New Experiments With Spheres The NEWS Project Bei Cai for the NEWS collaboration Queen’s University SNOLAB Users Meeting Symposium September 1-2, 2016 Spherical gas detector working principle Drift region Ampl region rs rc E≈V/r2*rs for rc>> rs Bei Cai • Large metallic sphere grounded • Small sensor (1-16 mm) in the center of detector on positive high voltage • Filled with gas mixture • Particle interaction creates electron-ion pairs in the gas • Electrons drift and create avalanches toward center of detector • Ions drift toward the ground and induce current/charge on the electrode • Measured signal is proportional to particle energy 2 Spherical gas detector Drift region Ampl region rs rc E≈V/r2*rs for rc>> rs Bei Cai • • • • Simple detector design Low radioactivity Very low energy threshold Low mass targets (H, He, Ne), sensitive to low-mass WIMPs • Flexible gas pressure and interchangeable sensor size • Single signal readout channel • Good energy resolution 3 Gas mixture • Noble gases, hydrogen and nitrogen have low electron attachment coefficients. Electrons continuously migrate • Quench gas is necessary – Avalanche is based on secondary ionization. However gas molecule may be raised to an excited state but not ionized. This excited state decays by photon emission. These photons interact with gas molecule and produce secondary electrons, which distort proportionality of the gas detector – Quench gas is added to absorb these photons. Often this quench gas is methane (CH4) Bei Cai 4 NEWS-LSM detector Located at Modane Underground Laboratory 4800 m.w.e. NEWS-LSM detector and shielding Low radioactivity copper, 60 cm diameter, 6 mm sensor Shields 4 to 7 cm Cu, 10 cm Pb, 30 cm PE Operation and data taking conditions • • • • • • • • Use of 3.1 bar Ne/CH4 mixture with 0.7% CH4 Energy to ionize a single electron in Neon w = 36 eV High Voltage on sensor set to 2520 V, no sparks Gain around 3000 Sealed mode, no recirculation Data taking continuously for 42 days 12.6 kg*day exposure Acquisition threshold set at around 50 eV, no noise in stable conditions • Loss of gain around 4% overall monitored with 210Po alpha line • Calibration in energy with 37Ar gas source (from (n,a) reaction on 40Ca) • Anticipated main backgrounds : – Compton (volume) – 210Pb decay products (surface) Comparison of simulation with AmBe neutron calibration data Pusle simulations include radial field and diffusion WIMP search data ROI Side bands for background (surface & Compton) used for preliminary analysis Show strong component of surface events in data “Conservative” analysis 1) Apply threshold cut at 150 eV 2) Simulations and side bands are used to determine volume and surface populations 3) Given expected shapes of background contributions in ROI, use Boosted Decision Tree analysis to determine cuts to optimize signal/background discrimination Expected sensitivity (SI) of the NEWS-LSM assuming events in ROI are pure backgrounds and behave in ROI as expected SuperCDMS Expected sensitivity of this experiment CRESST 2016 DAMIC Background free limit with present exposure LUX Limit set on spin independent coupling WIMPs with standard assumptions on WIMP velocities, escape velocity and with quenching factor of Neon nuclear recoils in Neon calculated from SRIM Inside a sound-proof room 15 cm stainless steel sphere (S15) NEWS at Queen’s Pressure transducer Gas line To vacuum pumps Detector sensor design HV2 HV1 Bei Cai 13 Raw pulse Gain/stability studies with Fe-55 X-rays Fe-55 6 keV X-rays Time bin (µs) Ne+2%CH4 500 mbar HV1 (ball) = 650 V HV2 (umbrella) = 72 V Alphas in S15 Ar+2%CH4, 1 bar HV1=1 kV, HV2=167 V Po-210 alpha rate < 3 mHz Po-210 2% energy [email protected] Po-218 Po-214 Bei Cai Integral of pulse 15 Laser calibration • Nitrogen gas laser produces UV photons • Photons extract surface atomic electrons from stainless steel sphere • Electron drift time and diffusion time measurements – to be compared with simulations with Magboltz • Single electron measurement • Looking into solid state laser to study stability of detector gain Bei Cai 16 Laser calibration N2 laser (60 electrons) Ne+2%CH4 200 mbar HV1 = 550 V HV2 = 69 V Fe-55 6-keV X-rays Amplitude (ADU) Bei Cai 17 Electron drift/diffusion time study • Timing difference between laser trigger pulse and gas detector signal electron drift time • Width of the distribution electron diffusion Peak @ 15 µs Sigma is 1 µs Ne+2%CH4 1 bar HV1 = 1050 V HV2 = 170 V Bei Cai 18 Two new prototype detectors at Queen’s 30 cm diameter high pressure stainless steel vessel and 50 cm diameter stainless steel sphere NEWS-SNO • • • • • 140 cm diameter copper sphere Operates up to 10 bar pressure Ne, He, CH4 gas mixture Clean copper: 1 uBq/kg uranium and thorium content Compact lead & polyethylene shield Lead shield Copper sphere Bei Cai 20 NEWS at SNOLAB NEWS-SNO will be located in the Cube Hall next to the DEAP-3600 and MiniCLEAN detectors MiniCLEAN 40 cm PE shield DEAP-3600 NEWS-SNO 35 ton lead shield Bei Cai 21 NEWS-SNO status • Detector and shield designs are finalized • Prototype copper sphere has been produced in France, samples sent to PNNL for radiopurity assay • Sensor design and test are ongoing • Gas handling system is being implemented and tested at Queen’s • Radioactive source and laser calibration system are being finalized • SNOLAB Gateway 2 review is scheduled for this October • Detector installation at SNOLAB is expected to start in fall 2017 Bei Cai 22 NEWS-SNO R&D programs Queen’s University • • • • • Single electron response study Gain stability Drift time & diffusion measurements Surface background (implanted alpha sources) study Calibration system and source deployment testing LSM • Internal surface cleanliness using high pressure water jet • Further data taking with He and H rich gas Grenoble • Quenching factor measurement with ion beams below 1 keV TUM • Gas scintillation properties & Laser studies PNNL • Plan for electroforming of copper vessel for future NEWS detector Bei Cai 23 Projected NEWS-SNO spin-independent WIMP sensitivity CDMSLite1 DAMIC CRESSTII H 2017 COGeNT He CDMSLite2 CDMS_Si DAMA NEWS-SNO CRESST Ne DarkSide50-Ar Edelweiss LE CDMS-Edelweiss CDMS reanalysis Xenon LUX Multi-ball ACHINOS structure Developed in Saclay in collaboration with University of Thessaloniki Volume electric field tuned by the structure and ball size Multichannel signal Detector segmentation, directionality for dark matter Bei Cai 25 Additional physics prospects • Neutrino-nucleus coherent elastic scattering – D. Z. Freedman, Phys. Rev. D, 9(1389) 1974 • Dedicated supernovae detector – Simple and cost effective - lifetime >>1 century – Could be a worldwide network of several of such dedicated Supernova detectors. To be managed by an international scientific consortium and operated by students – Y. Giomataris, J. D. Vergados, Phys. Lett. B, 23(634) 2006 • Competitive double beta decay experiment with Xe-136 at 50 bar – I. Giomataris, J. Phys. Conf. Ser., 309(2011) 012010 Bei Cai 26 Summary • NEWS-SNO is a spherical gas detector to be located at SNOLAB, sensitive to low mass WIMPs • Installation is expected to start in 2017 • 12.6 kg*day of neon data using a 60 cm low radioactivity prototype (NEWS-LSM) is currently being analyzed • Preliminary analysis results for WIMP sensitivity are promising and pave the way to the larger scale detector to be installed at SNOLAB • Gas characterization and calibrations are ongoing with small prototype detectors at Queen’s University Bei Cai 27 Collaboration meeting at Modane, France in April 2016 NEWS Collaboration • Queen’s University Kingston – GG, P di Stefano, R Martin, T Noble, B Cai, A Brossard, A Akamaha, P Vasquez dS, Q Arnaud, K Dering, J McDonald, M Clark, and summer students Copper vessel and gas set-up specifications, calibration, project management Gas characterization, laser calibration, on smaller scale prototype Simulations/Data analysis IRFU (Institut de Recherches sur les Lois fondamentales de l’Univers)/CEA Saclay -I Giomataris, M Gros, C Nones, I Katsioulas, T Papaevangelou, A Gigagnon, JP Bard, JP Mols, XF Navick, – Sensor/rod (low activity, optimization with 2 electrodes) – Electronics (low noise preamps, digitization, stream mode) – DAQ/soft LSM (Laboratoire Souterrain de Modane), IN2P3, U of Chambéry - F Piquemal, M Zampaolo, A DastgheibiFard – Low activity archeological lead – Coordination for lead/PE shielding and copper sphere Thessaloniki University – I Savvidis, A Leisos, S Tzamarias, C Elefteriadis, L Anastasios – Simulations, neutron calibration – Studies on sensor LPSC (Laboratoire de Physique Subatomique et Cosmologie) Grenoble - D Santos, JF Muraz, O Guillaudin – Quenching factor measurements at low energy with ion beams Technical University Munich – A Ulrich – Gas properties, ionization and scintillation process in gaz Pacific National Northwest Lab– E Hoppe – Low activity measurements, Copper electroforming Associated lab : TRIUMF - F Retiere June 2016 – Future R&D on light detection, sensor – – – • • • • • • •
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