TeVPA 20091 Current Status of The EXO-200 Experiment Kevin O’Sullivan Stanford University 136 Xe 136 Ba ++ + 2e - (+ 2ν e )

Slides:



Advertisements
Similar presentations
SNOLAB and EXO David Sinclair SNOLAB Workshop August 2005.
Advertisements

Neutrino Masses double beta decay oscillations Majorana Dirac.
The SNO+ Experiment: Overview and Status
Progress on a Gaseous Xe detector for Double Beta Decay (EXO) David Sinclair Xenon Detector Workshop Berkeley, 2009.
DMSAG 14/8/06 Mark Boulay Towards Dark Matter with DEAP at SNOLAB Mark Boulay Canada Research Chair in Particle Astrophysics Queen’s University DEAP-1:
COBRA Kai Zuber University of Sussex 5 th SNOLAB Workshop,
September 14, 2007Hardy Simgen, TAUP 2007 / Sendai1 Status of the GERDA experiment Hardy Simgen Max-Planck-Institut für Kernphysik Heidelberg on behalf.
GERDA: GERmanium Detector Array
Charles Prescott - SLAC Neutrino Day - April 18, 2003 The Search for Neutrinoless Double Beta Decay - Physics Motivations - Limits from ν oscillations.
14 June 2005EXO SLAC DOE Pgm Rev M. Breidenbach1 D.Leonard, A.Piepke Physics Dept, University of Alabama, Tuscaloosa AL P.Vogel Physics Dept Caltech, Pasadena.
The XENON Project A 1 tonne Liquid Xenon experiment for a sensitive Dark Matter Search Elena Aprile Columbia University.
From CUORICINO to CUORE: To probe the inverted hierarchy region On behalf of the CUORE collaboration DUSL Meeting, Washington DC November 2,-4, 2007 Frank.
Daniel Lenz, University of Wisconsin, Madison 11/05/ APS DNP Cryogenic search for neutrinoless double beta decay Daniel Lenz on behalf of the CUORE.
Search for Neutrinoless double beta-decays with the Enriched Xenon Observatory Derek Mackay and Nicole Ackerman.
Z.Djurcic, D.Leonard, A.Piepke Physics Dept, University of Alabama, Tuscaloosa AL P.Vogel Physics Dept Caltech, Pasadena CA A. Bellerive, M. Dixit, C.
The COBRA Double Beta Decay Search Experiment
Jun 2, 2004EXO - SLAC Program Review1 Z.Djurcic, D.Leonard, A.Piepke Physics Dept, University of Alabama, Tuscaloosa AL P.Vogel Physics Dept Caltech, Pasadena.
Status of EXO-200 Carter Hall, University of Maryland DUSEL town meeting November 4, 2007.
PANDAX Results and Outlook
Proportional Light in a Dual Phase Xenon Chamber
EXO-Development Program DUSEL Workshop Washington, November 2007 David Sinclair Carleton/TRIUMF.
LAUNCH - Low-energy, Astroparticle Underground, Neutrino physics and Cosmology in Heidelberg, Low-level techniques applied in experiments.
Chad Orzel Union College Physics Radioactive Background Evaluation by Atom Counting C. Orzel Union College Dept. of Physics and Astronomy D. N. McKinsey.
EXO-GAS Detector Status report for the SNOLAB EAC August 2007.
Full EXO in Cryopit Cryopit Workshop August 2011 David Sinclair.
EXO Gas Progress and Plans October, 2008 David Sinclair.
NEMO-3  experiment First Results and Future Prospects Ruben Saakyan, UCL UK HEP Neutrino Forum The Cosener’s House, Abingdon.
GERmanium Detector Array – a Search for Neutrinoless Double Beta Decay X. Liu - MPI für Physik, München Symposium – symmetries and phases in the universe,
ZEPLIN II Status & ZEPLIN IV Muzaffer Atac David Cline Youngho Seo Franco Sergiampietri Hanguo Wang ULCA ZonEd Proportional scintillation in LIquid Noble.
Double Beta Decay in SNO+ Huaizhang Deng University of Pennsylvania.
Z.Djurcic, D.Leonard, A.Piepke Physics Dept, University of Alabama, Tuscaloosa AL P.Vogel Physics Dept Caltech, Pasadena CA A. Bellerive, M. Dixit, C.
6/11/11TIPP Ba Tagging activities in EXO Karl Twelker Stanford University Enriched Xenon Observatory TIPP Conference June 11, 2011.
Status of COBRA 6 th SNOLAB Workshop, Picture courtesy
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.
A large water shield for dark matter, double beta decay and low background screening. T. Shutt - Case R. Gaitskell - Brown.
Contribution of Penning trap mass spectrometry to neutrino physics Szilárd Nagy MPI-K Heidelberg, Germany New Instruments for Neutrino Relics and Mass,
Poster Design & Printing by Genigraphics ® Neutrino Interactions Studying the properties of neutrinos will shed light on the origin of the.
1 Liquid Argon Dark Matter: Synergies with R&D for Neutrino Detectors: Chemically clean Argon for drifting electrons and light output (Oxygen and H20 relevant.
M. Wójcik for the GERDA Collaboration Institute of Physics, Jagellonian University Epiphany 2006, Kraków, Poland, 6-7 January 2006.
Performance and applications of a  -TPC K. Miuchi a†, H. Kubo a, T. Nagayoshi a, Y. Okada a, R. Orito a, A. Takada a, A. Takeda a, T. Tanimori a, M. Ueno.
VIeme rencontres du Vietnam
M. Wójcik Instytut Fizyki, Uniwersytet Jagielloński Instytut Fizyki Doświadczalnej, Uniwersytet Warszawski Warszawa, 10 Marca 2006.
Barium-ion tagging for 136 Xe double-beta decay studies with EXO Thomas Brunner for the EXO collaboration TIPP2014 – June 5, Xe  136 Ba ++ +
1/27/2016Katsushi Arisaka 1 University of California, Los Angeles Department of Physics and Astronomy Katsushi Arisaka XAX 10.
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.
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.
Stefano Torre University College London for NEMO3 and SuperNEMO collaborations Half day IoP Meeting 12 Oct 2011 Outline 0νββ and 2νββ Observation technique.
Double Beta Decay Experiments Jeanne Wilson University of Sussex 29/06/05, RAL.
A screening facility for next generation low-background experiments Tom Shutt Case Western Reserve University.
DARK MATTER SEARCH Carter Hall, University of Maryland.
The COBRA Experiment Jeanne Wilson University of Sussex, UK On behalf of the COBRA Collaboration TAUP 2007, Sendai, Japan.
GERDA – a Search for Neutrinoless Double Beta Decay MPI für Physik, München Neutrinoless double beta decay and the GERDA experimentThe detector array and.
A Gas Option for EXO David Sinclair EXO Week January 2006 Note – Most of the ideas here come from a discussion with Bill.
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.
MPI für Physik, Fachbeirat, Béla Majorovits The GERDA experiment Béla Majorovits.
DPF-JPS 2006 Oct 31, Hawaii 1 CANDLES system for the study of 48-Ca double beta decay T. Kishimoto Osaka Univ.
Search for Neutrinoless Double Beta Decay with NEMO-3 Zornitza Daraktchieva University College London On behalf of the NEMO3 collaboration PANIC08, Eilat,
The NEMO3 Double Beta Decay Experiment Ruben Saakyan IoP meeting on Double Beta Decay Manchester 21 November 2007.
The EXO-200 Detector Razvan Gornea for the EXO Collaboration LHEP, Center for Research and Education in Fundamental Physics, Bern University Frontier Detectors.
1 Cary Kendziora Fermi National Laboratory Cary Kendziora Fermi National Laboratory CEC-ICMC 2013 Anchorage Alaska – June, 2012.
Sheffield - Headline News NaI SMALL ARRAY DM55(high gamma background) vs. DM46 -> similar bump rate DM48 -> some evidence for a bump? DM50 (QMW) -> abandoned.
0νDBD Experimental Review and 136 Xe With HP Gas at CJPL 季向 东.
Status of EXO experiment F. Juget Université de Neuchâtel.
PandaX DM Search Exp Xiangdong Ji (季向东)
Prompt Gamma Activation Analysis on 76Ge
Double Beta Decay - status and future
XAX Can DM and DBD detectors combined?
Presentation transcript:

TeVPA Current Status of The EXO-200 Experiment Kevin O’Sullivan Stanford University 136 Xe 136 Ba e - (+ 2ν e )

TeVPA Why use xenon? Xenon isotopic enrichment is easier. 200kg of Xe has already been enriched to 80% in 136 Xe Xenon is “reusable”. Can be repurified & recycled into new detector Monolithic detector. LXe is self shielding, surface contamination minimized. Minimal cosmogenic activation. No long lived radioactive isotopes of Xe. … admits a novel coincidence technique. Background reduction by Ba daughter tagging. Energy resolution is poorer than the crystalline devices (~factor 10), but

TeVPA Ba Ion Identification Ba + system well studied (Neuhauser, Hohenstatt, Toshek, Dehmelt 1980) Ba + system well studied (Neuhauser, Hohenstatt, Toshek, Dehmelt 1980) Very specific signature: “shelving” Very specific signature: “shelving” Single ions can be detected from a photon rate of 10 7 /s Single ions can be detected from a photon rate of 10 7 /s Important additional Important additional constraint constraint Drastic background Drastic background reduction reduction 6P 1/2 5D 3/2 6S 1/2 493nm 650nm Metastable 47s  R = 5.28 MHz  B = 15.2 MHz

TeVPA Paths to a Ton Scale Experiment EXO-200 –Low-background Xe TPC with 200kg of 80% enriched 136 Xe –No Ba Tagging Liquid Phase Barium Tagging –Ion transfer from LXe to ion trap –Ba tagging in Situ –Ba tagging in SXe Gas Phase R&D –~100kg prototype detectors –Ion manipulation in gas

TeVPA EXO-200

TeVPA Improving the Energy Resolution ~570 keV Ionization and Scintillation results using 207 Bi Ionization alone: σ(E)/E = 570 keV or Q ββ or Q ββ Ionization & Scintillation: σ(E)/E = 570 keV or Q ββ or Q ββ E.Conti et al. Phys. Rev. B (68) EXO-200 will collect 3-4 times as much scintillation…

TeVPA teflon light reflectors flex cables on back of APD plane (copper on kapton) field shaping rings (copper) acrylic supports LAAPD plane (copper) and x-y wires (photo-etched phosphor bronze) Central HV plane (photo-etched phosphor bronze) ~40 cm x-y crossed wires, 60 o

TeVPA EXO-200 Copper Chamber

TeVPA The EXO-200 detector class 100 clean room The Xe vessel HFE (Heat transfer fluid) Vacuum insulation 25cm enclosure of low activity lead Refrigeration feedthroughs HFE feedthrough Vacuum pump-out port

TeVPA Materials qualification database ~ 330 entries Neutron Activation Analysis (NAA) - Alabama (MIT reactor) ICP-MS and GD-MS - INMS (Ottawa), commercial outfits Radon emanation - Laurentian (Sudbury) Gamma counting - Neuchâtel, Alabama Alpha counting - Alabama, Carleton, SLAC, Stanford Monte Carlo

Xenon Handling System xenon condenser xenon purity monitor and heater EXO-200 goal: 0.1 ppb O 2 equivalent t ~ 4 ms (electrons)

TeVPA muon flux at WIPP (~ 1700 m.w.e.): 4.77×10 -3 m -2 s -1 (3.10×10 -3 m -2 s -1 sr -1, ~15 m -2 h -1 ) E.-I.Esch et al., Nucl. Instr. Meth. A 538(2005)516 ★ EXO-200

TeVPA Assumptions: 1)200kg of Xe enriched to 80% in 136 2)σ(E)/E = 1.4% obtained in EXO R&D, Conti et al., Phys Rev B 68 (2003) )Low but finite radioactive background: 20 events/year in the ±2σ interval centered around the (0.4) keV endpoint 1 5)Negligible background from 2  (T 1/2 >1·10 22 yr) 2 EXO-200 Majorana mass sensitivity EXO-200 Case Majorana mass (meV) QRPA 3 NSM 4 40 Radioactive Background (events) 6.4* * T 1/2 0ν (yr, 90%CL) σ E 2.5MeV (%) Run Time (yr) Eff. (%) Mass (ton) 1) M. Redshaw, J., McDaniel, E. Wingfield and E.G. Myers (Florida State Precision Penning Trap), to be submitted to Phys. Rev C. 2) R. Bernabei et al., Phys. Lett. B 546, 23 (2002) 3) Rodin, et. al., Nucl. Phys. A 793 (2007) ) Caurier, Phys. Rev. Lett. 100, (2008)

TeVPA Future Plans All EXO-200 infrastructure is underground undergoing final testing The LXe TPC is built Electronics testing underway The TPC is scheduled to be installed in the cryostat before the end of 2009 Running will start next year with natural Xenon with an eventual switch to enriched Xenon Ba Tagging and gas phase R&D ongoing

TeVPA Stanford University, Stanford, Ca Enriched Xenon Observatory for double beta decay K.Barry, E.Niner, A.Piepke Physics Dept, U. of Alabama, Tuscaloosa Al P.Vogel Physics Dept Caltech, Pasadena Ca M.Dixit, K.Graham, C.Green, C.Hagemann, C.Hargrove, E.Rollin, D.Sinclair, V.Strickland Carleton University, Ottawa, Canada C. Benitez-Medina, S.Cook, W.Fairbank Jr., K.Hall, B.Mong Colorado State U., Fort Collins Co M.Moe Physics Dept UC Irvine, Irvine Ca D.Akimov, I.Alexandrov, A.Burenkov, M.Danilov, A.Dolgolenko, A,Karelin, A.Kovalenko, A.Kuchenkov, V.Stekhanov, O.Zeldovich ITEP Moscow, Russia B.Aharmim, K.Donato, J.Farine, D.Hallman, U.Wichoski Laurentian U., Sudbury, Canada H.Breuer, C.Hall, L.Kaufman, D.Leonard, S. Slutsky, Y-R. Yen U. of Maryland, College Park Md K.Kumar, A.Pocar U. of Massachusetts, Amherst Ma M.Auger, G.Giroux, R.Gornea, F.Juget, G.Lutter, J-L.Vuilleumier, J-M.Vuilleumier Laboratory for High Energy Physics, Bern, Switzerland N.Ackerman, M.Breidenbach, R.Conley, W.Craddock, S. Herrin, J.Hodgson, D.McKay, A.Odian, C.Prescott, P.Rowson, K.Skarpaas, K.Wamba, J.Wodin, L.Yang, S.Zalog SLAC, Menlo Park CA L.Bartoszek, R.DeVoe, M.Dolinski, P.Fierlinger, B.Flatt, G.Gratta, M.Green, F.LePort, M.Montero-Diez, R.Neilson, A.Reimer-Müller, A.Rivas, K.O’Sullivan, K.Twelker

TeVPA Back up Slides

TeVPA Xenon Enrichment Total of 200kg of Xe enriched to 80% in 136 Xe EXO Stockpile Natural Xe Enriched Xe

TeVPA Ba Tagging

TeVPA CCD e- Quadrupole linear ion trap Ba + grabber Ba + Tagging Schematic for EXO

TeVPA Single Ba ion trapping... Ba ovene-gun Fluorescence imaging 0 V -10 V RF quadrupole potential in each segment Multiply by 16, and add a buffer gas to cool down the ions injected at one end of the trap into a DC minimum short longitudinal trapping segment radial trapping longitudinal trapping

TeVPA Detection of Single Ions in Buffer Gas Single ion cloud (5 s integration) Torr He P(493) = 75 μW P(650) = 300 μW 1 ion 2 ions 3 ions 0 ions 1 ion 2 ions 3 ions M. Green, et al. Phys. Rev. A (2007) Electrodes glowing from scattered laser light

TeVPA Capacitive cryo-tip Picture of sensor 1 mm 2 mm Cryo-tip (ground) Electrostatic field lines Capacitive sensor (-HV) Ion mobility: µ ~ 0.3 cm 2 /kVs K. Wamba et al., NIM A 555 (2005) 205 v = µ x 1kV/cm ~ 0.3 cm/s from LXe

TeVPA Full EXO Sensitivity Assumptions: 1)80% enrichment in 136 2)Intrinsic low background + Ba tagging eliminate all radioactive background 3)Energy res only used to separate the 0ν from 2ν modes: Select 0ν events in a ±2σ interval centered around the (0.4) keV endpoint 1 4)Use for 2νββ T 1/2 >1·10 22 yr 2 1) M. Redshaw, J., McDaniel, E. Wingfield and E.G. Myers (Florida State Precision Penning Trap), to be submitted to Phys. Rev C. 2) R. Bernabei et al., Phys. Lett. B 546, 23 (2002) 3) Rodin, et. al., Nucl. Phys. A 793 (2007) ) Caurier, Phys. Rev. Lett. 100, (2008) Aggressive Conservative Case Majorana mass (meV) QRPA 3 NSM (use 1) 0.5 (use 1) 2νββ Background (events) 4.1* †1† * * 5701 T 1/2 0ν (yr, 90%CL) σ E 2.5MeV (%) Run Time (yr) Eff. (%) Mass (ton)