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Status of Ultra-low Energy HPGe Detector for low-mass WIMP search

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Status of Ultra-low Energy HPGe Detector for low-mass WIMP search. Li Xin (Tsinghua University) KIMS collaboration. Oct.22nd, 2005. Index. Motivation Previous status Current system setup Calibration Background data analysis Future plan. 5g Ge. 1cpd. Motivation. - PowerPoint PPT Presentation
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Status of Ultra-low Energy HPGe Detector for low-mass WIMP search Li Xin (Tsinghua University) KIMS collaboration Oct.22nd, 2005
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Page 1: Status of Ultra-low Energy HPGe Detector for low-mass WIMP search

Status of Ultra-low Energy HPGe Detector

for low-mass WIMP search

Li Xin (Tsinghua University)

KIMS collaboration

Oct.22nd, 2005

Page 2: Status of Ultra-low Energy HPGe Detector for low-mass WIMP search

Index

1. Motivation

2. Previous status

3. Current system setup

4. Calibration

5. Background data analysis

6. Future plan

Page 3: Status of Ultra-low Energy HPGe Detector for low-mass WIMP search

Motivation

5g Ge

1cpd

Low mass Dark Matter candidate search - Low energy threshold necessary - Use 5g of prototype Ge detector ( plan to upgrade up to 1 kg )

Expected threshold: ~100eV

Page 4: Status of Ultra-low Energy HPGe Detector for low-mass WIMP search

Depth Minimum 700 m

Temperature 20 ~ 25 oC

Humidity 35 ~ 60 %

Rock contents 238U less than 0.5 ppm 232Th 5.6 +/- 2.6 ppm

K2O 4.1 %

Muon flux 4.4 x 10-7 /cm2/s

Neutron flux 8 x 10-7 /cm2/s

222Rn in air 2 ~ 4 pCi/liter

Y2L Underground Lab

Page 5: Status of Ultra-low Energy HPGe Detector for low-mass WIMP search

Previous DAQ Setup by He Dao

• DAQ:

4 channels

SR=25MHz, 8bit

100 us window

GPIB interface

Three typical signal:

HPGe High gain(0~7keV)

HPGe Low gain(0~50keV)

CsI(Tl) channel(charge signal)

Page 6: Status of Ultra-low Energy HPGe Detector for low-mass WIMP search

HPGe & CsI Calibration by He Dao

HPGe calibration

Source: Fe-55 (5.9, 6.5 keV)Target: Ti (4.5, 4.9 keV)

CsI calibration

Source :Na-22 (0.511 & 1.275MeV)Mn-54 (0.835MeV)

Page 7: Status of Ultra-low Energy HPGe Detector for low-mass WIMP search

HPGe detector threshold

Energy threshold by He Dao

CsI (Tl) detector threshold

HPGe Threshold: 265eV CsI Threshold: 50keV

Page 8: Status of Ultra-low Energy HPGe Detector for low-mass WIMP search

Ge signal beyond threshold vetoed by CsI signal:

Originally: 416+764 = 1180 events

After veto: 357+456 = 813 events (270 events in 10.29keV peak)

Background level:

813/(1909350/3600/24)/0.005/55 = 133 counts/(day*Kg*keV)

Efficiency = 1 - 813/1180 = 31.1%

Background level and veto efficiency by He Dao

High gain channel Low gain channel

(22.1 days data)

Page 9: Status of Ultra-low Energy HPGe Detector for low-mass WIMP search

PSD for HPGe noise reduction

i ii

ii

Att

A

Time region

400 ~ 2000 (40ns/bin)

(the best time range for discrimination)Total window: 80us, 2000bin

Blue: calibration data Red: background data

Page 10: Status of Ultra-low Energy HPGe Detector for low-mass WIMP search

Current system setup

• ULE-Ge detector:– H.V.: -500V– Gain: 20x– Shaping time: 6 us– Range: 0~100keV

• CsI detector:– H.V.: -1300V– Gain: 100x

• N2 flow: 1 liter/min

Page 11: Status of Ultra-low Energy HPGe Detector for low-mass WIMP search

New DAQ system

• DAQ device:

4-channel FADC

SR=64MHz, 12bit

64 us window

USB2.0 interface

Typical signals:

HPGe High gain(0~9keV)

HPGe Low gain(0~100keV)

CsI(Tl) channel(current signal)

Page 12: Status of Ultra-low Energy HPGe Detector for low-mass WIMP search

HPGe high gain channel calibration

Gain shift:

Date: Sep.6th~13th

Source: Fe-55 5.9keV peak

0 4.20955 00, 0 4.40426 03

, 1 1.98459 04

2 2.23065 03, 2 2

1 1.9

.203

8411 0

8

2

5 01

p e p e

p e

p e p e

p e

0 1 ( ) 2p p time hour

height

e p

Equation:

50hours For stabilization: 10 days

Amplitude of gain shift ~ 2.5% (7 days)

Page 13: Status of Ultra-low Energy HPGe Detector for low-mass WIMP search

HPGe high gain channel calibration

The carbon window will stop the particles whose energy is lower than about 2keV.

Structure of HPGe detector

Page 14: Status of Ultra-low Energy HPGe Detector for low-mass WIMP search

HPGe high gain channel calibration

Source: X-ray generator (AMPTEK INC.)

Target: Ti (4.5, 4.9 keV) Target: CsI (4.3, 4.6, 5.3 keV)

Polyelectric crystal (LiTaO3) is used to

generate electrons that produce X-ray

in the target material (Cu).

Page 15: Status of Ultra-low Energy HPGe Detector for low-mass WIMP search

HPGe high gain channel calibration

Source: X-ray generator (internal peaks)

peak Energy (keV) σ

(keV)

Expected element

Expected energy (keV)

ΔE/ σ

A 1.680±0.0139 0.074 Ta (Ma) 1.702 0.2973

B 2.7519± 0.0036 0.0586 Ru (L) 2.71785 0.5815

*red: we cannot explain the source of the element polyelectric crystal (LiTaO3)

Page 16: Status of Ultra-low Energy HPGe Detector for low-mass WIMP search

HPGe high gain channel calibration

Peaks: Ta, Ca, Cs, Ti, Mn, Fe, Cu X-ray

After gain correction

2

117.7

12.23

offset eV

ndf

Page 17: Status of Ultra-low Energy HPGe Detector for low-mass WIMP search

HPGe low gain channel calibration

Source: Am-241 Source: Cd-109

Np L-series X-ray:

13.9257, 16.8400, 17.7502, 20.7848 (keV)

Am alpha decay: 59.5412 (keV)

Ag K-series X-ray:

21.9903, 22.16292, 24.9424, 25.463 (keV)

Page 18: Status of Ultra-low Energy HPGe Detector for low-mass WIMP search

HPGe low gain channel calibration

Peaks:

Np (L X-ray), Ag (K X-ray), Am (alpha decay gamma)

2

0.0694

20.67

offset keV

ndf

Page 19: Status of Ultra-low Energy HPGe Detector for low-mass WIMP search

CsI (Tl) channel calibration

2

1.397

1.99972

offset keV

ndf

Gamma energy:

Cd-109 (Ag X-ray): 22.577 keV

Am-241: 59.5412 keV

U-238 (Th-234): 92.6 keV

Co-57: 123.66 keV

Page 20: Status of Ultra-low Energy HPGe Detector for low-mass WIMP search

Background data analysis

Only 5.33 days’ dataHPGe energy spectrum

High gain channel Low gain channel

( 0 ~ 9 keV ) ( 0 ~ 100 keV )

Page 21: Status of Ultra-low Energy HPGe Detector for low-mass WIMP search

Background data analysis

HPGe threshold

Threshold: 260eV

Page 22: Status of Ultra-low Energy HPGe Detector for low-mass WIMP search

CsI (Tl) PSD for noise reduction

Panorama Detail

( )i i

i

ii

I tt vs energy keV

I

Blue: calibration file (U-238) Red: background file

Page 23: Status of Ultra-low Energy HPGe Detector for low-mass WIMP search

Background data analysis

Background level and veto efficiency

Veto efficiency: 191/436=43.81%

High gain channel Low gain channel

Counting rate: (436-191)/100/0.005/5.326≈92cpd

Page 24: Status of Ultra-low Energy HPGe Detector for low-mass WIMP search

1. PSD of HPGe high gain channel for noise reduction

— to reduce the threshold

2. Time coincidence relation between HPGe and CsI

— improve the discrimination for Compton veto events

3. Simulation and shielding for neutron

— to reduce the background level

Future plan


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