Existing counting facilities in the US Analysis centers at most Universities User fees – cheaper for University faculty Commercial Labs Longer turn around,

Slides:



Advertisements
Similar presentations
M. Carson, University of Sheffield, UKDMC ILIAS-Valencia-April Gamma backgrounds, shielding and veto performance for dark matter detectors M. Carson,
Advertisements

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.
Status of COUPP Experiment in the MINOS tunnel Erik Ramberg AEM 4 February, 2008.
Soudan Underground Laboratory Features Moderate depth (2100 mwe) augmented with active muon veto shield Existing infrastructure (power, water, networking,
U.S. Low Level Counting Facilities Status and Plans LRT 2004, Laurentian University Dec 12-13, 2004 Prisca Cushman University of Minnesota.
SNOLAB is drawing on expertise developed by the SNO collaboration for screening materials for new experiments. Material Screening DUSEL Town Meeting 2-4.
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
Backgrounds. Their removal and avoidance Tom Shutt Princeton University.
Measurement and Survey Protocols Defining and Identifying Radioactive Materials.
WP3: R&D for ultra-low background techniques and facilities in the EU underground labs Dr. Matthias Laubenstein Laboratori Nazionali del Gran Sasso ITALY.
Background Study in NDBD Ming Shao. sources environmental gamma radioactivity cosmic rays Neutrons Radon contamination of materials which detectors and.
DUSEL Low-Background Counting (to get the program started) Dongming Mei 1, Kevin Lesko 2,Christina Keller 1, Yongchen Sun 1, Zhongbao Yin 1, Keenan Thomas.
Low Background Counting Facility at Henderson DUSEL Lots of resources already exist, e.g. 1. Homestake NUSL Reference Design Report WBS 6.1 (Low-level.
Search for Dark Matter at CJPL with PANDAX
Proposal for high sensitive measurements of 238 U and 232 Th with NAA Ezio Previtali INFN Sez. Milano Milano-Bicocca University ILIAS: JRA1 3rd General.
Low-Background Activation Analysis NAA for ultrapure materials analysis Richard M. Lindstrom Analytical Chemistry Division National Institute of Standards.
Status of SNOLAB Development Fraser Duncan SNOLAB Workshop 4 Oct 2008.
Report on the Workshop for
Future Development and Needs for Low Background Counting and Assay Capability Richard Ford (SNOLAB) Future Project Planning Workshop 25 th August 2015.
Low background Screening and Prototyping Facility at the Soudan Underground Lab 40’ x 35’ x 100’ cavern surrounded by a 99% efficient active muon veto.
Eun-Ju Jeon Sejong Univ. Sept. 09, 2010 Status of RENO Experiment Neutrino Oscillation Workshop (NOW 2010) September 4-11, 2010, Otranto, Lecce, Italy.
A screening facility for next generation low-background experiments Tom Shutt Laura Cadonati Princeton University.
Low Background Counting, Materials Purity, Radon issue Prisca Cushman University of Minnesota Not LBC… New Name? AALRMS Assay and Acquisition of Low Radiation.
Fraser Duncan Queen’s University Synergies in Low Background Techniques 26 July 2005 Underground Facilities at SNOLAB.
APS April meeting Jacksonville, 2007 WIMP Search With SNOLAB Chris Jillings SNOLAB Staff Scientist For the DEAP-1 Collaboration.
Topical Workshop in Low Radioactivity Techniques, Sudbury, Canada, August 28-29, 2010 Surface cleaning techniques B. Majorowits a, M. Wójcik b, G. Zuzel.
A large water shield for dark matter, double beta decay and low background screening. T. Shutt - Case R. Gaitskell - Brown.
Brian W. Miller, Ph.D. Linus Pauling Distinguished Postdoctoral Fellow Radiation Detection & Nuclear Sciences Group Pacific Northwest National Laboratory.
Context: astroparticle physics, non-accelerator physics, low energy physics, natural sources physics, let’s-understand-the-Universe physics mainly looking.
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.
A Study of Background Particles for the Implementation of a Neutron Veto into SuperCDMS Johanna-Laina Fischer 1, Dr. Lauren Hsu 2 1 Physics and Space Sciences.
PHENO 2010 Christopher White, IIT 1 The Daya Bay Reactor Antineutrino Experiment Christopher White 1.
Silvia Borjabad Copper Electroforming 7th JRA-1 Meeting Zaragoza (November 2007) Status Report.
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.
M. Wójcik for the GERDA Collaboration Institute of Physics, Jagellonian University Epiphany 2006, Kraków, Poland, 6-7 January 2006.
TUNL R. B. Vogelaar March 1, 2007 Measuring the complete Solar neutrino spectrum E th =114 keV (95% of pp spectrum) Measure pp- 3% Determine CNO-fraction.
March 19, 2010Kara Keeter1 Ultra-Sensitive Immersion Tank MOTIVATION –WHOLE-BODY COUNTING –TARGET SENSITIVITIES TO – g/g U/Th, etc. –POLLING.
Tracking (wire chamber) Shield radon, neutron,  Source foil (40 mg/cm 2 ) Scintillator + PMT 2 modules 2  3 m 2 → 12 m 2 Background < 1 event / month.
Dan Bauer - CDMS Project ManagerAll experimenters meeting - April 23, 2007 Cryogenic Dark Matter Search (CDMS) Progress at Soudan since last summer Successful.
Ultra-low background gamma spectrometry 2 nd LSM-Extension Workshop, Valfréjus, 16 October 2009 Pia Loaiza Laboratoire Souterrain de Modane.
The Daya Bay Reactor Neutrino Experiment R. D. McKeown Caltech On Behalf of the Daya Bay Collaboration CIPANP 2009.
CTF at Gran Sasso (overview of the hardware) Richard Ford (SNOLAB) (who has not been in the collaboration since 2004) March 19 th 2010.
TG 11 overview / Material screening Hardy Simgen MPI für Kernphysik for Task Group 11.
Daya Bay Reactor Neutrino Experiment On behalf of the DayaBay collaboration Virginia Polytechnic Institute and State University Joseph ykHor YuenKeung,
Results of the NEMO-3 experiment (Summer 2009) Outline   The  decay  The NEMO-3 experiment  Measurement of the backgrounds   and  results.
Gaitskell SOLO SOudan LOw Background Counting Facility Rick Gaitskell Brown University, Department of Physics see information at
ILIAS Project Summary ILIAS is an Integrated Infrastructure Initiative that has pulled together all of Europe's leading infrastructures in Astroparticle.
B.Sadoulet CDMS DUSEL The Deep Underground Science and Engineering Laboratory The process Themes DUSEL and CDMS Bernard Sadoulet Dept. of Physics.
Low Background Studies at the Soudan Underground Laboratory-9/20/ Low Background Studies at the Soudan Underground Laboratory The Soudan Underground.
A screening facility for next generation low-background experiments Tom Shutt Case Western Reserve University.
Pia Loaiza AARM-Berkeley March 2010
1 Study of 48 Ca Double Beta Decay by CANDLES T. Kishimoto Osaka Univ.
SPHENIX MECHANICAL D. Lynch September 11, AGENDA Global Design Concept – Updated Global Assembly Concept – Updated Inner HCal Installation concept.
Template for DUSEL Meeting with Potential Experiments.
CDMS II Shielding To Installation To Construction From Design.
GeMPI-type low background counting system for SURF Kara Keeter 15 September 2014.
The Princeton NaI Experiment (SABRE) Frank Calaprice Princeton University Cosmic Frontier Workshop SLAC March
NSD Update James Symons 9/14/ Inch Cyclotron / Accelerator Based Nuclear Science News Element 114 Confirmation Fixed Vacuum Leak in “D” - July 2009.
Neutron Shield/Muon Veto (WBS 1.3) and Underground Installation Issues (WBS 1.6) May 11, 2009 Erik Ramberg.
1 DarkSide Collaboration APC Paris, France Augustana College, USA Black Hills State University, USA Fermilab, USA IHEP, China INFN Laboratori Nazionali.
Main Entry: syn·er·gy Inflected Form(s): plural -gies Etymology: New Latin synergia, from Greek synergos working together A mutually advantageous conjunction.
1 Cary Kendziora Fermi National Laboratory Cary Kendziora Fermi National Laboratory CEC-ICMC 2013 Anchorage Alaska – June, 2012.
SuperCDMS and CUTE at SNOLAB
SuperCDMS & Radon Ray Bunker
Simulation for DayaBay Detectors
Harry Nelson UCSB DUSEL Henderson at Stony Brook May 5, 2006
• • • Ge measurements for SuperNEMO
Open to the Public & Open for Business
Presentation transcript:

Existing counting facilities in the US Analysis centers at most Universities User fees – cheaper for University faculty Commercial Labs Longer turn around, more expensive, more standardized “Use for Others” at most national labs (Oak Ridge, LANL, BNL) A few shallow  middle depth sites open for users LBL Bldg72 and Oroville Dam – now LOMO at PNNL - soon Deep screening sites are only in development stage WIPP (MEGA ) Soudan:  -screening capability in SOLO Plans to create a multi-purpose LBCF Really, Really Deep sites are DUSEL era DEPTH

Sensitivity for US Sites Surface counters LBL Bldg 72, PNNL, and many other places etc. Shielded on surface PNNL 17-A LBNL Oroville mwe Soudan, MEGA LoMoCF estimate

Berkeley Complex: Surface and Shallow Site under same umbrella organization: Institute of Nuclear and Particle Astrophysics STAFF Kevin Lesko Al Smith Dick McDonald Donna Hurley

Throughput determined by number of Ge detectors Bldg72 has NaI counters and a 130% HPGe, Oroville has a 80% p-type HPGe Major User: SNO (screened virgin and machined acrylic, plastic resins, PMT envelopes, internal components, stainless steel, etc.) Also Clean room preparation and operation, sample handling procedures Sensitivity is currently limited by detector contamination Bldg 72 (LBL) Dam (140 mi) from LBL

PNNL – UW Complex: Surface + 17-A ULB + new initiative at Lower Monumental Dam 1 hr from PNNL 37 meters of overburden Operated by US Army Corp of Engineers

Inside LoMo Counting Facility: Currently being used as cosmogenic isolation space for copper stock and MEGA parts Plan is to install gamma screening in lead cave. Funding is in place. 4’ 1’ 4’ 1’1’1’ Water trough ~8’ Person Access 4-person elevator access Two sets of 3 HPGe counters with active cosmic veto shield UW J.A. Formaggio J.F. Wilkerson PNNL C.E. Aalseth R.L. Brodzinski T. Hossbach H.S. Miley J.L. Orrell

WIPP DOE Facility Impressive infrastructure Modest depth (1600 mwe) Science not primary mission SEGA underground by next summer (not a screener) Assembling MEGA at WIPP now. 1st detector ready to take data Completed in a couple years.

Low background Screening and Prototyping Facility at the Soudan Underground Lab Last Soudan2 proton decay calorimeters (at back) were removed Nov 23 rd 2004 SOLO HPGe Jim Reeves: Cu Electroforming SBIR + Cu screening detector (microBq/kg) Diode M (35%) Twin (75%) UF detector (100%) Arrives 3 rd week in March

Low background Screening and Prototyping Facility at the Soudan Underground Lab CDMS offices CDMS Aux Clean Room BFand SiLi detector, leaching lab? other? Veto shield repaired last summer DAQ: location & time stamp for each muon

Medtronics “suitcase” experiment (soft memory errors) COUPP dark matter prototype (J. Collar) Phase 2 proposal (Reeves SBIR) Fabricate Ge detectors (Princeton Gamma-Tech SBIR) Neon dark matter prototype (James White, TAMU) XENON going to Italy for the espresso and climate? Other near term users (in ranked-order of real  maybe)

Strategy for Soudan LBCF Create minimum facility now DOE University supplements for infrastructure (power feed, technician, lease fee) Define fee structure for users & sign EPS Continue to improve gamma screening Fix Twin, upgrade electronics, upgrade DAQ, Diode-M becomes pre-screener, UF HPGe into castle Provide novel beta screeners through CWRU, Caltech … (or possible MRI 2006) Take this next year to Increase size of collaboration Modify design according to input and new users Put in complete proposal next Fall ‘05 Funding from NSF, DOE (HEP and Nuc) implies main justification must be from Astro/HEP/Nucl community. Reduce financial impact by maintaining it thru user fees to other groups DUSEL is a different model – can we get other divisions involved?

University of Minnesota Intercollegiate Grant 1.Seek out other user communities for LBCF 2.Coordinate low level counting/analysis across sites Examples of other user communities involved: Tritium and 14 C in groundwater Radioactive environmental sampling (accidental release of radio-isotopes) Exposure assessment studies ( 14 C as a tracer of particiulate lung burden) Epidemiological studies of uranium workers (tissue samples) Short-lived isotopes for sediment dating Tracers in uptake and transport (geomicrobiology) Bioremediation studies etc etc… These “other” users need well-type HPGe, chemical separation, sample handling AND beta-counting applications ( 14 C, 3 H, 40 K) DUSEL work has uncovered new synergies with geomicrobiology, geology, hydrology WORKSHOP in Minneapolis in July to explore these synergies

Material to be screened: Ge, Si wafers LEDs Copper (detector holders, icebox, copper tape) Low activity solder, silver epoxy, brass screws, cables and connectors Magnetic shield Striplines, side coaxes and squet cards, kevlar Shielding materials (inner lead, outer lead, copper, polyethylene) Estimated samples/year (including replicates): 36 samples/year (HPGe) 12 samples/year (Ge, Si wafers) contaminant screened or isotope(s) analyzed 238-U, 232-Th, 40-K, 60-Co, 134-Cs, 137-Cs, 207-Bi, 210-Pb sensitivity desired (ppb or Bq/kg): 100 mBq/kg to < 0.5 mBq/kg SuperCDMS (response to DUSEL survey) Laura’s first draft How many of these can go through ICPMS or other? How many ultra-low samples?

Ante- room Multi- purpose clean room Clean room over tank Water ports with crane Electro form 40 ft Upper mezzanine above tank top User shielding Clean room over tank anteroom Clean room Water tank Shielded bays mezzanine anteroom radon scrubbing plenum. stairs current mezzanine Muon veto shield 100 ft Drawings and Design Consultation: Short Elliott Henderson Engineering, Inc

Figure E-16 from the Homestake Reference Design Secure lab Emanation and leaching laboratory (TBA) Pool 2 Gd-loaded liq. Scint for neutron sensitivity or Mini-Borexino for U/Th down to g/g Pool 1 12 m cube – ultra-pure water NAA Laboratory + general environmental sample handling Built-in liq. Scint acrylic thimble ports read out by PMT’s for U/Th down to g/g