University of South Dakota

Slides:



Advertisements
Similar presentations
Dante Nakazawa with Prof. Juan Collar
Advertisements

1 Aaron Manalaysay Physik-Institut der Universität Zürich CHIPP 2008 Workshop on Detector R&D June 12, 2008 R&D of Liquid Xenon TPCs for Dark Matter Searches.
NEST: Noble Element Simulation Technique Modeling the Underlying Physics of Noble Liquids, Gases Matthew Szydagis, UC Davis UCLA DM 02/28/14 1
Status of XMASS experiment Shigetaka Moriyama Institute for Cosmic Ray Research, University of Tokyo For the XMASS collaboration September 10 th, 2013.
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:
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,
Report from Low Background Experiments Geant4 Collaboration Workshop 10 September 2012 Dennis Wright (SLAC)
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.
PANDAX Results and Outlook
Search for Dark Matter at CJPL with PANDAX
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.
Form Factor Dark Matter Brian Feldstein Boston University In Preparation -B.F., L. Fitzpatrick and E. Katz In Preparation -B.F., L. Fitzpatrick, E. Katz.
ZEPLIN II Status & ZEPLIN IV Muzaffer Atac David Cline Youngho Seo Franco Sergiampietri Hanguo Wang ULCA ZonEd Proportional scintillation in LIquid Noble.
CRESST Cryogenic Rare Event Search with Superconducting Thermometers Max-Planck-Institut für Physik University of Oxford Technische Universität München.
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.
Annual Modulation Study of Dark Matter Using CsI(Tl) Crystals In KIMS Experiment J.H. Choi (Seoul National University) SUSY2012, Beijing.
Direct Dark Matter Searches
Neutron Monitoring Detector in KIMS Jungwon Kwak Seoul National University 2003 October 25 th KPS meeting.
Neutron scattering systems for calibration of dark matter search and low-energy neutrino detectors A.Bondar, A.Buzulutskov, A.Burdakov, E.Grishnjaev, A.Dolgov,
Dark Matter Search with SuperCDMS Results, Status and Future Wolfgang Rau Queen’s University.
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,
The Recent Status of KIMS Group and New Plan Li Xin (Tsinghua University) KIMS collaboration Aug. 28th, 2006.
J.T. White Texas A&M University SIGN (Scintillation and Ionization in Gaseous Neon) A High-Pressure, Room- Temperature, Gaseous-Neon-Based Underground.
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.
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.
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.
The dual light-emitting crystals detector for WIMPs direct searches TIPP2014, Amsterdam 1 Xilei Sun (presented by Yuguang Xie) IHEP, Beijing, China.
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.
WIMP search Result from KIMS experiments Kim Seung Cheon (DMRC,SNU)
Direct search of a dark matter with NaI: current status and possible perspective Dzhonrid Abdurashitov Institute for nuclear research, Moscow
? 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)
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.
Current status of XMASS experiment 11 th International Workshop on Low Temperature Detectors (LTD-11) Takeda Hall, University of Tokyo, JAPAN 8/1, 2005.
DARK MATTER SEARCH Carter Hall, University of Maryland.
Characterization of the QUartz Photon Intensifying Detector (QUPID) Artin Teymourian UCLA Dark Matter Group Dept. of Physics and Astronomy.
I. Giomataris, CEA-Irfu-France
1 A two-phase Ar avalanche detector with CsI photocathode: first results A. Bondar, A. Buzulutskov, A. Grebenuk, D. Pavlyuchenko, R. Snopkov, Y. Tikhonov.
PyungChang 2006/02/06 HYUNSU LEE CsI(Tl) crystals for WIMP search Hyun Su Lee Seoul National University (For The KIMS Collaboration)
SuperCDMS From Soudan to SNOLAB Wolfgang Rau Queen’s University 1W. Rau – IPA 2014.
The Princeton NaI Experiment (SABRE) Frank Calaprice Princeton University Cosmic Frontier Workshop SLAC March
1 CRESST Cryogenic Rare Event Search with Superconducting Thermometers Jens Schmaler for the CRESST group at MPI MPI Project Review December 14, 2009.
Low Mass WIMP Search with the CDMS Low Ionization Threshold Experiment Wolfgang Rau Queen’s University Kingston.
Andrey Sokolov Novosibirsk State University (NSU) Budker Institute of Nuclear Physics (Budker INP) Novosibirsk, Russia Two-phase Cryogenic Avalanche Detector.
CaMoO 4 at low temperature - LAAPD and PMTs - Woonku Kang, Jungil Lee, Eunju Jeon, Kyungju Ma, Yeongduk Kim Sejong University for KIMS collaboration Double.
CRESST Cryogenic Rare Event Search with Superconducting Thermometers Max-Planck-Institut für Physik University of Oxford Technische Universität München.
Study of the cryogenic THGEM-GPM for the readout of scintillation light from liquid argon Xie Wenqing( 谢文庆 ), Fu Yidong( 付逸冬 ), Li Yulan( 李玉兰 ) Department.
WIMPs Direct Search with Dual Light-emitting Crystals Xilei Sun IHEP International Symposium on Neutrino Physics and Beyond
Leo Stodolsky 80th anniversary
SuperCDMS and CUTE at SNOLAB
SuperCDMS and CUTE at SNOLAB Wolfgang Rau Queen’s University for the
From Edelweiss I to Edelweiss II
Status of ULE-HPGe Experiment for WIMP Search in YangYang
SuperCDMS Energy-scale, Resolution, and Sensitivity
A Bubble Chamber for Dark Matter Detection
Functional test of a Radon sensor based on a high resistivity silicon BJT detector G.-F. Dalla Betta et al. A battery-powered,
COHERENT at the Spallation Neutron Source
SuperCDMS at SNOLAB Wolfgang Rau Queen’s University for the
CRESST Cryogenic Rare Event Search with Superconducting Thermometers
Irina Bavykina, MPI f. Physik
XAX Can DM and DBD detectors combined?
CsI Compton Veto Detector for A low Mass WIMP Experiment
Dark Matter Search with Stilbene Scintillator
BINP:Two-phase Cryogenic Avalanche Detector (CRAD) with EL gap and THGEM/GAPD-matrix multiplier: concept and experimental setup Concept: Detector of nuclear.
LUX: Shedding Light on Dark Matter
LUX: A Large Underground Xenon detector WIMP Search
Yue, Yongpyung, Korea Prospects of Dark Matter Search with an Ultra-Low Threshold Germanium Detector Yue, Yongpyung, Korea
Neutrino Magnetic Moment : Overview
The Estimated Limits For A 5g LE-Ge Detector
Presentation transcript:

University of South Dakota Supported by NSF PHY-1506036 JSPS Grant-in-Aid(B) 26800122 Pure NaI/CsI at Cryogenic Temperatures for Rare-Event-Search Experiments Science@SURF Rapid City, May 14, 2017 Jing Liu University of South Dakota

Science@SURF, Rapid City Beyond G2 DAMA: still to be verified! Sub-GeV: Dark sector Less than $10M Low threshold Electronic recoil G2: Main target: WIMP More than $10M Large mass Nuclear recoil May 14, 2017 Science@SURF, Rapid City

Science@SURF, Rapid City DAMA Energy spectrum of NaI(Tl) from DAMA NaI/CsI based effort: COSINE DM-ICE KIMS ANAIS SABRE etc. X-rays/Auger electrons from Ar-40, the daughter of K-40 EC-decay How about here? Focus: Location Purification Active shield PMT Light collection May 14, 2017 Science@SURF, Rapid City

Low energy threshold  high light yield Higher light yield with still the SAME crystal? May 14, 2017 Science@SURF, Rapid City

Light yield as a function of temperature Eur. Phys. J. C (2012) 72:2061 Phys. Rev. B 5 (1995) 2195 Part of CRESST LY of Pure NaI VS Temperature May 14, 2017 Science@SURF, Rapid City

History of studies of pure NaI/CsI Inconsistent results on absolute light yield, the best are about twice higher than those of doped ones at RT May 14, 2017 Science@SURF, Rapid City

Science@SURF, Rapid City Light readout devices Light loss in complicated readout system cancels out the gain from light yield  PMT at RT Light guide Crystal at LNT Light guide PMT at RT PMTs working at 77 K (Hotta, DM2014) May 14, 2017 Science@SURF, Rapid City

Proof-of-concept measurement R8778MODAY (AR) CsI PTFE wrapped side surface Bottom CF flange NaI May 14, 2017 Science@SURF, Rapid City

Energy calibration of a pure CsI crystal Room temperature 77 K May 14, 2017 Science@SURF, Rapid City

Science@SURF, Rapid City Light yields QE of the PMT quoted by Hamamatsu at room temperature is 29.5% at 300 nm = Light collection efficiency (A rough estimation) 77 K Room temperature May 14, 2017 Science@SURF, Rapid City

Science@SURF, Rapid City Trigger efficiency 50% photon PMT PMT May 14, 2017 Science@SURF, Rapid City

Science@SURF, Rapid City Trigger efficiency COSINE achieved 15 PE/keV with NaI(Tl) at RT -> There is still room for us to improve! 20 PE/keVee 30 PE/keVee May 14, 2017 Science@SURF, Rapid City

CEvNS event rate VS nuclear recoil energy J. Collar et al. NIM A773 (2015) 56–65 MINER COHERENT May 14, 2017 Science@SURF, Rapid City

Dark matter sensitivity at 77 K arXiv:1607.01009 Good chance to verify DAMA  No chance for sub-GeV DM  LY of DAMA: ~ 8 PE/keV Another Raymond Davis?! Have to use TES for 100% QE Zero dark count  no coincident requirement Phonon readout as well  particle identification arXiv:1512.03506 May 14, 2017 Science@SURF, Rapid City

Science@SURF, Rapid City Sensitivity with TES TES for 100% QE  ~ 60 PE/keV @ mK Zero dark count  no coincident requirement  100% trigger eff. arXiv:1607.01009 Assume 10% DAMA background: 0.1 cnt/kg/day/keV  ~ 0.3 cnt/kg/year/eV May 14, 2017 Science@SURF, Rapid City

Science@SURF, Rapid City Phased approach Phase I, physics focus: CEvNS, technical focus: light yield CsI + PMT for MINER background Quenching factor measurement @ TUNL NaI/CsI + PMT/SiPM for CEvNS with MINER/COHERENT NaI/CsI + TES for CEvNS with MINER Phase II, physics focus: DAMA, technical focus: low background CsI/NaI + PMT/SiPM + liquid argon/neon active veto Collaborating with COSINE/SABRE for radio-pure crystals Phase III, physics focus: sub-GeV DM, technical focus: integration CsI/NaI + TES for photon only or photon + phonon Collaborating with SuperCDMS $20k (new crystals, photon sensors) $30k, 3 kg radio-pure crystals $24k, 3 pairs of PMTs/SiPM $100k, cryostat $100k, shielding $100k (new crystals, TES, integration) May 14, 2017 Science@SURF, Rapid City

Science@SURF, Rapid City Phase II @ SURF?! SURF Infrastructure LN2 SDSMT Radon control Surface background control BHSU Screening facility USD Shielding and muon veto Light sensors and crystals Electronics Potentially mK refrige + TES Overall budget << $0.5 M with SD collaborators alone! Support from community at large makes it even easier. May 14, 2017 Science@SURF, Rapid City

Science@SURF, Rapid City Summary A rather conventional approach with guaranteed physics results A bit novelty each step forward with great physics potential A rather conventional approach with guaranteed physics results A bit novelty each step forward with great physics potential Credit: US Cosmic Vision: New Ideas in Dark Matter, Maryland, March 2017 May 14, 2017 Science@SURF, Rapid City

Single-photoelectron response of the PMT May 14, 2017 Science@SURF, Rapid City

Science@SURF, Rapid City Ideal case arXiv:1607.01009 Assuming TES + SuperCDMS cavity: Photon + phonon Multiple targets May 14, 2017 Science@SURF, Rapid City

Science@SURF, Rapid City May 14, 2017 Science@SURF, Rapid City

Science@SURF, Rapid City Measurement of QE change from room temperature to 77 K using an LED with fixed light intensity: May 14, 2017 Science@SURF, Rapid City

Science@SURF, Rapid City LY = 20 PE/keV, @ 0.1 keV May 14, 2017 Science@SURF, Rapid City

Science@SURF, Rapid City https://indico.cern.ch/event/491882/contributions/2308724/attachments/1378313/2093996/CosPA2016_Pushpa.pdf May 14, 2017 Science@SURF, Rapid City

Science@SURF, Rapid City May 14, 2017 Science@SURF, Rapid City

Science@SURF, Rapid City May 14, 2017 Science@SURF, Rapid City

Science@SURF, Rapid City arXiv:1612.06071 May 14, 2017 Science@SURF, Rapid City