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Measurement of surface radioactivity by Alpha/Beta detection

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Presentation on theme: "Measurement of surface radioactivity by Alpha/Beta detection"— Presentation transcript:

1 Measurement of surface radioactivity by Alpha/Beta detection
Pia Loaiza LRT2017, Seoul May 2017

2 Surface screening: motivations in DM search
Bolometers in dark matter search, Edelweiss, CDMS : 210Pb on detector surface or directly in contact with the detectors produce events leaking in the nuclear recoil band To achieve required sensitivities, detectors must have ACTIVE REJECTION And screening to minimize surface radioactivity Surface events

3 Alpha background in 2b0n search
g/b-region a -region Qbb 130Te = 2530 keV Degraded Alphas main background in CUORICINO/CUORE-0 234U 208Tl 210Po 190Pt 226Ra 230Th 238U 222Rn CUORICINO CUORE-0 factor ~7 reduction in the alpha continuum region thanks to surface contamination reduction 218Po from CUORICINO/ CUORE-0 cryostat from surface contaminations

4 Background in SuperNEMO 2b0n search
Thin 2b0n source in tracker surrounded by calorimeter, 2b0n isotope: 82Se A 2b0n event is recognized as 2 electrons from the source foil with ∑E = 3 MeV and t1 t2 One of the most dangerous background : 208Tl and 214Bi from source foils and Radon a’s used to asses contaminations: ~ 200 mm Number of 212Po a’s going out of the source foil 208Tl b 208Tl b g Eg = 2.7 MeV 208Pb Qb=4.9 MeV In this case, if g is not giving a hit in the calorimeter it mimics a 2b0n event

5 Alpha/Beta screening This talk will be restricted to large surface detectors Not inclusive of the many efforts and detectors existing My sincere apologies if your favourite detector is not mentioned Alpha screening: - XIA’s alpha counter UltraLo-1800 Surface alpha detector using m-TPC Alphas and Betas - BetaCage Alpha/Beta coincidence: - BiPo3

6 XIA’s Alpha counter – UltraLo-1800
Talk « Improving the limits of detection of low background alpha emission measurements » by Brendan McNally  Images courtesy of e- Talk: ‘Precise measurement of Pb210 and Po210 contamination in bulk copper’ by Kazuyoshi Kobayashi Poster: ‘An Ar-gas ionization chamber for alpha particle detection at the Yangyang underground laboratory’ by Chang Hyon Ha Ar+ a a Drift chamber filled with Ar Electrodes at +1kV

7 XIA’s Alpha counter – UltraLo-1800
Alphas : ≥ 2 MeV Discrimination of alphas from walls and ceiling Alphas from sample : no guard signal amplitude Total sample surface: 1800 or 707 cm2 Background sea-level, unshielded ~ 10-3 a/cm2/hr underground, shielded ~ 10-4 a/cm2/hr Sensitivity < 0.5 mBq/m2 for 210Po Images courtesy of 7 7

8 Surface alpha detector using m-TPC
Talk: « Development of a low alpha emitting m-PIC for NEWAGE direction-sensitive dark matter search » by Takashi Hashimoto Position sensitive Located at Kamioka mine Background (outside sample region): 0.119 ± events/cm2/h Total sample surface: (10 x 10) cm2

9 The BetaCage Poster: « The BetaCage: An Ultra-sensitive screener for surface contamination » by Eric Miller Drift chamber with Multi-wire proportional counter Sample in the gas (90 % Ne, 10% methane) A ‘trigger’ MWPC creates the trigger region Drift region contains all 200 keV e- and alphas A ‘bulk’ MWPC collects the charges Total sample surface: 0.45 m2 = 4500 cm2

10 The BiPo-3 detector Measurement of 212Bi(208Tl) and 214Bi
Initially developed to measure SuperNEMO 2b0n source foils Detection principle: b-a delayed coincidence detection

11 Detector principle The foil of interest is installed between two thin low radioactive organic scintillators Source Foil Scintillator Light Guide PMT

12 Assembling of BiPo sub-OMs in the structure
The set-up Optical sub-module Assembling of BiPo sub-OMs in the structure Optical sub-module: Polyestyrene scintillators coupled to 5’’ PMTs through a PMMA guide 20 pairs of optical sub-modules assembled in one Module BiPo3= 2 modules Total detector surface= 3.6 m2 = cm2 Installed in Canfranc Underground Laboratory

13 Time window for event selection
212BiPo 214BiPo Eprompt= 576 keV Eprompt= keV Dt= 40 ms Edelay= keV Edelay= 967 keV Dt=390 ns The delay time between the prompt and the delayed signal is 20 ns < Dt < 1500 ns (212Po T1/2 = 300 ns) The delay time between the prompt and the delayed signal is 10 ms < Dt < 1000 ms (214Po T1/2 = 164 ms)

14 Backgrounds Scintillator surface Scintillator bulk Random coincidences
contamination Radon in the sensitive volume Random coincidences Compton e- from external g’s Scintillator bulk contamination rejected

15 212BiPo background measurement
Three dedicated background measurements (200.4 days of measurement) One measurement: 75 days x 3.42 m2 12 212BiPo candidates All events from surface background: a’s deposit all their energy inside the scintillator → peak at about 1000 keV source a energy scint For events with Ea < 700 keV (bulk activity) background free measurement Surface background: A(208Tl) = 0.9 ± 0.2 mBq/m2 (= events/cm2 hr)

16 214BiPo background measurement
Two dedicated background measurements (111.9 days of measurement) One measurement: 75 days x 3.42 m2 30 214BiPo candidates Events from surface background: a’s depositing all its energy inside the scintillator → peak at about 800 keV Random coincidences at low energies→ dominant background Surface background: A(214Bi) = 1.0 ± 0.4 mBq/m2 a energy (= events/cm2 hr) Random coincidences average: = 0.12 cts/day/m2 (= counts/cm2 hr) 16

17 Sample measurements SuperNEMO foils 82Se powder mixture:
A(208Tl) mBq/kg 90% CL A(214Bi) mBq/kg 90% CL A(214Bi) mBq/m2 90% CL Mylar < 49 <195 < 5 Irradiated Mylar 100 ± 53 < 690 3.7 ± PVA < 12 < 505 31 ± 8 6.8 3.5 212BiPo SuperNEMO foils Se mixture Mylar scint. surface contamination 82Se powder mixture: A(208Tl) = (21 ± 11) mBq/kg, 90% CL a energy

18 Sensitivity Sensitivity to Se powder mixture:
A(208Tl) < 2 mBq/kg , 90% CL in 6 months A(214Bi) < 140 mBq/kg , 90% CL in 6 months Using total BiPo3 area = 3.6 m2 Mylar ideally radiopure Surface background and random coincidences from dedicated bkg measurements

19 Summary A number of dark matter and neutrino experiments are sensitive to surface contaminants Surface screening is needed to control and reduce surface contaminants Alpha detection used to asses surface and bulk radiopurity levels Current background in alpha detectors ~ 10-4 a/cm2/hr. Sensitivities < 0.5 mBq/m2 for 210Po Beta/Alpha coincidence used to asses 212Bi/214Bi radioactivity levels. Sensitivity reached A(208Tl) < 10 mBq/kg


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