status of the cosine-100 experiment at yangyang · 2017-07-18 · status of the cosine-100...

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.

+

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