Pia Loaiza AARM 19-20 March 2010 Background studies for EURECA EURECA The ‘submarine’ (water tank) design: background expected from stainless steel structure.

Slides:



Advertisements
Similar presentations
Edelweiss-II : status and first results A new generation of background-free bolometers for WIMP search X-F. Navick - CEA Saclay, IRFU, France LTD13 – Stanford.
Advertisements

Stefano Pirro, IDEA Meeting –Milano November Status of the scintillating bolometer program Scintillating Bolometers Background rejection capabilities.
M. Carson, University of Sheffield, UKDMC ILIAS-Valencia-April Gamma backgrounds, shielding and veto performance for dark matter detectors M. Carson,
Activity for the Gerda-specific part Description of the Gerda setup including shielding (water tank, Cu tank, liquid Nitrogen), crystals array and kapton.
M. Carson, University of Sheffield IDM 2004, University of Edinburgh Veto performance for a large xenon detector.
Background issues for the Cryogenic Dark Matter Search Laura Baudis Stanford University.
September 14, 2007Hardy Simgen, TAUP 2007 / Sendai1 Status of the GERDA experiment Hardy Simgen Max-Planck-Institut für Kernphysik Heidelberg on behalf.
R. Lemrani CEA Saclay Search for Dark Matter with EDELWEISS Status and future NDM ’06 Paris, September 3-9, 2006.
GERDA: GERmanium Detector Array
Possible merits of high pressure Xe gas for dark matter detection C J Martoff (Temple) & P F Smith (RAL, Temple) most dark matter experiments use cryogenic.
Status of activities of the WP4 on Radiopurity of Materials Pia Loaiza Laboratoire Souterrain de Modane JRA1 meeting Paris February 20 th, 2007.
1 Edelweiss-II status Eric Armengaud (CEA), for the Edelweiss Collaboration Axion-WIMPs training workshop, Patras, 22/06/2007.
First results of the Ge semi-planar detector in LSM ILIAS JRA1 meeting-Zaragoza, 23 rd November 2007 Pia Loaiza Laboratoire Souterrain de Modane.
Low radioactivity at the Modane Underground Laboratory
ILIAS Physics in deep underground laboratories JRA1 : Low background techniques WP4 : Radiopurity of materials Pía Loaiza Laboratoire Souterrain de Modane,
Search for Dark Matter at CJPL with PANDAX
M. Dracos, CEA, 10/04/ Double Beta experiment with emulsions?
LAUNCH - Low-energy, Astroparticle Underground, Neutrino physics and Cosmology in Heidelberg, Low-level techniques applied in experiments.
Stefano Pirro LRT-2004 Sudbury December 13, 2004 Cleanliness backgrounds and surface contaminations in Cuore Stefano Pirro INFN-Milano.
1 Low radioactivity issues in EDELWEISS-II Low Radioactivity Techniques, LRT 2010 Sudbury, August 2010 Pia Loaiza, Laboratoire Souterrain de Modane,
Report on The Study of (α,n) Neutron Yield and Energy Spectrum Dongming Mei for the AARM collaboration 1.
EDELWEISS-II : Status and future
FIRST RESULTS OF THE NEMO 3 EXPERIMENT Laurent SIMARD LAL Orsay (France) HEP-EPS 2003 conference CENBG, IN2P3-CNRS et Université de Bordeaux, France CFR,
A screening facility for next generation low-background experiments Tom Shutt Laura Cadonati Princeton University.
NEXT radiopurity measurements: status and results S. Cebrián (on behalf of the radiopurity measurements group) NEXT Collaboration Meeting Canfranc, 9th.
From CDMSII to SuperCDMS Nader Mirabolfathi UC Berkeley INPAC meeting, May 2007, Berkeley (Marina) CDMSII : Current Status CDMSII Perspective Motivation.
Status of the Se82 project Selenium production and purification JRA2-ILIAS Prague, April 20th, 2006, IDEA-N4 meetingDominique Lalanne.
Topical Workshop in Low Radioactivity Techniques, Sudbury, Canada, August 28-29, 2010 Surface cleaning techniques B. Majorowits a, M. Wójcik b, G. Zuzel.
SuperCDMS From Soudan to SNOLAB Wolfgang Rau Queen’s University.
Ultra-low background HPGe detector at ChyeongPyung Underground Laboratory TaeYeon Kim and KIMS(Korea Invisible Mass Search) Collaboration. * Contents *
Low background radioactivity measurements Pia Loaiza Laboratoire Souterrain de Modane CNRS/CEA, France  Why do we need ultra-low radioactivity measurements?
HEP-Aachen/16-24 July 2003 L.Chabert IPNL Latest results ot the EDELWEISS experiment : L.Chabert Institut de Physique Nucléaire de Lyon ● CEA-Saclay DAPNIA/DRECAM.
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.
VIeme rencontres du Vietnam
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.
Ultra-low background gamma spectrometry 2 nd LSM-Extension Workshop, Valfréjus, 16 October 2009 Pia Loaiza Laboratoire Souterrain de Modane.
M. Wójcik Instytut Fizyki, Uniwersytet Jagielloński Instytut Fizyki Doświadczalnej, Uniwersytet Warszawski Warszawa, 10 Marca 2006.
The EDELWEISS-II experiment Silvia SCORZA Université Claude Bernard- Institut de Physique nucléaire de Lyon CEA-Saclay DAPNIA/DRECAM (FRANCE), CNRS/CRTBT.
The GENIUS dark matter project Laura Baudis Stanford University.
Véronique SANGLARD Université de Lyon, UCBL1 CNRS/IN2P3/IPNLyon Status of EDELWEISS-II.
BACKGROUND REJECTION AND SENSITIVITY FOR NEW GENERATION Ge DETECTORS EXPERIMENTS. Héctor Gómez Maluenda University of Zaragoza (SPAIN)
28 May 2008NEMO-3 Neutrino081 NEMO-3 A search for double beta decay Robert L. Flack University College London On behalf of the NEMO-3 collaboration.
NEMO3 experiment: results G. Broudin-Bay LAL (CNRS/ Université Paris-Sud 11) for the NEMO collaboration Moriond EW conference La Thuile, March 2008.
Results of the NEMO-3 experiment (Summer 2009) Outline   The  decay  The NEMO-3 experiment  Measurement of the backgrounds   and  results.
A screening facility for next generation low-background experiments Tom Shutt Case Western Reserve University.
DARK MATTER SEARCH Carter Hall, University of Maryland.
Pia Loaiza AARM-Berkeley March 2010
Phase I: Use available 76 Ge diodes from Heidelberg- Moscow and IGEX experiments (~18 kg). Scrutinize with high siginificance current evidence. Phase II:
Nasim Fatemi-Ghomi, Group Christmass Meeting December Nasim Fatemi-Ghomi Double Beta Decay Study of 150 Nd at NEMO3 (The magic isotope!!)
Sep. 22, 2011 Seoul National University Jae Keum Lee KIMS Background 1 China-Korea Workshop 2011 September 22-23, 2011.
GeMPI-type low background counting system for SURF Kara Keeter 15 September 2014.
1 Double Beta Decay of 150 Nd in the NEMO 3 Experiment Nasim Fatemi-Ghomi (On behalf of the NEMO 3 collaboration) The University of Manchester IOP HEPP.
November 19, 2007Hardy Simgen, IDEA-Meeting Paris Status of the GERDA experiment Hardy Simgen Max-Planck-Institut für Kernphysik Heidelberg on behalf.
Search for Neutrinoless Double Beta Decay with NEMO-3 Zornitza Daraktchieva University College London On behalf of the NEMO3 collaboration PANIC08, Eilat,
From Edelweiss I to Edelweiss II
Application of AMS for the Analysis of
Institute for Scintillation Materials
Possible Rad. Background in 136Xe DBD
On measurability of mBq/kg levels of alpha activity
Measurement of surface radioactivity by Alpha/Beta detection
The Heidelberg Dark Matter Search Experiment
Serge Nagorny – GSSI-INFN
Simulation for DayaBay Detectors
Very preliminary study of the random background for the BiPo detector (PhoSwich configuration) Work done by Jonathan Ferracci.
CRESST Cryogenic Rare Event Search with Superconducting Thermometers
XAX Can DM and DBD detectors combined?
• • • Ge measurements for SuperNEMO
Gilles Gerbier for EDELWEISS collab.
BACKGROUND STUDY IN CRESST
Presentation transcript:

Pia Loaiza AARM March 2010 Background studies for EURECA EURECA The ‘submarine’ (water tank) design: background expected from stainless steel structure The ‘pool’ design: - gamma background from vessel - gamma background from copper - beta background and rejection

Pia Loaiza AARM March pb goal = no background in kg.d Joint effort from teams from EDELWEISS, CRESST, ROSEBUD, CERN, + others… >>100 kg cryogenic experiment, multi- target Part of ILIAS/ASPERA European Roadmap Preferred site: m 3 extension of present LSM (4  /m2/d), to be dug in EURECA

Pia Loaiza AARM March events -equivalent to ~10 3 kgd arXiv: accepted by PLB Gamma Rejection better than 1 in 10 5 EDELWEISS II: GAMMA REJECTION

Pia Loaiza AARM March 2010 HALL B: DARK MATTER (EURECA TYPE) Hall B m 3 Approx. dimensions: 18x15x50 m Internal dimensions (2400 m 3 ): 11x6x46 m water First shielding configuration: the ‘submarine’ design

Pia Loaiza AARM March 2010 STAINLESS STEEL 226 Ra 228 Th 40 K 60 CoSUM Borexino Steel for flanches Astrop. Phys. 18, 1 (2002) A (mBq/kg) 6.2   1.6 <  1 Single e - recoils < Double Chooz Outkumpu P. Loaiza A (mBq/kg) 5  25.5  1.3 <  2 Single e - recoils < Edelweiss 304L C. Goldbach, G. Nollez A (mBq/kg) 4  25  214  1014  3 Single e - recoils GERDA Ugine&Alz Ti W. Maneschg et al NIM A 593, 448 (2008) A (mBq/kg) < 0.74< 0.41<  0.7 Single e - recoils < 32000<19100< XENON Fábrica del Campo de Gibraltar, Cádiz 316Ti From L. Baudis, IDM08 A (mBq/kg) < 1.3< 0.9< Single e - recoils 57000<42000< Events from 2cm thick water-tank per 100 kg Ge per year, 10 keV <E r < 50 keV ~2 ·10 5 Simulations by V. Kudryavtsev et al

Pia Loaiza AARM March 2010 Gamma background from stainless steel water tank for the ‘submarine’ configuration  pb goal = no background in kg.d  from stainless steel water-tank: 2 ·10 5 evts/100 kg year = 8 ·10 5 evts in kg.d  Gamma rejection factor in EDWII : 1 in 10 5 Untolerable gamma background

Pia Loaiza AARM March 2010 ‘Pool’ configuration Preliminary layout, to be evolved By CEA/IRFU

Pia Loaiza AARM March 2010 cryostat Cold Signals in/out Amplis Pure water Radiation level -gamma -neutron neutron gamma

Pia Loaiza AARM March 2010 Attenuation of gamma-rays by water  Swimming-pool: without water, comparable e recoil event rate expected wrt ‘submarine’ design  Around factor attenuation if 3 m water-shield  Different attenuation factors for different energies, hence for K, Co, U series → we expect no gamma-background events in the detectors from water tank vessel in the ‘pool’ design Plot by V. Kudryavtsev et al

Pia Loaiza AARM March U 232 Th 40 K 60 Co A (ppb) mBq/kg Single e - recoils/year 1.9 · ·10 5 Gamma background expected from Cu Simulations by V. Kudryavtsev et al Simulation results for e - recoils expected in 500 kg of Ge from copper parts (cryostat=2173 kg + inner parts = 692 kg), keV: Copper 226 Ra 228 Th 40 K 60 CoSUM NOSV G. Heusser, LRT2004 A (  Bq/kg) < 20< 23< 90< 10 Single e - recoils/year ~ 2 ·10 4 ~ 4 ·10 3 ~ 2 ·10 4 Which translates to: → roughly, we need the previous Cu purity to get acceptable backg levels

Pia Loaiza AARM March 2010 Beta background and rejection arXiv: v1 EDELWEISS II: beta calibration with a 210 Pb source: Beta backgroundLevel of 210 Pb backg in ROIID rejection factor Residual background Edelweiss (fid. volume Ge)3 evts/kg.d  1 / 10 5  1 / kg.d EURECA Ge0.3 evts/kg.d  1 / 10 5  1 / kg.d

Pia Loaiza AARM March 2010 SUMMARY  We have considered the water-tank design: Unacceptable gamma background from the stainless steel structure  Hence, we’ve chosen the ‘pool’ design: - no gammas expected in detectors from the vessel - need cryostat copper with 20  Bq/kg to get reasonable background levels - beta background should not be a problem if the level of surface contamination is improved by a factor 10 – within reach

Pia Loaiza AARM March 2010 Measurements of extremely low radioactivity levels in stainless steel for GERDA Amount of costly copper to be used depends drastically on the contamination of stainless steel NIM A Vol. 593, 448 (2008), W. Maneschg et al W. Manesch, H. Simgen: Private comm. Commonly available stainless steel : Ti has very low concentrations in primordial radionuclides (Mo content allows high corrosion resistance) Measurement campaign in collaboration with trading company Nironit Samples from different European manufacturers ElementCSiMnPSCrMoNiTi Min (%) (5xC) Max (%)  0.08  1.00  2.00  

Pia Loaiza AARM March 2010 SampleG2G3G5G6 VendorIlsenburgUgine&AlzAcroniIlsenburg 228 Ra (mB/kg)< 0.86<  0.5 < Th (mB/kg)<0.11<  0.2 < Ra (mB/kg)<0.24<  0.6 < m Pa (mB/kg)<12<  16 < U (mB/kg)<0.63<  1.5 < K (mB/kg)<0.93< 1.1< 0.81< Co (mB/kg) 14.0     Cs (mB/kg)<0.16<0.36< 0.1< Be (mB/kg)<3<   Mn (mB/kg) 1.5     Co (mB/kg) 0.99     Co (mB/kg) 0.17  0.06 <  0.10 < Sc (mB/kg) 0.24  0.06 <  0.14 < V (mB/kg) 0.36     0.12 U < 1 mBq/kg, Th < 1 mBq/kg, 40 K < 1 mBq/kg, 60 Co ~ 10 mBq/kg

Pia Loaiza AARM March 2010 For easier comparison activities are given as U, Th and K concentrations. For the conversion of 226Ra into U and 228Th into Th secular equilibrium was assumed although this is seldom the case Concentrations in SS used in previous experiments Collab.Ref. / measureDescription 238 U (ppb) mBq/kg 232 Th (ppb) mBq/kg nat K (ppm) mBq/kg 60 Co (mBq/kg) BOREXINOAst.Phys. 18, 1, 2002 AISI304L for SSS 0.37     1.1 < 0.45 < 14 6161 Steel for flanges 0.5     1.6 < 0.42 <13 14  1 Steel for storage vessel 1.4     2.6 <0.6 <19 12  2 Steel TK3B for storage vessel 0.4       2 46  3 DOUBLE CHOOZ P. LoaizaOutokumpu 0.41     1.3 <0.47 <15 14  2 EDWC. Goldbag and G. Nollez 304L 0.32        3

Pia Loaiza AARM March 2010

‘Xenon stainless steel’ 316Ti steel Provider: Nironit Edelstahlhandel GmbH & Co. KG Producer: Fábrica del Campo de Gibraltar, Cádiz Grade of the material : X6CrNiMoTi Works Grade : ACX Need to scan the samples since the 60 Co content may vary with charge number

Pia Loaiza AARM March 2010 NEMO 3/SUPERNEMO PURE IRON Iron petals for NEMO 3 Will be used also for SuperNemo AK Steel, provider in France, had already get to an ‘understanding’ concerning the screening of the samples prior to the ‘command’ with LAL: Open to their needs. Material 214 Bi ( 226 Ra) (mBq/kg) 208 Tl ( 228 Th) (mBq/kg) 40 K (mBq/kg) 60 Co (mBq/kg) Pure Iron< 0.6< 0.8<  0.4 Pure iron does not rust Cheaper than SS Single recoils from: Electron recoils (vessel - 2 cm thick) U < 0.6 mBq/kg< Th < 0.8 mBq/kg< K < 5 mBq/kg< Co: 1.7 mBq/kg73100 Sum < < 1.5 x 10 5 Would need a rejection factor ~ 10 5 if no external shielding