontaneous muon emission from lead nuclei with OPERA bricks M. Giorgini, V. Popa Bologna Group OPERA Collaboration Meeting, LNGS, 19-22/05/2003.
WP3: R&D on ultra low-level WP3: R&D on ultra low-level detectors and facilities JRA1 general meeting, Paris, Feb. 14 th 2006.
WP3: R&D on ultra low-level detectors and facilities WP3: R&D on ultra low-level detectors and facilities status and outlook Matthias Laubenstein JRA1.
Cosmic Induced Backgrounds D. Reyna Argonne National Lab.
Calorimetry and Showers Learning Objectives Understand the basic operation of a calorimeter (Measure the energy of a particle, and in the process, destroy.
WP3: R&D on ultra low-level detectors and facilities WP3: R&D on ultra low-level detectors and facilities LNGS: status and outlook.
Materials Assay & ICPMS for DUSEL R&D
WP3: R&D for ultra-low background techniques and facilities in the EU underground labs Dr. Matthias Laubenstein Laboratori Nazionali del Gran Sasso ITALY.
WP1: Measurement of the backgrounds in the EU underground sites Dr. Matthias Laubenstein Laboratori Nazionali del Gran Sasso ITALY J1 General Meeting Paris.
Background Study in NDBD Ming Shao. sources environmental gamma radioactivity cosmic rays Neutrons Radon contamination of materials which detectors and.
THE LABORATORY FOR LOW-LEVEL RADIOACTIVITY LNGS
Low radioactivity at the Modane Underground Laboratory
LAUNCH - Low-energy, Astroparticle Underground, Neutrino physics and Cosmology in Heidelberg, Low-level techniques applied in experiments.
1 Neutrino Possibilities at the SNS 2 Motivation For me as an experimentalist motivation is two fold On this workshop we have nice theory talks about.
Laser Induced breakdown spectroscopy in Water for elemental analysis.
Lee, Myeong Jae DMRC, Seoul national university
1 JASMIN Activation Experiments (T-972/993/994) Yoshimi Kasugai on behalf of JASMIN Activation team JASMIN Activation team Y. Kasugai, K. Oishi, H. Matsumura,
Institute of Isotopes Hungarian Academy of Sciences Current R&D Activities at the Institute of Isotopes Related to Nuclear Safeguards, Forensics and Environmental.
Trace element content comparison for high-loss and low-loss sapphire* S. C. McGuireG. P. Lamaze and E. A. Mackey Department of PhysicsChemical Sciences.
Neutron Activation Analysis at the Radiochemical Laboratory, Institute of Nuclear Techniques, Budapest University of Technology and Economics N. Vajda,
A screening facility for next generation low-background experiments Tom Shutt Laura Cadonati Princeton University.
2001 Mars Odyssey GRS RDS 1 HEND Workshop 2002 May 20 th – 22 nd 2002 Mars Odyssey Gamma-Ray Spectrometer Richard Starr NASA/GSFC – Catholic University.
Low Background Counting, Materials Purity, Radon issue Prisca Cushman University of Minnesota Not LBC… New Name? AALRMS Assay and Acquisition of Low Radiation.
Cosmic Rays The discovery of cosmic rays Discoveries made with cosmic rays Cosmic rays in modern physics education Let’s count cosmic rays around us.
NIST Surface and Microanalysis Science Division Low-Level Counting (llc) At NIST George A. Klouda Surface and Microanalysis Science Division National Institute.
Airborne Radioactivity By Beth Harmony. Reasons for the experiment: Radiation is something that we are constantly being bombarded with from all directions.
Fraser Duncan Queen’s University Synergies in Low Background Techniques 26 July 2005 Underground Facilities at SNOLAB.
Cosmic-Ray Induced Neutrons: Recent Results from the Atmospheric Ionizing Radiation Measurements Aboard an ER-2 Airplane P. Goldhagen 1, J.M. Clem 2, J.W.
Neutron Monitoring Detector in KIMS Jungwon Kwak Seoul National University 2003 October 25 th KPS meeting.
Ultra-low background HPGe detector at ChyeongPyung Underground Laboratory TaeYeon Kim and KIMS(Korea Invisible Mass Search) Collaboration. * Contents *
Internal background of CsI(Tl) crystal detectors for dark matter search Tae Yeon Kim Seoul National University For the KIMS Collaboration Seoul National.
CTF and low background facility at Gran Sasso A. Ianni a, M. Laubenstein a and Y. Suvorov a a INFN, Gran Sasso Laboratory, Assergi (AQ), Italy The Counting.
75 th Annual Meeting March 2011 Imaging with, spatial resolution of, and plans for upgrading a minimal prototype muon tomography station J. LOCKE, W. BITTNER,
Experimental part: Measurement the energy deposition profile for U ions with energies E=100 MeV/u - 1 GeV/u in iron and copper. Measurement the residual.
Warszawa, July 3rd Measurements of natural radioactivity in European underground labs within the ILIAS project Jan Kisiel Institute of Physics, University.
May 6, 2006Henderson Dusel Capstone Meeting Low Background Counting A Facility Wish List for the New Underground Laboratory F. Calaprice.
Underground Laboratories and Low Background Experiments Pia Loaiza Laboratoire Souterrain de Modane Bordeaux, March 16 th, 2006.
Stellenbosch University
M. Wójcik for the GERDA Collaboration Institute of Physics, Jagellonian University Epiphany 2006, Kraków, Poland, 6-7 January 2006.
1 Henderson DUSEL Capstone 05/06/2006 Background Modeling and Clean Room Design Considerations for HUSEP Zeev Shayer and Jonathan Ormes Department of Physics.
M. Wójcik Instytut Fizyki, Uniwersytet Jagielloński Instytut Fizyki Doświadczalnej, Uniwersytet Warszawski Warszawa, 10 Marca 2006.
Structure of the Earth and Mineralogy Environmental Science Earth Science Unit Environmental Science Earth Science Unit.
Muon and Neutron Backgrounds at Yangyang underground lab Muju Workshop Kwak, Jungwon Seoul National University 1.External Backgrounds 2.Muon.
The analytical techniques most widespread for certification in the iron and steel industry are X-ray Fluorescence Spectrometry (XRF), Arc/Spark Optical.
Results of the NEMO-3 experiment (Summer 2009) Outline   The  decay  The NEMO-3 experiment  Measurement of the backgrounds   and  results.
Trace element analysis of K, U and Th in high purity materials by Neutron Activation Analysis P. ILA Dept. of Earth Atmospheric & Planetary Sciences Massachusetts.
Low Background Studies at the Soudan Underground Laboratory-9/20/ Low Background Studies at the Soudan Underground Laboratory The Soudan Underground.
DEPARTMENT OF PHYSICS AND ASTRONOMY X-ray Astronomy and Space Instrumentation I3 Meeting, December 2004 Integrating Space Radiation Sensing Infrastructures.
A screening facility for next generation low-background experiments Tom Shutt Case Western Reserve University.
Pia Loaiza AARM-Berkeley March 2010
1 Underground Gamma-ray Spectrometry in HADES Mikael Hult Institute for Reference Materials and Measurements (IRMM) Geel, Belgium
GeMPI-type low background counting system for SURF Kara Keeter 15 September 2014.
Neutron Shield/Muon Veto (WBS 1.3) and Underground Installation Issues (WBS 1.6) May 11, 2009 Erik Ramberg.
Application of AMS for the Analysis of
Background simulations: update and simulations of absorbed dose
Fast neutron flux measurement in CJPL
Measuring light elements (e. g
Pulse-shape discrimination with Cs2HfCl6 crystal
Simulation for DayaBay Detectors
Muon and Neutron detector of KIMS experiment
Status of Neutron flux Analysis in KIMS experiment
Nuclear Power Regulatory Overview
Study of Muon-induced Neutrons in the KIMS Experiment
Presentation transcript:

Low-Background Activation Analysis NAA for ultrapure materials analysis Richard M. Lindstrom Analytical Chemistry Division National Institute of Standards and Technology Gaithersburg, Maryland

Detection Limit for  Assay Detection limit is inversely proportional to the detector efficiency and counting time, and ~proportional to the square root of the resolution R and the environmental background B n where A =1/desired precision and b the peak integration width (Cooper 1970)

Example: Composition of Interplanetary Dust Particles Desired a factor ~10 6 improvement in sensitivity over "normal” INAA 200x by longer, higher-flux irradiation 100x by increasing counting efficiency and time 7x by reduced background –D. J. Lindstrom, Analysis of Submicrogram Samples by INAA, Nucl. Instrum. Methods A299 (1990),

Background: NIST vs. RCL Nearly all background at NIST (ground level) is from cosmic muons Going 60 ft underground at NASA-JSC reduced all cosmic components by a factor 5 –R. M. Lindstrom, D. J. Lindstrom, L. A. Slaback, and J. K. Langland, A Low-Background Gamma Ray Assay Laboratory for Activation Analysis, Nucl. Instrum. Methods A299 (1990),

Example: Forensics Locating and measuring 100 fg Ir particle in 60 mg of rock by INAA –B. C. Schuraytz, D. J. Lindstrom, L. E. Marín, R. R. Martinez, D. W. Mittlefehldt, V. L. Sharpton, and S. J. Wentworth, Iridium Metal in Chicxulub Impact Melt: Forensic Chemistry on the K-T Smoking Gun, Science 271 (1996),

Other Counting LDEF:12 nuclides measured in stainless steel Genesis: 3 years of solar wind at L1 Ambient 85 Kr in 1.5 liters of air –L. A. Currie and G. A. Klouda, Detection and Quantification Capabilities for 85 Kr with the NIST Low-Level Gas Counting System: Impacts of Instrumental and Environmental Backgrounds, J. Radioanal. Nucl. Chem. 248 (2001),

Lab Design 1 Depth Floor space Lifting equipment Environment conditioning –Temperature –Humidity –Particulates –Radon?

Lab Design 2 Utilities –UPS, filtered power –Network –LN 2 Sample prep clean area (above ground?) Change room Chemical fume hood Assembly shop –Zone refining & crystal growing?

Graded Shielding Room cm salt or ultrabasic rock; 2 m water Several Ge detectors, separated by ~ meters Lead or iron shield Inner shield (old Pb, Cu, Fe)

Intermediate Depth Laboratory For materials characterization For equipment testing More accessible than Homestake –NBSR: “America’s favorite neutron source.” Modest depth – 30 m rock (70 mwe) attenuates 30x

Example: Cosmic-ray Neutron Activation Activation at ground level –Elements W, Au, Ta, In, Re, Sm, Dy, Mn Counting at 500 mwe in HADES –M. J. Martínez Canet, M. Hult, M. Köhler, and P. N. Johnston, Measurement of activation induced by environmental neutrons using ultra low-level  -ray spectrometry, Appl. Radiat. Isotop. 52 (2000),

CELLAR: Collaboration of European Low-level underground LAboRatories EC-JRC-IRMM (HADES), Belgium (~225 m) IAEA-MEL, Monaco LNGS, Italy (~1700 m) LNSCE, France (~2200 m) MPI Heidelberg, Germany (~10 m) PTB, Gemany (~925 m) University of Iceland (~165 m) VKTA (Felsenkeller), Germany (~50 m)