status of the cosine-100 experiment at yangyang · 2017-07-18 · status of the cosine-100...
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Status of the COSINE-100 experiment at Yangyang
Chang Hyon HaOn behalf of the COSINE collaboration
Chang Hyon Ha, Center for Underground Physics, IBS ICRC2017, Busan, July.12-20
8 low-radioactive NaI(Tl) crystals, 106 kg in total, submerged in 2 tons of liquid scintillator.
Physics run started Sept. 2016
Motivation : DAMA annual modulation signal, to be checked with independent measurements with the
same NaI(Tl) target material
Dark Matter Modulation 9.2 sigma
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Modulation between 2-6 keV
Background : ~1 count/day/kg/keV
(dru=differential rate unit) above 2 keV
NDM15
Eur. Phys. J. C (2010) 67: 39-49NIMA 592 (2008) 297
Chang Hyon Ha, Center for Underground Physics, IBS ICRC2017, Busan, Jul. 12-20
• Every scientific results should be reproducible, independently.
• Apple-to-apple comparison is necessary.
• Large crystal detector experience helps, and community supports.
Motivation : Right thing to doPhys. Rev. D 94, 122001
3Chang Hyon Ha, Center for Underground Physics, IBS ICRC2017, Busan, Jul. 12-20
COSINE-100 experiment
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Joint collaboration between KIMS and DM-Ice to search for dark matter interactions in NaI(Tl) scintillating crystals.
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Chang Hyon Ha, Center for Underground Physics, IBS ICRC2017, Busan, Jul. 12-20
Shields, Vetoes, and µ-counters
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Plastic Scintillators for CR Muons3-cm thick, 37 panels
20-cm thick lead shielding
3-cm thick Cu box
40-cm active Liquid Scintillator veto
NaI crystals2-inch PMTs
5-inch PMTs
3-inch PMTs
Neutron Detector
40 cm
Chang Hyon Ha, Center for Underground Physics, IBS ICRC2017, Busan, Jul. 12-20
Construction TimelineDec. 2015 Jan. 2016 Feb. 2016
Mar. 2016 Apr. 2016
May. 2016 Sep. 2016Jun. 2016
6Chang Hyon Ha, Center for Underground Physics, IBS ICRC2017, Busan, Jul. 12-20
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COSINE-100 detector setup
Chang Hyon Ha, Center for Underground Physics, IBS ICRC2017, Busan, Jul. 12-20
COSINE-100 Operation
Very stable operation More than 85% of physics data.
95% are good runs. Roughly 8 months data
are collected
Crystal Trigger Rate (13 Hz)
Muon Detector Rate (12 Hz)
Calibration
Chang Hyon Ha, Center for Underground Physics, IBS ICRC2017, Busan, Jul. 12-208
8 NaI(Tl) Crystals
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8 crystals with a total mass of 106 kg Internal background components are measured.
Average light yield ~15 PE/keVU/Th/K contaminations are below DAMA value.
210Po (210Pb) is still higher than DAMA.
Preliminary
3-inch PMT
35% QE
Chang Hyon Ha, Center for Underground Physics, IBS ICRC2017, Busan, Jul. 12-20
Crystal-LS Coincidence
• 40K emits 1460 keV gamma with 3 keV Auger electron energy deposition in NaI crystal
• Tagging 1460 keV events with LS enables to veto 3 keV background events (70% tagging efficiency)
γ (1460 keV)
Liquid Scintillator
40Ke- (3 keV)
3 keV 40K peaks
Preliminary
+ Data (vetoed) – Fit – Subtracted 40K
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Poster :: DM013, Govinda AdhikariChang Hyon Ha, Center for Underground Physics, IBS ICRC2017, Busan, Jul. 12-20
CR Muon detector systemCOSINE-100 Preliminary
gamma backgroundCR Muons
Muon flux monitor. CR muon induced crystal
events are vetoed when muon pass through it.
4x10-7/cm2/s
COSINE-100 Preliminary
Poster :: DM017, Hafizh PrihtiadiChang Hyon Ha, Center for Underground Physics, IBS ICRC2017, Busan, Jul. 12-2011
Low Energy Spectrum (210Pb bkg.)
Internal components (crystal growing/raw material) : 210Pb (t1/2=22yr), U/Th External components (handling of crystal/material assay) 210Pb on the surface Cosmogenic components (excitation) : 125I (59d), 109Cd-109 (460d), 3H (12yr)
2-20 keV2-100 keV
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2-4 dru (counts/day/kg/keV) between 2-6 keV
DAMA 1 dru
Chang Hyon Ha, Center for Underground Physics, IBS ICRC2017, Busan, Jul. 12-20
Understanding single-site event spectrum— data— sim
210Pb (bulk)210Pb (surf) 125I
109Cd
210Pb (PTFE,Cu)
3H
Currently, 10-15% discrepancy at the ROI Goal <5%
COSINE-100 Preliminary
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Poster :: DM012, Pushparaj Adhikari
Chang Hyon Ha, Center for Underground Physics, IBS ICRC2017, Busan, Jul. 12-20
Expected Sensitivity for COSINE-100
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*Assumed 2 dru or 4 dru flat backgrounds depending on crystals.
The sensitivity should be comparable with the DAMA allowed region.
Chang Hyon Ha, Center for Underground Physics, IBS ICRC2017, Busan, Jul. 12-20
COSINE-200 (Phase-II)
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Goal : Reaching background lower than DAMA (1 dru). a factor two or more improvement is needed.
Powder purification (Recrystallization)
Crystal growing & HandlingEstablished a facility at our
centerPowder purification
(mass production facility for purification under
construction)Chang Hyon Ha, Center for Underground Physics, IBS ICRC2017, Busan, Jul. 12-20
Expected sensitivity for COSINE-200 (Phase-II)
Chang Hyon Ha, Center for Underground Physics, IBS ICRC2017, Busan, Jul. 12-2016
*Assumed 1 dru flat backgrounds
Conclusion & Outlook
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• KIMS and DM-Ice join forces (the COSINE-100 collaboration) to reproduce DAMA annual modulation using the same NaI(Tl) target material.
• COSINE-100 (Phase-I) is running with 106 kg of NaI(Tl) crystals.
• CR muon tagging and liquid scintillator tagging.
• Physics run started on September 2016
• Initial performance of COSINE-100 is promising. 2 keV thres., 2-4 dru at ROI
• Expect to have DAMA-comparable sensitivity in ~2 years
• Continued R&D for higher purity crystals for COSINE-200 (Phase-II)
Chang Hyon Ha, Center for Underground Physics, IBS ICRC2017, Busan, Jul. 12-20
BACKUP
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Environmental control/monitoringTemperature
Humidity
• < 0.1˚C temperature fluctuation on the crystals in LS
• more than 150 environmental variables are monitored online
Current/VoltageChang Hyon Ha, Center for Underground Physics, IBS ICRC2017, Busan, Jul. 12-20
High Energy Spectrum100-2000 keV
— data— sim
U/Th/K/Cosmogenics
20Chang Hyon Ha, Center for Underground Physics, IBS ICRC2017, Busan, Jul. 12-20
Liquid Scintillator for COSINE-100 is ready
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3000 liters of liquid scintillators
Purification Setup (Humidity removal)
Linear alkylbenzene (LAB) : Good optical/radioactive properties
2,5-Diphenyloxazole (PPO) : fluor, scintillator/wavelength shifter
p-bis-(o-methylstyryl)-benzene (bis-MSB) : wavelength shifter
Ready to be filled
U238 < 7 ppt Th232 < 4 ppt
Rn222 daughters
This background of the liquid scintillator
contributes negligible amount to the crystal (<0.01 dru)
Chang Hyon Ha, Center for Underground Physics, IBS ICRC2017, Busan, Jul. 12-20
Global NaI(Tl) efforts
ANAIS @ Canfranc
DAMA/LIBRA @ LNGS
SABRE @ LNGS
DM-Ice17 @ South Pole
COSINE-100 @ Y2L
PICO-LON @ Kamioka
SABRE @ Stawell
22Chang Hyon Ha, Center for Underground Physics, IBS ICRC2017, Busan, Jul. 12-20
Event selection efficiency measured with 60Co Compton beta events
Above 2 keV, more than 90% selection efficiency Hardware trigger threshold ( 0.14 keV )
LS
Beta spectrum obtained by multiple-site events using 60Co source
Ratio of event selection applied to triggered events
COSINE-100 Preliminary
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Poster :: DM027, Hanwool JooChang Hyon Ha, Center for Underground Physics, IBS ICRC2017, Busan, Jul. 12-20