Low background DBD search in CANDLES

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Low background DBD search in CANDLES Takashi Iida (Osaka) for the CANDLES collaboration 2016 Nov. 8 th DBD16 @Osaka University

Outline The CANDLES experiment Progress from the last DBD Background and its reduction Sensitivity for 0nbb Future R&D Summary 2

20 PMT Acrylic LS tank CaF2 crystal Stainless Water tank 13 PMT 3D picture T. Iida CAlcium fluoride for studies of Neutrino and Dark matters by Low Energy Spectrometer

Double beta decay sensitivity KamLAND 0nbb search with 136 Xe World best limit on 0nbb T1/2 > 1.1 10 26 [year] mbb < 61 165 mev CANDLES 0nbb search with 48 Ca Current sensitivity on 0nbb T1/2 ~ 10 22 [year] Aim for below IH region by making a breakthrough in future!!

What s breakthrough? Since 0nbb is very rare signal, we need to achieve stringent conditions. Low background level Q-value of 48 Ca (4.27MeV) is highest among all the 0nbb candidates and therefore low background (BG) level is naturally possible. In addition, active veto by LS and additional shield can reduce more BGs. Good energy resolution For separating 0nbb and 2nbb. Current energy resolution is s~2% @4.27MeV. Plan to develop CaF2 Bolometer (s~0.3%) for future. Large volume Natural abundance of 48 Ca is 0.2%. Developing 48 Ca enrichment technique. Mainly focus on BG today!! Now we ve achieved enrichment with factor of 6 by MCCCE method. T. Kishimoto et al., Prog. Theor. Exp. Phys. 033D03 (2015)

The CANDLES-III (U.G.) detector Experiment is located in Kamioka, Japan. Schematic view CaF2 (pure) scintillator τ 1msec 10 10 10 cm3 96 crystals 300 kg 2m3 Liquid scintillator τ 10nsec Liq. scintillator Water Active veto using different time constant!! Cylindrical water tank (φ3m h4m) 62 Photomultipliers PMT 13 inch PMT R8055 48 20 inch PMT R7250 14 Light collection system Al sheet Reflectance ~93% @ 420nm Light pipe CaF2 PMT 6

The CANDLES (U.G) detector in Kamioka observatory CaF2 crystals 4m 3m CANDLES III detector PMT & Light pipe 7

4p active veto by Liquid scintillator (LS) - Rejection of external g ray background Pulse shape information by 500 MHz Flash ADC. Distinguish event type by offline pulse shape analysis taking advantage of different decay time. Detail of analysis method is explained later. bb signal!? External g BG External g BG CaF 2 (1msec) CaF 2 + Liquid Scintillator Liquid Scintillator (~10nsec) b-ray g-ray CaF 2 CaF 2 Liquid Scintillator CaF 2 Liquid Scintillator 8

Background spectrum in CANDLES Stainless Energy [kev] Even after LS cut, there exist background in high energy region above 4MeV. BG spectrum has peak around 7.5MeV. This BGs seem to be produced from neutron capture on surrounding material (n,g).

2m Neutron source run In order to confirm that our assumption is correct, 252 Cf neutron source was set on the detector and data was taken in 2014. Spectra for neutron source run and physics run are consistent. MC simulation of (n,g) can well reproduce the BG spectrum. We identified main BG as (n,g)!!

Shield for (n,g) background reduction CANDLES shield overview n g CANDLES tank Pb shield (7-12cm) Reduce g-ray from surrounding rock Effect of Pb (n,g) is one order smaller than that of stainless tank Boron sheet (4-5mm) Reduce n captured by stainless tank (n,g) BGs in CANDLES is expected to become 1/80 by MC. Expected number of backgrounds after shield installation: Rock : 0.34±0.14 event/year Tank : 0.4±0.2 event/year

Pb shield construction Pb shield construction was started from March 2015. All the collaborators worked very hard! I used even professors like a horse ;) Side Pb shield Top Pb shield Bottom Pb shield 12

B shield construction Neutron shield (B sheet) installation. B4C 40wt% Silicone rubber (B sheet) Outer sheet Inner sheet Liq. type Bottom 4-5mm thickness. Covered 100m 2 area For bottom B shield, liquid type was poured on top of the Pb. This is for both shielding neutron and waterproofing the bottom Pb blocks. B and Pb elution into water have been checked periodically after water filling. 13

PMT reinstallation 10inch PMT Fast time response. Twelve 10inch PMTs are installed for performance study. 13 inch PMT 14

Material change near CaF2 crystal Data Total BG (MC) Material near crystal Neutron capture g-ray 2nbb 208 Tl 212 Bi- 212 Po Radioactivity measurement with Ge detector indicated that Al sleeve and O-ring are dirty. We replaced them with new ones which are expected to be cleaner during shield construction. BG in 3 3.5 MeV is expected to decrease about less than half.

Top of the detector after the top Pb shield was closed. Cabling Tank assembly Collaboration meeting @Toyama Construction finished in May 2016!!

2m Events/50keV/44.6hours Neutron source run again! New 252 Cf source data was taken in June 7 th 14 th in order to check performance of the shield with same setup. To compare with high statistics, loose LS cut was applied. (n,g) with 252 Cf was decreased by ~1/70!! This reduction is similar to we expected from MC. Since reduction for fast neutron is worse than for thermal neutron, reduction factor is not exactly same as expected. Fe (n, γ) Before shield After shield ~1/70 Ni or Cr (n, γ) Energy [kev]

Events/50keV/56.9d Energy spectra of physics run after loose LS cut External g-ray reduced by the shield Data in 2014 (56.9 days) After cooling (28.1 days) After shielding (21.5 days) 3 4 MeV was reduced due to changing O-ring and Al sleeve. (n,γ) with environmental neutron was reduced by the shield!! ~1/100 Internal radioactive BGs ( 208 Tl & Bi-Po) Qbb region Energy [kev]

Remaining backgrounds and reduction After shielding external BGs were reduced about two order. Remaining BGs is originating from internal radioactivity of Th chain ( 208 Tl and 212 Bi- 212 Po). 2nbb is not serious BG in current sensitivity. (it will be major BG after 48Ca enrichment) We reject remaining BGs by analysis. b+a decay Qvis=5.3MeV T1/2=300ns b+g decay Q=5MeV

Th activity [mbq/kg] Position reconstruction and crystal selection Position of each event is reconstructed by weighted mean of observed charge in each PMT. σ Npe(i) PMT(i) Crystal separation is ~7s peak to peak. σ Npe(i) Crystal selection criteria is within 3s from the peak. 27 clean crystals (Th contamination < 10 mbq/kg) out of 96 crystals are selected and the results are compared to all crystals. ±3s X axis [mm]

Pulse shape discrimination Pulse shape a/b are different in CaF2 scintillator and LS has also very different shape. Make reference pulse for each event type (a / b / LS). Chi2 fitting each reference pulse to the data and identify which event type is most likely event by event. Data a reference b reference b + LS event

Bi-Po event cut 212 Bi- 212 Po sequential decay has enough short half-life (T1/2=300ns) to be included in one event (4 msec). It can be a BG in Qbb region since its total visible energy is 5.3 MeV at maximum. Pulse shape analysis can remove this background and effect to 0nbb search is negligibly small for now. Typical Bi-Po event Prompt b Delayed a

208Tl event cut Th 系列 232 Th 212 Bi T 1/2 =60.6m Q a = 6.21MeV a 208 Tl T 1/2 =3.05min Q b = 5.00MeV b 208 Pb stable a-b 崩壊 Eneryg spectrum of prompt events 212Bi candidate Accidental event 212Bi candidate-accidental T½ = 178±55sec Delayed : 3.1-5MeV Time gate : ~180sec 1. Find parent 212Bi a-decay candidate by pulse shape analysis. 2. Apply 12min veto from 212Bi candidate in the same crystal.

208 Tl multi-hit event cut 208 Tl multi-hit event 3min. 1. 212 Bi nucleus undergo alpha decay. 2. After ~3min. 208 Tl undergo b+g decay. 3. g-ray go outside and detected in different crystal. 4. In this case, a and b are reconstructed in different crystal due to deposit energy. In order to remove multi-hit event as well as single hit, we tried to apply veto not only for the same crystal, but also for the neighboring crystals. Although this cut is powerful to remove 208 Tl BG, signal efficiency become worse due to many accidental coincidence. Now we are under studying and improving cut method.

Energy spectrum at each reduction 27 Crystal All crystal Qbb No cut Bi-Po cut LS cut (PSD) 208Tl cut Multi crystal cut Qbb

Sensitivity for 0nbb in 1 year Sensitivity is calculated from expected BGs. Data set : 21.5 days after shielding Qbb region: 4170-4480 kev (Qbb -1s +2s) Without multi-hit cut With multi-hit cut 27 crystals All crystals 27 crystals All crystals # of ev @Qbb 1 5 0 0 Expected 208 Tl 0.22 2.2 0.14 1.4 Expected (n.g) 0.01 0.04 0.01 0.04 Sig. eff. 0.46 0.30 Sensitivity @1y 0.7 10 23 [y] 1.0 10 23 [y] 0.5 10 23 [y] 0.9 10 23 [y] Sensitivity of CANDLES for 0nbb after 1 year is 0.5 1.0 10 23 [year]

R&D for future Scintillating bolometer for low BG 48 Ca enrichment for large target volume 27

Bolometer development Now 208 Tl is dominant BG and 2nbb is almost negligible in the current sensitivity. However, 2nbb will become main enemy for future after 48 Ca enrichment. Better energy resolution is necessary. Scintillator Bolometer New BG appear in bolometer. 48 Ca Qbb: 4268 kev / 238 U Qa : 4270 kev Need particle ID Scintillating bolometer The technique of scintillating bolometer was already established. CRESST-II (CaWO4), Lucifer, AMoRE Simultaneous measurement both heat and scintillation enables to identify the particle types (α/β particle ID).

Bolometer development Dilution refrigerator We will use the dilution refrigerator which was developed for the dark matter search with LiF by the Univ. of Tokyo, and was customized to low BG measurement. Cooling power is 2μW @ 20mK Target 2cm cube of CaF2 crystal (25 g) in the initial stage. Temperature rise at Q-value is 1.43 10-1 K at 10 mk. Neutron Transmutation Doped Germanium(NTD-Ge) thermistors borrowed from the Univ. of Tokyo. Schedule 2016 Achieve low temperature (~a few K) Done!! Achieve ultra low temperature (~10mK) Detect heat signal 2017 Please see Tetsuno s poster Add a light detector to bolometer and achieve the simultaneous detection of heat and light signals Increase crystal size and number

48 Ca enrichment Natural abundance of 48 Ca is 0.187%. Commercial 48 Ca too expensive (M$/10g but kg-ton) Developing enrich technique of 48 Ca is crucial for large volume DBD search. Challenges in CANDLES: Crown ether resin + chromatography (Osaka, TIT ) 1.3 times and cost down Journal of Chromatography A Volume 1415, 9 October 2015, Pages 67 Crown ether + micro reactor (Osaka sangyo) Laser separation (Fukui) Good separation but smaller productivity Multi-channel counter current electrophoresis (Osaka)

R(MCCCE) Multi-channel counter current electrophoresis Electric field 48 Ca 40 Ca Counter current BN plate 10 mm thick 0.8mmΦ, every 4 mm Separation using difference of migration speed between 40 Ca / 48 Ca. Principle was demonstrated. Further study on parameter optimization for,,, R( MCCCE) High enrichment Large amount 43Ca / 48Ca( MCCCE) 43Ca / 48Ca( natural) 4 Enrichment (43/40): 3.08 (48/40): 6 3 2 1 0 145 155 165 175 185 V (Applied voltage)

Summary CANDLES is a project to search for double beta decay of 48 Ca using 300kg CaF2 scintillator, running in Kamioka underground lab.. Using 48 Ca has a great chance to achieve Background Free Measurement, one of the key to perform sensitive 0νββ search. Additional shield consisting of Pb/B was installed in 2015-2016 and data taking restarted from this May. The (n,g) background was reduced by almost two order of magnitude. Sensitivity of 0nbb is 0.5-1.0 10 23 [year] We are now trying to improve analysis method for achieving better sensitivity. Future R&D is also ongoing. 32

New collaborative institute and Postdoc are now wanted!! Thank you very much!! 33 33

Backup slide 34 34

35

m ββ (mev) 2nbb Double beta decay 0nbb Constraint of n mass from oscillation experiments KKDC Claim Standard model Already observed in some nuclei T1/2: 10 18 ~ 10 20 yr Beyond the SM Proof of Majorana neutrino T1/2: > 10 25 yr Inverted hierarchy Normal hierarchy 0nbb half-life: If Majorana neutrino Light neutrino mass (See-Saw mechanism) Matter dominated universe (Leptogenesis) Lightest neutrino m ν (mev) 36

2016 2015 2014 Recent detector upgrade Magnetic cancellation coil installation Detector cooling system installation For better energy resolution!! DBD14 @Hawaii Data taking Gamma and neutron shield construction For lowering background level! Preparation for next run Data taking DBD16 @Osaka 37

Magnetic cancellation coil Winded coil surrounding the water tank and apply ~1.5A current to cancel geomagnetic field. Better p.e. collection efficiency of PMT dynode is expected. Vertical coil Horizontal coil Reconstructed position Side view Top view 1pe distribution (13 PMT) 1. Light yield increased (later) 2. Position distortion improved 3. 1pe distribution improved Before After ADC count 38

Cooling system Cooling system was installed and tested in middle of 2014. Data was taken with low temperature in the end of 2014. CANDLES cooling system (Laboratory Room is cooled down by chiller) Light yield of CaF2 increase 2% by lowering 1 degree. Cooled air Detector direction Our measurement Literature value (w/o WLS) CaF2 temperature [ ] Room temp. 2, Water temp. 4.3 Test data was successfully collected with very good stability (±0.1 ) during ~1 month. 39

Light yield increase 40 K No improvement After Coil After cooling 208 Tl Total ADC count Light yield has been increased by the detector upgrades. Relative light yield Resolution Before 1 σ = 4.8% Coil 1.23 σ = 4.2% Cool 1.58 σ = 3.6% Obtained from 88 Y source calibration After improvements, ~1000 [p.e./mev] is achieved 40