The EDELWEISS-II experiment Silvia SCORZA Université Claude Bernard- Institut de Physique nucléaire de Lyon CEA-Saclay DAPNIA/DRECAM (FRANCE), CNRS/CRTBT.

Slides:



Advertisements
Similar presentations
The EDELWEISS-II experiment
Advertisements

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.
Status of XMASS experiment Shigetaka Moriyama Institute for Cosmic Ray Research, University of Tokyo For the XMASS collaboration September 10 th, 2013.
EDELWEISS-I last results EDELWEISS-II prospects for dark matter direct detection CEA-Saclay DAPNIA and DRECAM CRTBT Grenoble CSNSM Orsay IAP Paris IPN.
Dark Matter search with EDELWEISS and beyond Gilles Gerbier CEA Saclay – IRFU Rencontres de Moriond- VHEPU march 15 th Expérience pour DEtecter.
Institut für Kernphysik Markus Horn ILIAS-N3, BSNS-working group meeting Valencia, Forschungszentrum Karlsruhe in der Helmholtz-Gemeinschaft.
Status of Ultra-low Energy HPGe Detector for low-mass WIMP search Li Xin (Tsinghua University) KIMS collaboration Oct.22nd, 2005.
Background issues for the Cryogenic Dark Matter Search Laura Baudis Stanford University.
KIT – Universität des Landes Baden-Württemberg und nationales Forschungszentrum in der Helmholtz-Gemeinschaft Benjamin Schmidt, IEKP, KIT Campus North,
Direct search for Dark Matter with the EDELWEISS-II experiment: status and results Claudia Nones CSNSM-Orsay On behalf of the EDELWEISS-II collaboration.
R. Lemrani CEA Saclay Search for Dark Matter with EDELWEISS Status and future NDM ’06 Paris, September 3-9, 2006.
1 Edelweiss-II status Eric Armengaud (CEA), for the Edelweiss Collaboration Axion-WIMPs training workshop, Patras, 22/06/2007.
Present and Future Cryogenic Dark Matter Search in Europe Wolfgang Rau, Technische Universität München CRESSTCRESST EURECA ryogenic are vent earch with.
PANDAX Results and Outlook
30 Ge & Si Crystals Arranged in verticals stacks of 6 called “towers” Shielding composed of lead, poly, and a muon veto not described. 7.6 cm diameter.
CUORICINO and CUORE Chiara Brofferio Università di Milano – Bicocca and INFN, Sez. di Milano NOW 2004 – Otranto 12 – 17 September 2004 On behalf of the.
1 Low radioactivity issues in EDELWEISS-II Low Radioactivity Techniques, LRT 2010 Sudbury, August 2010 Pia Loaiza, Laboratoire Souterrain de Modane,
EDELWEISS-II : Status and future
Dan Bauer Fermilab Users Meeting June 3, 2004 Status of Cold Dark Matter Searches Dan Bauer, Fermilab Introduction Scientific case compelling for cold.
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,
TAUP2007, Sendai, 12/09/2007 Vitaly Kudryavtsev 1 Limits on WIMP nuclear recoils from ZEPLIN-II data Vitaly A. Kudryavtsev Department of Physics and Astronomy.
Direct Dark Matter Searches
Cryogenic particle detection at the Canfranc Underground Laboratory First International Workshop for the Design of the ANDES Underground Laboratory Centro.
th KPS meeting 1 Development of Radon Monitoring Detector for the KIMS Experiment Lee, Myoung Jae DMRC, Seoul national university.
From CDMSII to SuperCDMS Nader Mirabolfathi UC Berkeley INPAC meeting, May 2007, Berkeley (Marina) CDMSII : Current Status CDMSII Perspective Motivation.
Surface events suppression in the germanium bolometers EDELWEISS experiment Xavier-François Navick (CEA Dapnia) TAUP Sendai September 07.
Dark Matter Search with SuperCDMS Results, Status and Future Wolfgang Rau Queen’s University.
SuperCDMS From Soudan to SNOLAB Wolfgang Rau Queen’s University.
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.
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.
The European Future of Dark Matter Searches with Cryogenic Detectors H Kraus University of Oxford EURECA.
Michael Unrau, Institut für Kernphysik Analyse von Bolometersignalen der EDELWEISS Dark Matter Suche EDELWEISS dark matter searchFull InterDigitized detector.
Status of Surface Sensitive Bolometers University of Insubria – Como, Italy INFN – Milano, Italy Prague, Chiara Salvioni.
Underground Laboratories and Low Background Experiments Pia Loaiza Laboratoire Souterrain de Modane Bordeaux, March 16 th, 2006.
Search for double electron capture in 106 Cd using HPGe detectors and Si pixel detectors Ivan Štekl for TGV collaboration Institute of Experimental and.
Min Kyu Lee ( 이민규 ) Kyoung Beom Lee ( 이경범 ) Yong-Hamb Kim ( 김용함 ) Low Temperature Detectors 2006 Workshop on the Underground Experiment at Yangyang TEXONO-KIMS.
Experiment TGV II Multi-detector HPGe telescopic spectrometer for the study of double beta processes of 106 Cd and 48 Ca For TGV collaboration: JINR Dubna,
VIeme rencontres du Vietnam
Ultra-low background gamma spectrometry 2 nd LSM-Extension Workshop, Valfréjus, 16 October 2009 Pia Loaiza Laboratoire Souterrain de Modane.
Véronique SANGLARD Université de Lyon, UCBL1 CNRS/IN2P3/IPNLyon Status of EDELWEISS-II.
KPS Chonbuk University 2005/10/22 HYUNSU LEE Status of the KIMS dark matter search experiment with CsI(Tl) crystals Hyun Su Lee Seoul National.
Muon and Neutron Backgrounds at Yangyang underground lab Muju Workshop Kwak, Jungwon Seoul National University 1.External Backgrounds 2.Muon.
EDELWEISS-II -EDW I reminder -current status and future of EDWII -short report on DAMNED -few words on EURECA Hunt for Dark Matter, Fermilab may 10th 2007.
Physics at Extreme Energies, Hanoi, July 2000 Dark Matter Search in the EDELWEISS expt G. Chardin DAPNIA/SPP, CEA-Saclay.
WIMP search Result from KIMS experiments Kim Seung Cheon (DMRC,SNU)
EDELWEISS-II : Status and future Véronique SANGLARD CNRS/IN2P3/IPNLyon
Activities on double beta decay search experiments in Korea 1.Yangyang Underground laboratory 2.Double beta decay search with HPGe & CsI(Tl) 3.Metal Loaded.
Results of the NEMO-3 experiment (Summer 2009) Outline   The  decay  The NEMO-3 experiment  Measurement of the backgrounds   and  results.
DARK MATTER SEARCH Carter Hall, University of Maryland.
Pia Loaiza AARM-Berkeley March 2010
Ray Bunker (UCSB) – APS – April 17 th, 2005 CDMS SUF Run 21 Low-Mass WIMP Search Ray Bunker Jan 17 th -DOE UCSB Review.
SuperCDMS From Soudan to SNOLAB Wolfgang Rau Queen’s University 1W. Rau – IPA 2014.
1 CRESST Cryogenic Rare Event Search with Superconducting Thermometers Jens Schmaler for the CRESST group at MPI MPI Project Review December 14, 2009.
Limits on Low-Mass WIMP Dark Matter with an Ultra-Low-Energy Germanium Detector at 220 eV Threshold Overview (Collaboration; Program; Laboratory) Physics.
Low Mass WIMP Search with the CDMS Low Ionization Threshold Experiment Wolfgang Rau Queen’s University Kingston.
P. CermakRez near Prague, December 2005 EC/EC process measurement in TGV experiment For TGV collaboration: JINR Dubna, Russia CTU Prague, Czech Republic.
Scintillating Bolometers – Rejection of background due to standard two-neutrino double beta decay D.M. Chernyak 1,2, F.A. Danevich 2, A. Giuliani 1, M.
Slides for IG NewS : GG – analysis june juin 2016 Spherical detector: recent developments I. Giomataris, CEA-Irfu-France Spherical detector at.
CRESST Cryogenic Rare Event Search with Superconducting Thermometers Max-Planck-Institut für Physik University of Oxford Technische Universität München.
A Search for Cold Dark Matter with Cryogenic Detectors at Frejus Underground Laboratory * EDELWEISS experiment 1.Experiment status and results for first.
From Edelweiss I to Edelweiss II
Status of ULE-HPGe Experiment for WIMP Search in YangYang
The COBRA Experiment: Future Prospects
Dark Matter Search With an Ultra-low Threshold Germanium Detector proposed by Tsinghua University Seoul National University Academia Sinica Qian Yue.
Measurement of surface radioactivity by Alpha/Beta detection
The Heidelberg Dark Matter Search Experiment
Harry Nelson UCSB DUSEL Henderson at Stony Brook May 5, 2006
CRESST Cryogenic Rare Event Search with Superconducting Thermometers
CsI Compton Veto Detector for A low Mass WIMP Experiment
Status of Neutron flux Analysis in KIMS experiment
Presentation transcript:

The EDELWEISS-II experiment Silvia SCORZA Université Claude Bernard- Institut de Physique nucléaire de Lyon CEA-Saclay DAPNIA/DRECAM (FRANCE), CNRS/CRTBT Grenoble (FRANCE), CNRS/IN2P3/CSNSM Orsay (FRANCE), CNRS/IN2P3/IPN Lyon (FRANCE), CNRS/INSU/IAP Paris (FRANCE), CNRS-CEA/Laboratoire Souterrain de Modane (FRANCE), JINR Dubna (RUSSIA), FZK/Universtat Karlsruhe (GERMANY)

2 Direct Search Principle Detection of the energy deposited due to elastic scattering off target nuclei Event Rate : < 1 ev /kg/week Recoil Energy : 1 – 100 keV Low energy threshold Large detector mass Low background Radio – purity Active/passive shielding Deep underground sites

3 LSM

4 EDW–II set-up Radiopurity dedicated HPGe detectors for systematic checks of all materials Strict control of bkg: material selection/cleaning procedure/Environment  Shielding 20 cm Pb shielding 50 cm PE and better coverage active μ veto (> 98% coverage) Up to 110 detectors -> 40kg Ge detector Ge/NTD Develop new ID detectors  Goal: EDW-I × 100 σ W-n ≤ pb 10keV)

5 µ-veto Candidates for coincident veto-bolometer events Accidental coincidences Expected from Geant4 simulation: ~0.03 events/kg.d Measured: 0.04 events/kg.d

6 Ge Heat-Ionization Detectors Simultaneous measurements: few V/cm with Al electrodes 20 mK with Ge/NTD sensor Different Ionization/Heat energy ratio for nuclear and electronic recoils (dominate bkg)

7 Event by event background rejection

8 Edw-I limiting background PRD71, (2005) Problem: Surface electron recoils Interpretation: Bad charge collection (trapping and recombination) Indications of 210 Pb contamination (exposition to Radon):  α rate ~ e rate ~ 4 /kg.day

9 206 Pb β 210 Pb 210 Po  210 Po 210 Pb 210 Pb source

10 GeNTD data: improved bkg Gamma background: reduction of x3 relative to EDELWEISS-I 210 Pb-chain background: reduction of x2 relative to EDELWEISS-I EDW-I ~4 /kgd EDW-II ~2 /kgd 5 kgd 95 kgd preliminary Full volume Further bkg reductions after fiducial + coincidence cuts Conclusion: Reduction of background from EDW-I to EDW-II

11 Physics run: GeNTD 11 detectors with <30 keV threshold Threshold chosen before start of run (EDW-I results  expected  bkg) 93.5 kg.day 3 events observed in nuclear recoil band 31, 31 and 42 keV Evidence for events with deficient charge collection from 210 Pb Preliminary EDELWEISS 93.5 kgd Question: How to reach < pb ? NEED  >1000 kgd at 15 keV threshold  >10 5 rejection for gammas  to reject expected >4000  from 210 Pb IDea : Develop detectors with surface event rejection using interleaved electrode design (ID)

12 A A AAA B BBB C CCCC D DDD G H GuardFiducial volume → E → E → E → E ‘A’ electrodes: +2V ID detector Radius (cm) Z (cm) guard ‘G’: + 1V guard ‘H’: - 1V ‘C’ electrodes:-2V ‘D’ electrodes: -1V Electron trajectories hole trajectories ‘A&C’ bulk event ‘A&B’ near- surface event ‘A,B&C’ event in low-field area  NTD heat sensor E-field modified near surface with interleaved electrodes B+D signals -> vetos % surface 1x200g + 3x400g tested in x400g running ‘B’ electrodes: +1V

13 ID detector rejection Gamma rejection of 400g ~1 month calibrations Beta rejection of 200g -equivalent to 3x10 4 kgd 6x Bi 6x Po 0 events -equivalent to ~10 3 kgd

14 Physics run: ID detectors 1 x 400g + 1 x 350g detectors, 86 live days <15 keV threshold achieved for exposure of 18.6 kg.days 50% efficiency at 10 keV No events in (or around) nuclear recoil band Conclusion: This is the good technology for pb and beyond

15 Limits 93.5 kgd GeNTD 11 detectors x 4 months 30 keV threshold 3 events observed in nuclear recoil band 18.3 kgd ID 2 detectors x 4 months 15 keV threshold No nuclear recoils No evts outside  band 2009: 10 ID detectors improvement in sensitivity: 4x10 -8 pb More detectors build in 2009 Preliminary

16 Conclusions/Outlook Significant reduction in , β and γ backgrounds relative to EDELWEISS-I Improved understanding of backgrounds and of response of detectors to backgrounds Improved limit relative to EDELWEISS-I Passive background reduction alone not sufficient to reach < pb ID detectors have the surface rejection needed to reach this goal Running in 2009 with 10 x 400g detectors Prototype of ID detectors with larger fiducial volumes currently in test EURECA = 1 ton scale experiment (CRESST, EDELWEISS, CERN, LSM extension

This is the end…

18 Decay Chain 210 Po 206 Pb  5.3 MeV100 keV Al 70nm amGe 70nm Ge 2cm 206 Pb  e - 10keV - 100keV - 1MeV Cu few mm 5 mm ~50 nm 350 nm 20  m 700  m 210 Bi e MeV max 210 Pb e - 61 keV max  46.5 keV (4%)  46 keV 3 mm NO ionisation 22 yr

19 EDELWEISS-II 210 Pb source calibration Confirms interpretation of EDW-I bkg as 210 Pb surface . Response of detectors to this important background 210 Pb 206 Pb β 210 Po  E=5.3 MeV Q~0.3 Edw-I data EDELWEISS-II 210 Pb source 210 Pb 210 Po 206 Pb recoils coincident with 210 Po  210 Bi Edw-II Implantation depth of 210 Pb

20 EURECA - II

21 EURECA-I

22

23 France-Italy Fréjus tunnel : new safety gallery planned Existing road tunnel Existing lab s ?  2 projects  Limited extension  Very large cavity

24 G Gerbier EURECA ULISSE meeting- Lyon july Implantation of new lab First drawings nov 2006 (Lombardi eng company)

25 Compatibility DAMA other experiments SI

26 Compatibility DAMA other experiments SD

27 Present limits

28 Number of events in WIMP region: q< 0.5, 25 < E < 60 кэВ registered 23 events Experimental data Alpha rate 2.5 events

29 N alphas in calibration spectrum = 3040 events Number of events in WIMP region: q< 0.5, 25 < E < 60 кэВ registered = 460 events 460 events Expected number events from calibration with 210 Pb = 37 events Estimation of background from 210 Pb