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IBM Research
10/26/2011 © 2011 IBM Corporation
On the Calibration of Alpha Sciences Proportional Counters
Michael Gordon ([email protected])
Ken Rodbell
IBM Research1101 Kitchawan RoadYorktown Heights, NY 10598
IBM Research & IBM Systems and Technology Group
© 2010 IBM Corporation2 10/26/2011
Outline
How is the discriminator set on Alpha Sciences counter and what is thealpha-particle energy associated with the setting? What is the impact ofcutting out the low energy alphas from a sample?
– Introduction
– Background
– Overview of the Alpha Sciences proportional counters
– Our low-energy alpha-particle source
– Results
– Conclusion
IBM Research & IBM Systems and Technology Group
© 2010 IBM Corporation3 10/26/2011
Introduction
We review a technique for determining the alpha-particle energy associated with a discriminator setting.
We have a low energy “thick” alpha-particle source that was developed for this work.
The alpha particles from this source stop in the gas within the active volume of the detector (important for association between pulse-height analysis and alpha-particle energy).
We compared the count rate of the source vs discriminator setting in the proportional counter, and the count rate of the same source with a silicon surface barrier detector to obtain an energy scale.
IBM Research & IBM Systems and Technology Group
© 2010 IBM Corporation4 10/26/2011
Background
Many labs have Alpha Sciences proportional counters– Material labs– Semiconductor labs
Recently, several labs participated in a “round-robin” study of both low and ultra-low emissivity samples, “Multicenter comparison of alpha particle measurements and methods typical of semiconductor processing”* – Very few constraints were placed on the measurement
• No sample preparation or measurement protocol• Samples were in many pieces that could be tiled to account for different sizes of the
tray/active area of the counter– There was a ~ 2X difference between the largest and smallest sample
emissivity measured– It was proposed that this difference could be due to the discriminator settings
on the individual detectors• Most people “assume” that the discriminators are set to 1 MeV
* http://ieeexplore.ieee.org/stamp/stamp.jsp?tp=&arnumber=5784521
IBM Research & IBM Systems and Technology Group
© 2010 IBM Corporation5 10/26/2011
Cutaway section of an old Alpha Sciences counter
cathode plane
anode wires
6 mm
6 mmcathode
sample tray
anode
Cross section of counter
IBM Research & IBM Systems and Technology Group
© 2010 IBM Corporation6 10/26/2011
0
0.05
0.1
0.15
0.2
0.25
0 1 2 3 4 5 6 7 8 9 10
Energy (MeV)
dE/d
X (M
eV/m
m)
0
24
48
72
96
120
Ran
ge (m
m)
SRIM simulations of alpha-particles in Ar gas
36.2 mm1.43”
104.8 mm4.25”
The counter gas used is Ar/CH4
IBM Research & IBM Systems and Technology Group
© 2010 IBM Corporation7 10/26/2011
SRIM simulations of alpha-particles in Ar gas
0
0.05
0.1
0.15
0.2
0.25
0 0.25 0.5 0.75 1 1.25 1.5 1.75 2
Energy (MeV)
dE/d
X (M
eV/m
m)
0
4
8
12
16
20
Ran
ge (m
m)
~1.1 MeV α-particles have a 6 mm rangehigher-energy alpha particle will not stop in the detector volume
IBM Research & IBM Systems and Technology Group
© 2010 IBM Corporation8 10/26/2011
The low-energy α-sourceWe need a low-energy α-source (so that the α’s stop in the active volume in the counter)We made an alpha-particle source from natural Samarium since it’s one of the lowest energy naturally-occurring α-particle emitterSm has 3 naturally-occurring α-emitting radioactive isotopes, – only 147Sm is important, due to the shorter ½ life compared to 148Sm, or 149Sm
0.01311.27E151.93148Sm
13.8
15
Abundance (%)
>1E16 (stable?)
1.07149Sm
8501.06E112.25147Sm
Specific activity
(α/sec-g)
½-life (years)
α-energy (MeV)
Sm Isotope
http://www.nndc.bnl.gov/chart/Chart of the Nuclides, GE, 13th ed.
)/()/(
(sec)2
2/1 molgAmolatomsNx
TLnSA =
IBM Research & IBM Systems and Technology Group
© 2010 IBM Corporation9 10/26/2011
Table of natural alpha-particle emitters and their energies
Source- unknown, yellowed sheet in my lab
IBM Research & IBM Systems and Technology Group
© 2010 IBM Corporation10 10/26/2011
0.1
1
10
100
0 1 2 3 4 5
Energy (MeV)
Cou
nts/
hr/
chan
nel
Energy spectrum from Sm source, in vacuum
measured spectrum
noisedifference
110310-sm-1
IBM Research & IBM Systems and Technology Group
© 2010 IBM Corporation11 10/26/2011
1
10
100
1000
10000
0 2 4 6 8 10
Energy (MeV)
Cou
nts/
hr/
chan
nel
Energy spectrum from 232Th source, in vacuum
measured spectrum
β’s, noise
difference
110218-232th-1
IBM Research & IBM Systems and Technology Group
© 2010 IBM Corporation12 10/26/2011
Alpha Sciences counter with Ortec discrete electronics
amp discrim. CAMACcounter
+HV
Charge-sensitivepreamp
Anode
CathodeSample/ tray
Using off-the-shelf electronics allows for easy adjustment and repair
MCA
Applied VoltagePul
se A
mpl
itude
Ion saturation
Propregion
Geigerregion
Applied Bias
1 MeV
2 MeV
From Knoll
Analytical formfor cylindrical geo.b
a)/ln(
)(abr
VrE =
For r=a, V=800V, E~106 V/m
IBM Research & IBM Systems and Technology Group
© 2010 IBM Corporation13 10/26/2011
Pulse-height spectrum from sources in the Alpha Sciences counter
0.01
0.1
1
10
100
1000
0 200 400 600 800 1000
Channel
Cou
nts/
hr/
chan
nel
0.01
0.1
1
10
100
1000
0 200 400 600 800 1000
Channel
Cou
nts/
hr/
chan
nel
Ultra-low activity sample
GC9-111024
A2110311-20.01
0.1
1
10
100
1000
0 200 400 600 800 1000
Channel
Cou
nts/
hr/
chan
nel
A2110311-1
Sm source 232Th source
noise
noise, β’s
IBM Research & IBM Systems and Technology Group
© 2010 IBM Corporation14 10/26/2011
Energy spectrum of Sm source, energy loss from sample through cathode
0.01
0.1
1
10
100
0 0.5 1 1.5 2 2.5 3
Energy (MeV)
Cpu
nts/
hr/
chan
nel
0.01
0.1
1
10
100
0 0.5 1 1.5 2 2.5 3
Energy (MeV)
Cpu
nts/
hr/
chan
nel
0.01
0.1
1
10
100
0 0.5 1 1.5 2 2.5 3
Energy (MeV)
Cpu
nts/
hr/
chan
nel
vacuum
air
air + mylar
2 mm gap
2.5 mm gap
3 mm gap
gap
~1 MeV energy lossin air and mylar- beforeα’s reach active area
IBM Research & IBM Systems and Technology Group
© 2010 IBM Corporation15 10/26/2011
Energy spectrum of 232Th source, energy loss from sample through cathode
0.1
1
10
100
1000
10000
100000
0 2 4 6 8 10
Energy (MeV)
Cou
nts/
hr/
chan
nel 2.5 mm gap, in vacuum
2.5 mm gap, air + mylar
Passage of the alphas in the gap and mylar causes reduction in maximum energy and in the flux
IBM Research & IBM Systems and Technology Group
© 2010 IBM Corporation16 10/26/2011
Results
Integrate the measured alpha particle energy spectrum from the samarium source, using the silicon detector, above a given threshold (eg E>0.25 MeV, E>0.5 MeV, E>0.75 MeV and E>1.0 MeV)
Repeat integration for each of the source-to-detector gaps
Plot the resulting integrated count rate vs energy
Integrate the count rate for the Alpha Sciences counter above a given ADC voltage threshold (eg V>0.5V, V>0.9V, V>1.5V,V >2.0V) using the discrete electronics
We can correlate the pulse height with energy- given the MCA spectrum from the Alpha Sciences counter, and the maximum energy in the alpha particle energy spectra
IBM Research & IBM Systems and Technology Group
© 2010 IBM Corporation17 10/26/2011
Results
0
50
100
150
200
250
300
350
400
450
0 0.5 1 1.5 2 2.5 3
Energy (MeV)
Cou
nts/
hr/
chan
nel
2 0
0
50
100
150
200
250
300
350
400
450
0 0.5 1 1.5 2 2.5 3
Energy (MeV)
Cou
nts/
hr/
chan
nel
2 0
0
50
100
150
200
250
300
350
400
450
0 0.5 1 1.5 2 2.5 3
Energy (MeV)
Cou
nts/
hr/
chan
nel
2 0
Si detector data
gas counter data2 mm gap
2.5 mm gap
3 mm gap
O.50.9
1.5
2.02.5
data from Si detector “fits” thegas counter data with a ~2.5 mm gap
0 count rate with this source is ~1-1.3 MeV
IBM Research & IBM Systems and Technology Group
© 2010 IBM Corporation18 10/26/2011
Response of Alpha Sciences counter, original electronics
55000
60000
65000
70000
75000
80000
0 0.05 0.1 0.15 0.2 0.25 0.3 0.35
Discriminator setting (V)
coun
ts/ h
r
Th source
A1111019
0
50
100
150
200
250
300
0 0.05 0.1 0.15 0.2 0.25 0.3 0.35
Discriminator setting (V)
coun
ts/ h
r
A1111018
Sm source
Zero count rate corresponds to a total energy loss of 2.25 MeV
Raising the discriminator level lowersthe detection efficiency (lowers the count rate) for a thick source
The slope of count rate vs discriminator setting, and the discriminatorsetting where the count rate goes to zero, will depend on the amplifier gain
IBM Research & IBM Systems and Technology Group
© 2010 IBM Corporation19 10/26/2011
Conclusion
– We have shown the energy spectrum from a low-energy Sm α-particle source.
– There is an appreciable energy-loss of low-energy α’s before they reach the active gas volume in the Alpha Sciences counters.
– While the discriminator can be set higher to reduce the background count rate, it cuts out the detection of low-energy α’s.
– The efficiency of detection in these counters is energy-dependent.
– What energy α’s are really important for samples that we measure?
– What is the α-particle energy associated with the discriminator setting on your Alpha Sciences counters?