Characterization of Large CaMoO4 crystals for 0n bb search

Slides:



Advertisements
Similar presentations
Status of Ultra-low Energy HPGe Detector for low-mass WIMP search Li Xin (Tsinghua University) KIMS collaboration Oct.22nd, 2005.
Advertisements

Tests of scintillators CsI, CsI(Na), BGO, NaI(Tl) CsI(Tl)
Solotvina Underground Laboratory
Nustar/crystal simulations B. Genolini Crystal: CsI(Tl) (Saint Gobain), wrapped with reflector (VM2000, Tyveck?) Geometry:
Absolute light output determination of crystal scintillators
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.
Report on SiPM Tests SiPM as a alternative photo detector to replace PMT. Qauntify basic characteristics Measure Energy, Timing resolution Develop simulation.
2004/Dec/12 Low Radioactivity in CANDLES T. Kishimoto Osaka Univ.
Recent status of dark matter search with ULE-HPGe detector Tsinghua University Qian Yue nd Korea-China Joint Seminar on Dark Matter Search.
Prospect of  experiment in Korea Presented by H.J.Kim Yonsei Univ., 10/25/2003 KPS 2003 fall meeting Contents 1) Introduction of 2) Theory and Experiments.
A study on CaMoO4 crystal coupled with LAAPD for neutrinoless double beta decay Sejong University Jung il LEE LEE J.I., BHANG H.C.1, CHOI J.H.1, KIM S.C.1,
Neutron Monitoring Detector in KIMS Jungwon Kwak Seoul National University 2003 October 25 th KPS meeting.
Internal background of CsI(Tl) crystal detectors for dark matter search Tae Yeon Kim Seoul National University For the KIMS Collaboration Seoul National.
T. Sugitate / Hiroshima / PHX031 / Nov.01 The Photon Spectrometer for RHIC and beyond PbWO 4 Crystal Density 8.29 g/cm 3 Radiation length 0.89 cm Moliere.
The current status of XMAS S Introduction Current status of prototype detector Next step Summary Cryodet 1 Y.Koshio for XMASS collaboration (Kamioka observatory,
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.
1 Satoshi Mihara for the   e  collaboration, review meeting at PSI, Jul 2002 Photon Detector Satoshi Mihara ICEPP, Univ. of Tokyo 1.Large Prototype.
Development of metal-loaded liquid scintillators for the double beta decay experiment 연세대 : 황명진, 권영준 서울대 : 곽정원, 김상열, 김선기, 김승천, 김태연, 명성숙, 방형찬, 이명재, 이직,
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.
Stefano Pirro – NuMass 2010 Stefano Pirro Double beta decay searches with enriched and scintillating bolometers - Milano - Bicocca The Future of Neutrino.
WIMP search Result from KIMS experiments Kim Seung Cheon (DMRC,SNU)
Status of KIMS Sun Kee Kim Seoul National University For the KIMS Collaboration KPS meeting, Oct. 22, 2004.
? 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)
1/27/2016Katsushi Arisaka 1 University of California, Los Angeles Department of Physics and Astronomy Katsushi Arisaka XAX 10.
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.
By Matthew Kauer First Year Report – 15 June 07 Measurement of 2b2ν Half-Life of Zr96 and Lightguide Studies for SuperNEMO Calorimeter Matthew Kauer UCL.
Current status of XMASS experiment 11 th International Workshop on Low Temperature Detectors (LTD-11) Takeda Hall, University of Tokyo, JAPAN 8/1, 2005.
1 Study of 48 Ca Double Beta Decay by CANDLES T. Kishimoto Osaka Univ.
June INPC20071 Study of 48 Ca double beta decay with CANDLES OGAWA Izumi ( 小川 泉 ) Osaka Univ. ( 大阪大学 )
Tin loaded liquid scintillator for the double beta decay experiment Presented by H.J.Kim, KIMS Yonsei Univ, 10/23/2002 Workshop on Underground and Astropparticle.
SrCl 2 crystal for EC/  + search Presented by J.H. So (KNU)
CsI Veto Detector Performance Study He Dao DMRC. Tsinghua University For KIMS Collaboration.
PyungChang 2006/02/06 HYUNSU LEE CsI(Tl) crystals for WIMP search Hyun Su Lee Seoul National University (For The KIMS Collaboration)
A simulation study on DBD search with pilot setup AMoRE - SNU jilee.
Development of CaMoO 4 Scintillation Crystals for the 0-  decay search 1.Introduction 2.CaMoO4 Crystal R&D 3.YangYang underground laboratory for KIMS.
DPF-JPS 2006 Oct 31, Hawaii 1 CANDLES system for the study of 48-Ca double beta decay T. Kishimoto Osaka Univ.
WP 22 – SciFi Development and Characterisation of Inorganic Scintillating Fibers Made of LuAG:Ce and LYSO:Ce S. Diehl 1, R. Novotny 1, Aubry Nicolas 2.
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.
CaMoO 4 at low temperature - LAAPD and PMTs - Woonku Kang, Jungil Lee, Eunju Jeon, Kyungju Ma, Yeongduk Kim Sejong University for KIMS collaboration Double.
Neutrinoless double beta decay (0  ) CdTe Semico nductor Band gap (eV) Electron mobility (cm 2 /V/s) Hole mobility (cm 2 /V/s) Density (g/cm 3.
Positronium intensity measurement preparation SNU Bongho Kim.
09/04/2006NDM061 CANDLES for the study of 48 Ca double beta decay OGAWA Izumi ( 小川 泉 ) Osaka Univ. ( 大阪大学 )
The Status of Hyperball-J Akio Sasaki Dept. of Phys. Tohoku Univ. 23/9/2011.
Current status of R&D on MMC and TES and a full size crystal test setup Sang-jun Lee Seoul National University.
Status of ULE-HPGe Experiment for WIMP Search in YangYang
ArchPbMoO4 scintillating bolometers as detectors to search for neutrinoless double beta decay of 100Mo Serge Nagorny INFN – Gran Sasso Science Institute,
from Saint Gobain studies
Fast neutron flux measurement in CJPL
On behalf of TEXONO collaboration
Institute for Scintillation Materials
Activities on double beta decay search at KIMS
Double Beta Decay Experiment with CaMoO4 crystal
Double Beta Decay of 48Ca with CaF2(Eu) - ELEGANT VI -
The Heidelberg Dark Matter Search Experiment
Serge Nagorny – GSSI-INFN
Status of 100Mo based DBD experiment
Natural CMO+HPGe experiment
R&D status & possible configuration of the 1st round experiment
2nd International Workshop on Double Beta Decay
Sr-84 0n EC/b+ decay search with SrCl2 crystal
Mo-92 EC/beta+ search with CaMoO4 crystal at Y2L
• • • Ge measurements for SuperNEMO
Development of metal-loaded liquid scintillators
Status of Neutron flux Analysis in KIMS experiment
Tadashi Nomura (Kyoto U), KRare05 at Frascati, Italy
Neutron Beam Test for Measuring Quenching Factor of CsI(Tl) Crystal
The 0-neutrino double beta decay search
Plan with new HPGe detectors
Presentation transcript:

Characterization of Large CaMoO4 crystals for 0n bb search Presented by H.J.Kim (KyungPook National U.) 2007/11/24 2nd Korea-China Joint workshop

Double beta work status Sn-124 excited state, Zn-64 study was published in Nuclear Physics A 2007. 0-n bb for Sn-124 with LSC physics draft is in progress (NIMA published in 2007) CaMoO4 study is on going : Mo-92: EC/b+ study in 4p CsI(tl) shielding +CaMoO4 background test (J.I.Lee’s talk) SrCl2 : EC/b+ study in 4p CsI(tl) (J.So) CeBr3 crystal development for EC/b+, b+b+, study (Gulrooh’s talk) Sn-112 resonant 0n ECEC study with HPGe

CaMoO4 Scintillation crystals 12.5 cm 2.2 cm Korea(2004) Ukraina(2006) Russia(2006) Russia(2007), ISTC Project

History CaMoO4 crystal R&D in very fast progress 1) 2002 : Idea and try to grow CMO in Korea 2) 2003 : Discussion with V.Kornokov => Send test CMO (better quality) 3) 2004 : CMO characterizations and Conference presentation Extended idea of XMoO4, low temp. CaMoO4 4) 2005-2007 : Large CMO with ISTC 5) 2006 : Discussion with F. Fanevich => CMO by Lviv and collaborative effort 6) 2007 : CMO R&D in low temp. started by SNU group 7) ……….

Crystal used for test Russia S1 22x22x30mm S0 10x10x10mm Large (L1) 12.5 cm 2.2 cm S1 22x22x30mm S0 10x10x10mm Large (L1) 22x22x125 XL1, 2 30x30x210 f38x20 mm Ukraine UK2 UK3

Clustering method with 400 Mhz FADC The same method with Darkmatter Search Total 42 ms window with 34 ms pulse window

# of Photoelectron/keV & Absolute light yield

# of PE with 60keV gamma CdWo4 :197+-19 S1 :28+-8 UK2 :37.5+-8

Number of photoelectron from 60keV g # of photoelecton from Am-241 Crystals tested 0.6-0.7PE/keV : Ukraine 0.4-6PE/keV : Russia 0.5PE/keV : Korea * The size of crystals are different 0.6 PE/keV => 6% FWHM at 3MeV (theoretical limit) 9

CaMoO4 small absolute light yield CsI(Tl) reference test Cs-137 source Gain:20 Shaping time:4us HV:1800V Peak:1597±34.4 Pedestal:33±10 Resolution(FWHM): 4.9% e-h pair = 37000. NP = 37000/0.8/0.9 = 51000 CaMoO4 S0 test Na-22 source Gain:100 peak time:12us HV:1800V Peak:520±116 e-h of CsI(Tl): 8.6±1% 4300±500ph/MeV Assume 15% QE,90% eff 0.6 ± 0.1 PE/keV Need more study * Tested with LLAPD (Details by M.J.Kim)

Attenuation Length& Relative light output with S1 & XL1, XL2

Large size CaMoO4 test - using two 3" PMT’s and attached at both end faces of CaMoO4 crystal. made small holes of few millimeter diameter at every 2cm distance in the teflon along the length wise direction of the crystal. 12.5 cm 2.2 cm PMT1 PMT2

Comparison between S1 and L1 CaMoO4 Light yield of Big CMO/ Small CMO is 90%

Energy spectrum of Am-241 Placed the Am-241 radioactive source at every 2cm mark Red= 2cm Green= 4cm Blue= 6cm Pink= 8cm Black= 10cm

Attenuation Length = ~ 30 cm

Larger (XL1, XL2) CaMoO4 test - XL1,XL2 crystals were used for test. - using one 3" PMT (green extended) and one 2" PMT (bi-alkali) of CaMoO4 crystal. made small holes of few millimeter diameter at every 3cm distance

a test with S1 & XL1, XL2 XL1 : ~70% of S1, XL2 : ~80% of S2

3” PMT side with Cs-137

L1-CMO

L2-CMO

Resoultion & light output comparison with S1 and UK2,UK3

Checking energy resolution with CdWO4 Energy resolution of 9%

Cs137 source with CMOs and CdWo4

Cs-137 with S1 and UK2, UK3 Relative light yield ; 1.2 : 1.9 : 2.0

Different fitting, different results The best way is subtract background from data and fold MC data with data with Gausian fit only

S1 with Gaussian+Exp 18% FWHM

Mean time distribution of CMOs

Summary Different size of CMO crystals from Russia (ISTC project) and Ukraine are being tested # of photoelectron/keV, absolute light yield and attenuation length are measured Relative light output and energy resolution were compared.

Work list before experiment Resolution and light yield issue ->Different crystal results need to be resolved Test with the same size of LU3 and XL1 Improve light output… ->Further study of LAAPD : LAAPD or PMT? -> How low temperature is necessary? -> Size of CMO optimization Internal Background issue -> measurement UK3 (results) XL (soon…) => Shielding optimization for VETO Enriched 100Mo, purification, growing issues Low temp Det., XMoo4 (X->?)

Backgrounds and signal for 20kg of CaMoO4 with 5 years data taking (GEANT4) Sensitivity 10kg (100Mo) 5% FWHM resolution 0.05 mBq/kg for 208Tl, 214Bi 5 years  7.1x1024 y (90% CL) ( 0.18~0.71 meV) Mo-100 2n Ca-48 2n Signal (m=0.4eV) Bi-214 Tl-208 10s significance Current best limit on 100Mo : 4.6x1023 by NEMO3 with 6.9kg 100Mo Claim by Klapdor-Kleingrothaus et al.  ~ 400 meV  Assuming optimistic theoretical value

Thank you

New Crystal for Am-241 Distance Mean of det00 (2” PMT) Mean of det01(3” PMT) 1 15390 10960 3 14880 10950 6 14740 10990 9 14630 10930 12 14390 10610 15 13880 11398 18 15120 9494 Old Crystal for Am-241 Distance Mean of det00(2” PMT) Mean of det01(3” PMT) 1 12810 9370 3 11280 9785 6 10910 9784 9 10890 9695 12 10530 9757 15 9663 10460 18 11790 8416