PICASSO, COUPP and PICO - Search for Dark Matter with Bubble Chambers

Slides:



Advertisements
Similar presentations
Dec. 9-10, 2004 J.I. CollarKICP “Next Generation DM Detectors” Some Desirable Features in a Next Generation WIMP Detector  Background rejection as close.
Advertisements

Mar. 21, 2005 J.I. CollarUoM HEP seminar Recirculating chiller (-10 degrees) Glass dewar Cameras Safety shield box Superheated CF 3 Br First prototypes:
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:
The PICASSO experiment - searching for cold dark matter
A Study of Background Particles for the Implementation of a Neutron Veto into SuperCDMS Johanna-Laina Fischer Mentor: Dr. Lauren Hsu [FNAL, CDMS] September.
Status of COUPP Experiment in the MINOS tunnel Erik Ramberg AEM 4 February, 2008.
COUPP-60 NuMI Commissioning Andrew Sonnenschein All Experimenters Meeting, Oct 18, 2010.
Bubble Chambers: Old Tools In New Searches For Dark Matter Geoffrey Iwata Physics /16/10.
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.
Path Towards A Large Scale Ilan Levine Indiana University South Bend For the PICASSO collaboration Detector Workshop on Next Generation Dark Matter Detectors.
PANDAX Results and Outlook
These considerations bring to 3 different techniques for DARK MATTER SEARCH: I)Bubble Chambers Continuosly Sensitive (See COUPP) II)S.D.D. (Superheated.
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.
IDM2004, September 6-10, 2004 J.I. Collar Some Desirable Features in a Next Generation WIMP Detector  Background rejection as close to 100% as possible.
Collaboration The Université de Montréal: F. Aubin, M. Barnabé- Heider, M. Di Marco, P Doane, M.-H. Genest, R. Gornea, R. Guénette, C. Leroy, L., Lessard,
October 8th, 2009 Sujeewa Kumaratunga 1/27 Recent Progress in PICASSO Sujeewa Kumaratunga for the PICASSO collaboration.
Direct Detection of Dark Matter: CDMS and COUPP
Status of DRIFT II Ed Daw representing the DRIFT collaboration: Univ. of Sheffield, Univ. of Edinburgh, Occidental College, Univ. of New Mexico Overview.
UKDMC Dark Matter Search with inorganic scintillators Vitaly A. Kudryavtsev University of Sheffield IDM2000 York, UK September 19, 2000.
Dark Matter Search with Direction sensitive Scintillator Ⅱ Department of Physics, School of Science The University of Tokyo Y. Shimizu, M. Minowa, Y. Inoue.
COUPP: Chicagoland Observatory for Underground Particle Physics (FNAL Test Beam Program T-945) J. Collar, K. Crum, D. Nakazawa, B. Odom, J. Rasmussen,
August 15-17, 2005 SNOLab Workshop #4 1 The PICASSO Dark Matter Search Experiment: Tony Noble Queen’s University The PICASSO Detector Technique Overview.
SNOLAB WORKSHOP OCT V. Zacek Université de Montréal Project overview Progress report Milestones and Schedule Infrastructure needs Personnel & HQP.
Anticipated activities for the PICO project during the next SAP Long Range Planning period. Tony Noble, Queen’s University (For the PICO Collaboration)
Applications of Micro-TPC to Dark Matter Search 1. WIMP signatures 2. Performance of the Micro-TPC 3. WIMP-wind measurement 4. Future works 5. Conclusions.
Cryogenic particle detection at the Canfranc Underground Laboratory First International Workshop for the Design of the ANDES Underground Laboratory Centro.
COUPP 2L Chamber at SNOLAB Jeter Hall Fermilab Center for Particle Astrophysics.
APS April meeting Jacksonville, 2007 WIMP Search With SNOLAB Chris Jillings SNOLAB Staff Scientist For the DEAP-1 Collaboration.
FNAL PAC COUPP, from T-945 to P-961 J.I. Collar 10/19/06 COUPP, the “Chicagoland Observatory for Underground Particle Physics” From T-945 to P-961 University.
Neutron scattering systems for calibration of dark matter search and low-energy neutrino detectors A.Bondar, A.Buzulutskov, A.Burdakov, E.Grishnjaev, A.Dolgov,
DEAP Part I: Andrew Hime (Los Alamos National Laboratory) DEAP Concept DEAP-0 Test-Results & Requirements of a DEAP Program Synergy with CLEAN Program.
SuperCDMS From Soudan to SNOLAB Wolfgang Rau Queen’s University.
Iwha Womans University 2005/04/22 Hyunsu Lee & Jungwon Kwak Current Limit of WIMP search with CsI(Tl) crystal in KIMS 이현수 *, 곽정원, 김상열, 김선기, 김승천,
J.T. White Texas A&M University SIGN (Scintillation and Ionization in Gaseous Neon) A High-Pressure, Room- Temperature, Gaseous-Neon-Based Underground.
Future work Kamioka Kyoto We feel WIMP wind oh the earth NEWAGE ~ Direction Sensitive Direct Dark Matter Search ~ Kyoto University Hironobu Nishimura
K. Miuchi K. Miuchi July 10, 2008 Dark Matter and Dark Energy Direction-Sensitive Dark Matter Search --NEWAGE-- Kentaro Miuchi (Kyoto University) (New.
Underground Laboratories and Low Background Experiments Pia Loaiza Laboratoire Souterrain de Modane Bordeaux, March 16 th, 2006.
Bei Cai and Mark Boulay For the DEAP-1 Collaboration Queen’s University, Canada Pulse Shape Discrimination (PSD) in Liquid Argon from DEAP-1 APS meeting,
Institute of Experimental and Applied Physics Czech Technical University in Prague IEAP – CTU Prague 1 Current status and future development of neutron.
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.
Searching for Dark Matter with a Bubble Chamber Michael B. Crisler Fermi National Accelerator Laboratory 14 February, 2009.
WIMP search Result from KIMS experiments Kim Seung Cheon (DMRC,SNU)
? At Yangyang beach, looking for something in the swamp of particles and waves. 1 The recent results from KIMS Seung Cheon Kim (Seoul National University)
Kamioka Kyoto We feel WIMP wind on the earth NEWAGE Direction-sensitive direct dark matter search with μ-TPC * 1.Dark.
Dark Matter Search Results from the COUPP 4kg Bubble Chamber Russell Neilson for COUPP ICHEP 2012, Melbourne July 7, 2012.
DARK MATTER SEARCH Carter Hall, University of Maryland.
Second Workshop on large TPC for low energy rare event detection, Paris, December 21 st, 2004.
PyungChang 2006/02/06 HYUNSU LEE CsI(Tl) crystals for WIMP search Hyun Su Lee Seoul National University (For The KIMS Collaboration)
Detecting the Directionality of Dark Matter via “Columnar Recombination” (CR) Technique An attractive, natural candidate for Dark Matter is the WIMP –
Scintillating Bubble Chambers for Direct Dark Matter Detection Jeremy Mock On behalf of the UAlbany and Northwestern Groups 1.
Submergible Acoustic Transducers for Superheated Fluid Dark Matter Experiments Abstract: Abstract: Submergible Acoustic Transducers for the PICASSO Dark.
18-20 May 2015, Underground Science Conference, SDSM&T 1John Harton, Colorado State University Recent Results from the DRIFT Directional DM Experiment.
Alex Howard, Imperial College Slide 1 July 2 nd 2001 Underground Project UNDERGROUND PROJECT – Overview and Goals Alex Howard Imperial College, London.
WIMPs Direct Search with Dual Light-emitting Crystals Xilei Sun IHEP International Symposium on Neutrino Physics and Beyond
C OUPP is a series of progres- sively larger, refrigerant filled bubble chambers (from 50g to a proposed 500kg device) in the hunt to directly detect dark.
The PICASSO Dark Matter Search Experiment (Results and status) Ilan Levine Indiana University South Bend for the PICASSO Collaboration The 2006 Joint Meeting.
From Edelweiss I to Edelweiss II
Dark matter detection with bubble chamber detectors
Fast neutron flux measurement in CJPL
A Bubble Chamber for Dark Matter Detection
UK Dark Matter Collaboration
Simulation for DayaBay Detectors
Dark Matter Detection with Superheated Liquids
Harry Nelson UCSB DUSEL Henderson at Stony Brook May 5, 2006
CRESST Cryogenic Rare Event Search with Superconducting Thermometers
Irina Bavykina, MPI f. Physik
Status of Neutron flux Analysis in KIMS experiment
Yue, Yongpyung, Korea Prospects of Dark Matter Search with an Ultra-Low Threshold Germanium Detector Yue, Yongpyung, Korea
The Estimated Limits For A 5g LE-Ge Detector
Presentation transcript:

PICASSO, COUPP and PICO - Search for Dark Matter with Bubble Chambers Robert Filgas (on behalf of the PICO Collaboration) Institute of Experimental and Applied Physics (IEAP), Czech Technical University in Prague International Conference on New Frontiers in Physics, July 31 – August 6 2014, Kolymvari, Greece

C. Amole, M. Besnier, G. Caria, G. Giroux, A. Kamaha, A. Noble I. Lawson, E. Vázquez Jáuregui M. Ardid, M. Bou-Cabo, I. Felis D.M. Asner, J. Hall D. Baxter, C.E. Dahl, M. Jin, J. Zhang S. Gagnebin, C. Krauss, D. Marlisov, P. Mitra P. Bhattacharjee. M. Das, S. Seth R. Filgas, S. Pospisil, I. Stekl E. Behnke, H. Borsodi, O. Harris, I. Levine, E. Mann, J. Wells S.J. Brice, D. Broemmelsiek, P.S. Cooper, M. Crisler, W.H. Lippincott, M.K. Ruschman, A. Sonnenschein K. Clark F. Debris, M. Fines-Neuschild, C.M. Jackson, M. Lafrenière, M. Laurin, L. Lessard, J.-P. Martin, M.-C. Piro, A. Plante, O. Scallon, N. Starinski, V. Zacek J.I. Collar, R. Neilson, A.E. Robinson N. Dhungana, J. Farine, R. Podviyanuk, U. Wichoski D. Maurya, S. Priya

Superheated liquids Detection of elastic scattering of WIMPs on target nucleus Critical energy deposition within small volume induces bubble nucleation Advantages of bubble chambers: Insensitive to electron and gamma background Easily scalable to large sizes at reasonable cost Interchangeable liquids, excellent SD sensitivity Drawbacks: Threshold detectors – lack of direct energy measurement Sensitive to alpha radiation

PICASSO Acrylic container ø14 × 40 cm 4.5 liters 200 µm droplets 200 µm droplets of C4F10 dispersed in polymerised gel Droplets superheated at ambient temperature and pressure Operating temperature determines energy threshold (20 °C – 50 °C) Events recorded by 9 piezo-electric transducers Bubbles recompressed back to droplets by pressurization (6 bar) Low threshold Eth (45 °C) = 2 keV 4.5 liters 200 µm droplets of C4F10 Stainless steel frame 9 piezo-sensors

PICASSO 32 modules housed in 8 temperature and pressure control units Radiopure acrylic/steel vessels constructed at IEAP Total of 2.6 kg of active mass 40-50 hour runs of data-taking followed by 11 hours of recompression Located at SNOlab, Canada 2 km of rock and 50 cm of UPW shield against neutrons

PICASSO response At operating temperatures (< 50 °C) insensitive to electrons and gamma radiation Alpha particles are dominant background The acoustic signal from bubble formation is recorded and used for analysis Neutrons Alphas 50 GeV WIMPs Gammas, electrons

Neutron – alpha discrimination PICASSO pioneered the use of acoustic sensors to reject alphas Events initiated by alpha-decays include both long alpha tracks (~10 microns) and recoiling daughter nuclei - acoustic pulses are several times louder than those emitted by single nuclear recoil events > 99.4% alpha discrimination! Confirmed by COUPP detector

COUPP Superheated fluid contained within single pressure-controlled vessel Uses CF3I – probes both SD and SI sectors Cameras – excellent position reconstruction - able to identify multiple scattering events characteristic of neutrons Located at SNOLAB COUPP 4 kg -> PICO 2L 2013 – COUPP 60 kg

COUPP Energy threshold determined by pressure rather than temperature Rapid repressurization after each nucleation The detector consists of a quartz (synthetic fused silica) bell jar, a stainless steel diaphragm/bellows, seals, and highly purified fluids.

PICASSO + COUPP = PICO PICO combines operational principle of COUPP bubble chamber and fluid handling expertise from PICASSO Uses C3F8 better SD sensitivity due to higher fluorine concentration higher efficiency for detecting fluorine recoils lower threshold without gamma and electron background

PICO PICO 2L (former COUPP 4kg) running at SNOLAB Collaboration goal is to build PICO 250L - C3F8 or CF3I target fluid Background needs to be less than 1 event/year IEAP part of the material assay group to test U/Th contamination of all materials (dominant neutron source) and to devise Radon-cleaning facility (dominant alpha source)

PICO 2L VIDEO

Results Spin dependent Spin independent Results to be published soon: PICASSO run ended Dec 2013 COUPP 60 kg 1st run ended May 2014 PICO 2L 1st run ended May 2014

Extra Slides

SD and SI Reaction classified as spin-dependent (SD), when the sign of the scattering amplitude depends on the relative orientation of particle spin