Status of ULE-HPGe Experiment for WIMP Search
Li Xin (Tsinghua University)KIMS collaboration
Feb. 7th, 2006
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
Current System Setup
HPGe: -500VCsI(Tl): -1300V
H.V. (CEAN 1527) Amp. (CANBERRA 2026)
Shaping time: 6usGain: ×20
ULE - HPGe detector FADC & VME crate
DAQ System
► DAQ device:DAQ device:
4-channel FADC4-channel FADC
SR=64MHz, 12bitSR=64MHz, 12bit
64 us window64 us window
USB2.0 interfaceUSB2.0 interface
Typical signals:
HPGe High gain(0~9keV)
HPGe Low gain(0~100keV)
CsI(Tl) channel(current signal)
X-ray Generator
(From http://www.amptek.com )
LiTaO3
(From http://www.amptek.com )
X-ray Generator
Structure of the HPGe Detector
The carbon window can stop the particle with the energy less than about 1.5keV.
HPGe Calibration – high gain channel
Peaks: Ta, Ca, Cs, Ti, Mn, Fe, Cu X-ray
After gain correction and pedestal shift correction
2
113.13
12.9617
offset eV
ndf
HPGe Calibration – low gain channel
Peaks:
Np (L X-ray), Ag (K X-ray), Am (alpha decay gamma)
2
0.0694
20.67
offset keV
ndf
CsI Calibration
2
2.487
10.4607
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
PSD Parameters for CsI noise reduction
T-bar of CsI (Tl) Detail
Red: background files (Oct. 4th ~ Oct. 18th)Blue: calibration file (Co-57)Green: neutron file Threshold for CsI: ~10keV
Neutron Recoil Data for HPGe
Energy spectrum
Source: Cf-252 (outside Pb shielding)Time: Nov. 2nd, 14:00~19:00
Time coincidence relation (1D)
Detail
Time coincidence relation (2D)
Threshold for HPGeThreshold Pulse shape (270 ~ 290 eV)
Hardware threshold: ~ 150 eVElectronic noise level: τ~ 13 eV
Threshold for HPGe: 300eV
Energy spectrum of background pedestal shape fitting
50ln(1/ ) 13 ln(10 ) 150( )E h eV
exp( )E
h
Background Data Analysis
datedate ThresholThreshold (keV)d (keV)
Total Total countscounts
Vetoed Vetoed countscounts
Background Background level (cpd)level (cpd)
Veto Veto efficiencyefficiency
Oct. 4th ~ Oct. 4th ~ 18th18th
0.30.3 802802 487487 44.182644.1826 60.7232%60.7232%
Oct. 4th ~ Oct. 4th ~ 18th18th
11 772772 479479 41.096941.0969 62.0466%62.0466%
High gain channel Low gain channel
Background Data Analysis
datedate Threshold Threshold (keV)(keV)
Total Total countscounts
Vetoed Vetoed countscounts
Background Background level (cpd)level (cpd)
Veto Veto efficiencyefficiency
Oct. 18th ~ Oct. 18th ~ 31th31th
0.30.3 611611 368368 44.182644.1826 60.7232%60.7232%
Oct. 18th ~ Oct. 18th ~ 31th31th
11 587587 361361 45.033445.0334 61.4991%61.4991%
High gain channel Low gain channel
Background after Neutron Run
datedate Threshold Threshold (keV)(keV)
Total Total countscounts
Vetoed Vetoed countscounts
Background Background level (cpd)level (cpd)
Veto Veto efficiencyefficiency
Nov. 3rd ~ Nov. 3rd ~ 11th11th
0.30.3 504504 294294 47.151847.1518 58.3333%58.3333%
Nov. 3th ~ Nov. 3th ~ 11th11th
11 465465 286286 40.191340.1913 61.5054%61.5054%
High gain channel Low gain channel
10keV peak
Background with Strong γSource Outside
datedate Threshold Threshold (keV)(keV)
Total Total countscounts
Vetoed Vetoed countscounts
Background Background level (cpd)level (cpd)
Veto Veto efficiencyefficiency
Nov. 11th ~ Nov. 11th ~ 25th25th
0.30.3 830830 516516 44.440244.4402 62.1687%62.1687%
Nov. 11th ~ Nov. 11th ~ 25th25th
11 791791 508508 39.744139.7441 64.2225%64.2225%
High gain channel Low gain channel
Source: U-238, Th-232, Eu-152 (Outside Pb shielding)
Summary
1. The ULE-HPGe system has been set up and
the data taking has been run for several
months.
2. Background level: abut 40
count/kg/day/keV (not from external
gamma)
3. Veto efficiency: about 60%
4. Software threshold: about 300 eV5. Question:
(1). Is the background level acceptable?
(2). Is the energy threshold correct?
In the future…
1. Parameter selection for electronic system
2. Pulse shape study in low-energy region, and more
accurate calibration
3. Monte-Carlo simulation for external and internal
neutron, and build neutron shielding if necessary
4. Internal background study for HPGe and CsI(Tl)