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Performance study of GAGG: Ce crystal Zhigang Wang IHEP, CAS 2019.11.26 1 CHEF 2019- Calorimetry for the High Energy Frontier 2019, 25-29 November, Fukuoka

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Page 1: Performance study of GAGG: Ce crystalCHEF 2019- Calorimetry for the High Energy Frontier 2019, 25-29 November, Fukuoka 9 Light output of GAGG:Ce scintillator is linear in the range

Performance study of GAGG: Ce crystal

Zhigang Wang

IHEP, CAS

2019.11.26

1 CHEF 2019- Calorimetry for the High Energy Frontier 2019, 25-29 November, Fukuoka

Page 2: Performance study of GAGG: Ce crystalCHEF 2019- Calorimetry for the High Energy Frontier 2019, 25-29 November, Fukuoka 9 Light output of GAGG:Ce scintillator is linear in the range

Outline

1, Introduction of GAGG: Ce crystal

2, Scintillation properties of GAGG: Ce

(1) Emission spectra

(2) Decay times

(3) Relative light yield

(4) Linearity of light output

(5) Energy resolution

3, Thermal neutron detection of GAGG: Ce

4, Summary

2 CHEF 2019- Calorimetry for the High Energy Frontier 2019, 25-29 November, Fukuoka

Page 3: Performance study of GAGG: Ce crystalCHEF 2019- Calorimetry for the High Energy Frontier 2019, 25-29 November, Fukuoka 9 Light output of GAGG:Ce scintillator is linear in the range

1, Introduction of GAGG: Ce crystal

GAGG:Ce crystal is a promising scintillation material for high energy physics calorimeter.

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Recently developed cerium-doped GAGG(GAGG: Ce) is a novel scintillator characterized by a high density(6.63g/cm3), high light yield(56,000 photon/MeV), fast scintillation decay time(~100 ns), very good radiation hardness, non-hygroscopicity and extremely low internal background.

Ingot GAGG:Ce

CHEF 2019- Calorimetry for the High Energy Frontier 2019, 25-29 November, Fukuoka

GAGG:Ce crystal

Page 4: Performance study of GAGG: Ce crystalCHEF 2019- Calorimetry for the High Energy Frontier 2019, 25-29 November, Fukuoka 9 Light output of GAGG:Ce scintillator is linear in the range

2, Scintillation properties of GAGG: Ce

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S1 S2 S3 S4

S1 (5mm cube) and S2(5mm cube) samples are single crystal GAGG: Ce, produced in China and Russia, fabricated by the conventional Czochralski method. S3 (5mm cube) and S4 (5mm cube) samples are ceramic GAGG: Ce, produced in China and Japan, fabricated by the vacuum sintering method.

GAGG: Ce samples

CHEF 2019- Calorimetry for the High Energy Frontier 2019, 25-29 November, Fukuoka

Page 5: Performance study of GAGG: Ce crystalCHEF 2019- Calorimetry for the High Energy Frontier 2019, 25-29 November, Fukuoka 9 Light output of GAGG:Ce scintillator is linear in the range

Photodetectors

CHEF 2019- Calorimetry for the High Energy Frontier 2019, 25-29 November, Fukuoka 5

PMT-XP2020 Hamamatsu MPPC Area: 6mm×6mm, Pitch:10,25,50,75um

×

NDL SiPM Area: 3mm×3mm, Pitch:10um

Different types of photodetectors are coupled to GAGG:Ce scintillators to do performance study.

Page 6: Performance study of GAGG: Ce crystalCHEF 2019- Calorimetry for the High Energy Frontier 2019, 25-29 November, Fukuoka 9 Light output of GAGG:Ce scintillator is linear in the range

Emission spectra

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S3

S1 S2

S4

? ?

Primary emission spectra of these 4 samples appeared from 500 to 700 nm, but different with each other. Weak emission peaks clearly appeared at around 380 nm in crystal GAGG:Ce.

CHEF 2019- Calorimetry for the High Energy Frontier 2019, 25-29 November, Fukuoka

Page 7: Performance study of GAGG: Ce crystalCHEF 2019- Calorimetry for the High Energy Frontier 2019, 25-29 November, Fukuoka 9 Light output of GAGG:Ce scintillator is linear in the range

Decay times

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S1 crsytal GAGG:Ce t1= 50 ns , t2= 225 ns Weak peak: t1=14 ns , t2=88 ns

S2 crsytal GAGG:Ce t1= 32ns , t2= 115 ns Weak peak: t1=9 ns , t2=90 ns

S3 ceramic GAGG:Ce t1= 113 ns

S4 ceramic GAGG:Ce t1= 51 ns t2= 245 ns

CHEF 2019- Calorimetry for the High Energy Frontier 2019, 25-29 November, Fukuoka

A filter is used to test the decay times of the weak peaks in sample 1 and 2.

Page 8: Performance study of GAGG: Ce crystalCHEF 2019- Calorimetry for the High Energy Frontier 2019, 25-29 November, Fukuoka 9 Light output of GAGG:Ce scintillator is linear in the range

Relative light yield

CHEF 2019- Calorimetry for the High Energy Frontier 2019, 25-29 November, Fukuoka 8

In general, ceramic GAGG:Ce have higher light yield than crystal GAGG:Ce

S1:S2:S3:S4 = 1:0.68:1.72:1.55

Pulse height spectra measured with 4 samples coupled to Hamamatsu MPPC(6mm*6mm,25 um ) obtained by irradiation with 662 keV gamma

Page 9: Performance study of GAGG: Ce crystalCHEF 2019- Calorimetry for the High Energy Frontier 2019, 25-29 November, Fukuoka 9 Light output of GAGG:Ce scintillator is linear in the range

Linearity of GAGG:Ce light output

CHEF 2019- Calorimetry for the High Energy Frontier 2019, 25-29 November, Fukuoka 9

Light output of GAGG:Ce scintillator is linear in the range of 31 keV-1.27 MeV

Linearity of GAGG:Ce scintillator(S1/S3) coupled with PMT

Source Energy

(keV)

Na-22 511

Na-22 1274

Co-57 122

Co-60 1332

Ba-133 31

Ba-133 81

Ba-133 356

Cs-137 662

Radioactive source

Page 10: Performance study of GAGG: Ce crystalCHEF 2019- Calorimetry for the High Energy Frontier 2019, 25-29 November, Fukuoka 9 Light output of GAGG:Ce scintillator is linear in the range

Response curve of GAGG:Ce coupled with MPPC/SiPM

CHEF 2019- Calorimetry for the High Energy Frontier 2019, 25-29 November, Fukuoka 10

Response curve decided by the dynamic range of the MPPC/SiPM

Response curve of GAGG:Ce scintillator coupled with Hamamatsu MPPCs

Response curve of GAGG:Ce scintillator coupled with NDL SiPM

10 um 25 um 50 um 75 um

Page 11: Performance study of GAGG: Ce crystalCHEF 2019- Calorimetry for the High Energy Frontier 2019, 25-29 November, Fukuoka 9 Light output of GAGG:Ce scintillator is linear in the range

Energy resolution

CHEF 2019- Calorimetry for the High Energy Frontier 2019, 25-29 November, Fukuoka 11

Cs-137 source, S3 GAGG:Ce 5×5×5 mm3 + Hamamatsu MPPC 6×6mm2, 75 um pitch

FWHM = 3.5% @ 662 keV

Pulse height spectrum measured with GAGG coupled to Hamamatsu MPPC:75um pitch

Energy resolution of GAGG:Ce scintillator measured with two different MPPC:25/75 um pitch

75 um pitch 25 um pitch

Page 12: Performance study of GAGG: Ce crystalCHEF 2019- Calorimetry for the High Energy Frontier 2019, 25-29 November, Fukuoka 9 Light output of GAGG:Ce scintillator is linear in the range

3,Neutron detection with GAGG:Ce

CHEF 2019- Calorimetry for the High Energy Frontier 2019, 25-29 November, Fukuoka 12

The detection of photopeaks in a thin slice due to conversion electrons and low-energy X-rays make GAGG:Ce scintillator possible to discriminate the high energy gamma background efficiently. The low-energy gamma background incident on the crystal from outside can be easily stopped by using a thin lead sheet wrapped around the scintillator.

157Gd + n -> 158Gd + gamma + X ray + conversion electron 155Gd + n -> 156Gd + gamma + X ray + conversion electron

Page 13: Performance study of GAGG: Ce crystalCHEF 2019- Calorimetry for the High Energy Frontier 2019, 25-29 November, Fukuoka 9 Light output of GAGG:Ce scintillator is linear in the range

Neutron detector

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Hamamatsu MPPC Area: 6×6 mm2, Pitch:75 um

GAGG:Ce slice 5 mm×5 mm, thickness of 1.0 and 0.5 mm

Neutron detector Am-Be neutron source

Page 14: Performance study of GAGG: Ce crystalCHEF 2019- Calorimetry for the High Energy Frontier 2019, 25-29 November, Fukuoka 9 Light output of GAGG:Ce scintillator is linear in the range

Experiment setup of neutron test

CHEF 2019- Calorimetry for the High Energy Frontier 2019, 25-29 November, Fukuoka 14

A 3-mm cadmium sheet used to shield the detector for recording the background data.

HDPE with 5 cm thickness is used as moderator. The detector is shielded using a 2 mm lead (Pb) and 2 mm stainless steel (SS) sheet.

Digitizer DT5751

Page 15: Performance study of GAGG: Ce crystalCHEF 2019- Calorimetry for the High Energy Frontier 2019, 25-29 November, Fukuoka 9 Light output of GAGG:Ce scintillator is linear in the range

Energy calibration

CHEF 2019- Calorimetry for the High Energy Frontier 2019, 25-29 November, Fukuoka 15

Pulse height spectrum of 1mm thick GAGG:Ce

calibrated by Barium(Ba-133) 31 and 83 keV gamma

31 keV

83 keV

Page 16: Performance study of GAGG: Ce crystalCHEF 2019- Calorimetry for the High Energy Frontier 2019, 25-29 November, Fukuoka 9 Light output of GAGG:Ce scintillator is linear in the range

Thermal neutron detection

CHEF 2019- Calorimetry for the High Energy Frontier 2019, 25-29 November, Fukuoka 16

Thermal neutron Back ground with Cd

The photopeaks around 35 and 83 keV well discriminated from the background could be successfully observed by this neutron detector, provide a clear signature for thermal neutron detection.

34.9±0.8 keV

83.2 ± 11.8 keV

Neutron detection results of 1mm GAGG:Ce

The signal-to-background ratio of 83 keV is 5.6

Page 17: Performance study of GAGG: Ce crystalCHEF 2019- Calorimetry for the High Energy Frontier 2019, 25-29 November, Fukuoka 9 Light output of GAGG:Ce scintillator is linear in the range

Light output of GAGG:Ce slice

CHEF 2019- Calorimetry for the High Energy Frontier 2019, 25-29 November, Fukuoka 17

Light output of GAGG:Ce slice with different thickness,

5.0 mm: 1.0 mm: 0.5 mm: 0.2mm=1:1.09:1.26:1.34

0.2 mm 0.5 mm 1.0 mm 5.0 mm

Page 18: Performance study of GAGG: Ce crystalCHEF 2019- Calorimetry for the High Energy Frontier 2019, 25-29 November, Fukuoka 9 Light output of GAGG:Ce scintillator is linear in the range

Summary

1, Scintillation properties of GAGG:Ce scintillator as a calorimeter material studied detailed.

2, Slice of GAGG:Ce can clearly separate thermal neutron from gamma background.

CHEF 2019- Calorimetry for the High Energy Frontier 2019, 25-29 November, Fukuoka

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